Henri Poincaré#The three-body problem

{{Short description|French mathematician, physicist and engineer (1854–1912)}}

{{For|ships with this name|French ship Henri Poincaré}}

{{More citations needed|date=April 2016}}

{{Use dmy dates|date=November 2020}}

{{Infobox scientist

| name = Henri Poincaré

| other_names = Jules Henri Poincaré

| image = PSM V82 D416 Henri Poincare.png

| caption =

| birth_date = {{birth date|df=yes|1854|4|29}}

| birth_place = Nancy, Meurthe-et-Moselle, France

| death_date = {{death date and age|df=yes|1912|7|17|1854|4|29}}

| death_place = Paris, France

| relatives = Raymond Poincaré (cousin)
Lucien Poincaré (cousin)

| fields = {{flatlist|

}}

| spouse = Jeanne-Louise Poulain d'Andecy

| workplaces = {{plainlist|

| education = {{plainlist|

| thesis_title = Sur les propriétés des fonctions définies par les équations différences

| thesis_url = https://web.archive.org/web/20160506152142/https://iris.univ-lille1.fr/handle/1908/458

| thesis_year = 1879

| doctoral_advisor = Charles Hermite

| academic_advisors =

| doctoral_students = {{plainlist|

| notable_students = {{plainlist|

| known_for = {{collapsable list|

}}

| awards = {{plainlist|

| signature = Henri Poincaré Signature.svg

| footnotes = He was an uncle of Pierre Boutroux.

}}

{{special relativity sidebar}}

Jules Henri Poincaré{{Citation |last1=Heinzmann |first1=Gerhard |title=Henri Poincaré |date=2024 |encyclopedia=The Stanford Encyclopedia of Philosophy |editor-last=Zalta |editor-first=Edward N. |url=https://plato.stanford.edu/entries/poincare/ |access-date=2025-03-11 |edition=Summer 2024 |publisher=Metaphysics Research Lab, Stanford University |last2=Stump |first2=David |editor2-last=Nodelman |editor2-first=Uri}} ({{IPAc-en|UK|ˈ|p|w|æ̃|k|ɑr|eɪ}}, {{IPAc-en|US|ˌ|p|w|æ̃|k|ɑː|ˈ|r|eɪ}}; {{IPA|fr|ɑ̃ʁi pwɛ̃kaʁe|lang|Fr-Henri Poincaré.ogg}};{{Citation |title=Poincaré, n. |date=2023-03-02 |work=Oxford English Dictionary |url=https://oed.com/dictionary/poincare_n |access-date=2024-12-02 |edition=3 |publisher=Oxford University Press |language=en |doi=10.1093/oed/3697720964|url-access=subscription }} 29 April 1854{{snd}}17 July 1912) was a French mathematician, theoretical physicist, engineer, and philosopher of science. He is often described as a polymath, and in mathematics as "The Last Universalist",{{cite book |last1=Ginoux |first1=J. M. |title=Henri Poincaré: A Biography Through the Daily Papers |last2=Gerini |first2=C. |publisher=World Scientific |year=2013 |isbn=978-981-4556-61-3 |pages=vii–viii, xiii |doi=10.1142/8956}} since he excelled in all fields of the discipline as it existed during his lifetime. He has further been called "the Gauss of modern mathematics".{{Cite book |last=Folina |first=Janet |url=https://books.google.com/books?id=EPW-DAAAQBAJ&pg=PR12 |title=Poincaré and the Philosophy of Mathematics |date=1992 |publisher=Palgrave Macmillan UK |isbn=978-1-349-22121-9 |location=London |pages=xii |language=en |doi=10.1007/978-1-349-22119-6}} Due to his success in science, along with his influence and philosophy, he has been called "the philosopher par excellence of modern science".{{Cite book |last1=Moulton |first1=Forest Ray |author-link=Forest Ray Moulton |url=https://archive.org/details/autobiographyofs0000unse_n5k3/page/509 |title=The Autobiography of Science |last2=Jeffries |first2=Justus J. |publisher=Doubleday & Company |year=1945 |pages=509 |language=en}}

As a mathematician and physicist, he made many original fundamental contributions to pure and applied mathematics, mathematical physics, and celestial mechanics.{{cite journal|author=Hadamard, Jacques|author-link=Jacques Hadamard|title=The early scientific work of Henri Poincaré|journal=The Rice Institute Pamphlet|date=July 1922|volume=9|issue=3|pages=111–183|url=http://catalog.hathitrust.org/Record/100592035}} In his research on the three-body problem, Poincaré became the first person to discover a chaotic deterministic system which laid the foundations of modern chaos theory. Poincaré is regarded as the creator of the field of algebraic topology, and is further credited with introducing automorphic forms. He also made important contributions to algebraic geometry, number theory, complex analysis and Lie theory.{{Cite book |last=Gray |first=Jeremy |title=Henri Poincaré: A Scientific Biography |date=2013 |publisher=Princeton University Press |isbn=978-0-691-15271-4 |location= |pages=3, 16, 492 |language=en}} He famously introduced the concept of the Poincaré recurrence theorem, which states that a state will eventually return arbitrarily close to its initial state after a sufficiently long time, which has far-reaching consequences.{{Citation |last=Oxtoby |first=John C. |title=The Poincaré Recurrence Theorem |date=1980 |work=Measure and Category |series=Graduate Texts in Mathematics |volume=2 |pages=65–69 |url=http://link.springer.com/10.1007/978-1-4684-9339-9_17 |access-date=2024-12-01 |place=New York, NY |publisher=Springer New York |doi=10.1007/978-1-4684-9339-9_17 |isbn=978-1-4684-9341-2|url-access=subscription }} Early in the 20th century he formulated the Poincaré conjecture, which became, over time, one of the famous unsolved problems in mathematics. It was eventually solved in 2002–2003 by Grigori Perelman. Poincaré popularized the use of non-Euclidean geometry in mathematics as well.{{Citation |last1=Heinzmann |first1=Gerhard |title=Henri Poincaré |date=22 November 2021 |journal=Stanford Encyclopedia of Philosophy |pages= |url=https://plato.stanford.edu/entries/poincare/ |access-date=3 December 2024 |publisher=Stanford University |last2=Stump |first2=David}}

Poincaré made clear the importance of paying attention to the invariance of laws of physics under different transformations, and was the first to present the Lorentz transformations in their modern symmetrical form. Poincaré discovered the remaining relativistic velocity transformations and recorded them in a letter to Hendrik Lorentz in 1905. Thus he obtained perfect invariance of all of Maxwell's equations, an important step in the formulation of the theory of special relativity, for which he is also credited with laying down the foundations for, further writing foundational papers in 1905. He first proposed gravitational waves (ondes gravifiques) emanating from a body and propagating at the speed of light as being required by the Lorentz transformations, doing so in 1905.{{Cite journal |last1=Cervantes-Cota |first1=Jorge L. |last2=Galindo-Uribarri |first2=Salvador |last3=Smoot |first3=George F. |date=2016-09-13 |title=A Brief History of Gravitational Waves |journal=Universe |volume=2 |issue=3 |pages=22 |doi=10.3390/universe2030022 |issn=2218-1997|doi-access=free |arxiv=1609.09400 |bibcode=2016Univ....2...22C }} In 1912, he wrote an influential paper which provided a mathematical argument for quantum mechanics.{{Cite journal |last=Prentis |first=Jeffrey J. |date=1995-04-01 |title=Poincaré's proof of the quantum discontinuity of nature |url=https://pubs.aip.org/ajp/article/63/4/339/1043285/Poincare-s-proof-of-the-quantum-discontinuity-of |journal=American Journal of Physics |language=en |volume=63 |issue=4 |pages=339–350 |doi=10.1119/1.17919 |bibcode=1995AmJPh..63..339P |issn=0002-9505|url-access=subscription }} Poincaré also laid the seeds of the discovery of radioactivity through his interest and study of X-rays, which influenced physicist Henri Becquerel, who then discovered the phenomena.{{Cite journal |last1=Radvanyi |first1=Pierre |last2=Villain |first2=Jacques |date=2017-11-01 |title=The discovery of radioactivity |url=https://www.sciencedirect.com/science/article/pii/S1631070517300786 |journal=Comptes Rendus. Physique |language=en |volume=18 |issue=9–10 |pages=544–550 |doi=10.1016/j.crhy.2017.10.008 |bibcode=2017CRPhy..18..544R |issn=1878-1535|doi-access=free |url-access=subscription }} The Poincaré group used in physics and mathematics was named after him, after he introduced the notion of the group.{{Cite journal |last=Bacry |first=Henri |date=2004 |title=The foundations of the poincaré group and the validity of general relativity |url=https://linkinghub.elsevier.com/retrieve/pii/S0034487704900298 |journal=Reports on Mathematical Physics |language=en |volume=53 |issue=3 |pages=443–473 |doi=10.1016/S0034-4877(04)90029-8|bibcode=2004RpMP...53..443B |url-access=subscription }}

Poincaré was considered the dominant figure in mathematics and theoretical physics during his time, and was the most respected mathematician of his time, being described as "the living brain of the rational sciences" by mathematician Paul Painlevé.{{Cite book |last=Bell |first=E.T. |author-link=Eric Temple Bell |url=https://archive.org/details/in.ernet.dli.2015.59359/page/n295 |title=Men of Mathematics |publisher=Penguin Books |year=1937 |volume=II |pages=611 |language=en}} Philosopher Karl Popper regarded Poincaré as the greatest philosopher of science of all time,{{Cite book |url=https://books.google.com/books?id=9F7bY_ltzxIC&pg=PA373 |title=The Scientific Legacy of Poincaré |date=2010 |publisher=The London Mathematical Society |isbn=978-0-8218-4718-3 |editor-last=Charpentier |editor-first=Éric |series=History of Mathematics |location= |pages=373 |language=en |translator-last=Bowman |translator-first=Joshua |editor-last2=Ghys |editor-first2=E. |editor-last3=Lesne |editor-first3=Annick}} with Poincaré also originating the conventionalist view in science.{{Cite journal |last=Merritt |first=David |date=2017 |title=Cosmology and convention |url=https://linkinghub.elsevier.com/retrieve/pii/S1355219816301563 |journal=Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics |language=en |volume=57 |pages=41–52 |doi=10.1016/j.shpsb.2016.12.002|arxiv=1703.02389 |bibcode=2017SHPMP..57...41M }} Poincaré was a public intellectual in his time, and personally, he believed in political equality for all, while wary of the influence of anti-intellectual positions that the Catholic Church held at the time.{{Cite book |last=Gray |first=Jeremy |title=Henri Poincaré: A Scientific Biography |date=2013 |publisher=Princeton University Press |isbn=978-0-691-15271-4 |location= |pages=24, 201 |language=en}} He served as the president of the French Academy of Sciences (1906), the president of Société astronomique de France (1901–1903), and twice the president of Société mathématique de France (1886, 1900).

Life

Poincaré was born on 29 April 1854 in Cité Ducale neighborhood, Nancy, Meurthe-et-Moselle, into an influential French family.Belliver, 1956 His father {{ill|Léon Poincaré|fr}} (1828–1892) was a professor of medicine at the University of Nancy.Sagaret, 1911 His younger sister Aline married the spiritual philosopher Émile Boutroux. Another notable member of Henri's family was his cousin, Raymond Poincaré, a fellow member of the Académie française, who was President of France from 1913 to 1920, and three-time Prime Minister of France between 1913 and 1929.[http://www.utm.edu/research/iep/p/poincare.htm The Internet Encyclopedia of Philosophy] {{Webarchive|url=https://web.archive.org/web/20040202060803/http://www.utm.edu/research/iep/p/poincare.htm |date=2 February 2004 }} Jules Henri Poincaré article by Mauro Murzi – Retrieved November 2006.

=Education=

File:Henri Poincaré maison natale Nancy plaque.jpg

During his childhood he was seriously ill for a time with diphtheria and received special instruction from his mother, Eugénie Launois (1830–1897).

In 1862, Henri entered the Lycée in Nancy (now renamed the {{ill|Lycée Henri-Poincaré|fr}} in his honour, along with Henri Poincaré University, also in Nancy). He spent eleven years at the Lycée and during this time he proved to be one of the top students in every topic he studied. He excelled in written composition. His mathematics teacher described him as a "monster of mathematics" and he won first prizes in the concours général, a competition between the top pupils from all the Lycées across France. His poorest subjects were music and physical education, where he was described as "average at best".O'Connor et al., 2002 Poor eyesight and a tendency towards absentmindedness may explain these difficulties.Carl, 1968 He graduated from the Lycée in 1871 with a baccalauréat in both letters and sciences.

During the Franco-Prussian War of 1870, he served alongside his father in the Ambulance Corps.

Poincaré entered the École Polytechnique as the top qualifier in 1873 and graduated in 1875. There he studied mathematics as a student of Charles Hermite, continuing to excel and publishing his first paper (Démonstration nouvelle des propriétés de l'indicatrice d'une surface) in 1874. From November 1875 to June 1878 he studied at the École des Mines, while continuing the study of mathematics in addition to the mining engineering syllabus, and received the degree of ordinary mining engineer in March 1879.F. Verhulst

As a graduate of the École des Mines, he joined the Corps des Mines as an inspector for the Vesoul region in northeast France. He was on the scene of a mining disaster at Magny in August 1879 in which 18 miners died. He carried out the official investigation into the accident.

At the same time, Poincaré was preparing for his Doctorate in Science in mathematics under the supervision of Charles Hermite. His doctoral thesis was in the field of differential equations. It was named Sur les propriétés des fonctions définies par les équations aux différences partielles. Poincaré devised a new way of studying the properties of these equations. He not only faced the question of determining the integral of such equations, but also was the first person to study their general geometric properties. He realised that they could be used to model the behaviour of multiple bodies in free motion within the Solar System. He graduated from the University of Paris in 1879.

Image:Young Poincare.jpg

=First scientific achievements=

After receiving his degree, Poincaré began teaching as junior lecturer in mathematics at the University of Caen in Normandy (in December 1879). At the same time he published his first major article concerning the treatment of a class of automorphic functions.

There, in Caen, he met his future wife, Louise Poulain d'Andecy (1857–1934), granddaughter of Isidore Geoffroy Saint-Hilaire and great-granddaughter of Étienne Geoffroy Saint-Hilaire and on 20 April 1881, they married.{{Cite journal |last=Rollet |first=Laurent |date=2012-11-15 |title=Jeanne Louise Poulain d'Andecy, épouse Poincaré (1857–1934) |url=https://journals.openedition.org/sabix/1131 |journal=Bulletin de la SABIX |language=Fr |issue=51 |pages=18–27 |doi=10.4000/sabix.1131 |s2cid=190028919 |issn=0989-3059}} Together they had four children: Jeanne (born 1887), Yvonne (born 1889), Henriette (born 1891), and Léon (born 1893).

Poincaré immediately established himself among the greatest mathematicians of Europe, attracting the attention of many prominent mathematicians. In 1881 Poincaré was invited to take a teaching position at the Faculty of Sciences of the University of Paris; he accepted the invitation. During the years 1883 to 1897, he taught mathematical analysis in the École Polytechnique.

In 1881–1882, Poincaré created a new branch of mathematics: qualitative theory of differential equations. He showed how it is possible to derive the most important information about the behavior of a family of solutions without having to solve the equation (since this may not always be possible). He successfully used this approach to problems in celestial mechanics and mathematical physics.

=Career=

He never fully abandoned his career in the mining administration to mathematics. He worked at the Ministry of Public Services as an engineer in charge of northern railway development from 1881 to 1885. He eventually became chief engineer of the Corps des Mines in 1893 and inspector general in 1910.

Beginning in 1881 and for the rest of his career, he taught at the University of Paris (the Sorbonne). He was initially appointed as the maître de conférences d'analyse (associate professor of analysis).Sageret, 1911 Eventually, he held the chairs of Physical and Experimental Mechanics, Mathematical Physics and Theory of Probability,{{cite book|first =Laurent|last= Mazliak|chapter= Poincaré’s Odds |title = Poincaré 1912–2012 : Poincaré Seminar 2012|editor1-first= B.|editor1-last= Duplantier |editor2-first= V.|editor2-last= Rivasseau|volume = 67 |series = Progress in Mathematical Physics|publisher = Springer|isbn = 9783034808347|location = Basel|page = 150|url = https://books.google.com/books?id=njNpBQAAQBAJ|date= 14 November 2014}} and Celestial Mechanics and Astronomy.

In 1887, at the young age of 32, Poincaré was elected to the French Academy of Sciences. He became its president in 1906, and was elected to the Académie française on 5 March 1908.

In 1887, he won Oscar II, King of Sweden's mathematical competition for a resolution of the three-body problem concerning the free motion of multiple orbiting bodies. (See three-body problem section below.)

In 1893, Poincaré joined the French Bureau des Longitudes, which engaged him in the synchronisation of time around the world. In 1897 Poincaré backed an unsuccessful proposal for the decimalisation of circular measure, and hence time and longitude.see Galison 2003 It was this post which led him to consider the question of establishing international time zones and the synchronisation of time between bodies in relative motion. (See work on relativity section below.)

In 1904, he intervened in the trials of Alfred Dreyfus, attacking the spurious scientific claims regarding evidence brought against Dreyfus.

Poincaré was the President of the Société Astronomique de France (SAF), the French astronomical society, from 1901 to 1903.{{cite web| url = http://gallica.bnf.fr/ark:/12148/bpt6k9626551q/f616.item| title = Bulletin de la Société astronomique de France, 1911, vol. 25, pp. 581–586| year = 1911}}

==Students==

Poincaré had two notable doctoral students at the University of Paris, Louis Bachelier (1900) and Dimitrie Pompeiu (1905).[http://www.genealogy.ams.org/id.php?id=34227 Mathematics Genealogy Project] {{Webarchive|url=https://web.archive.org/web/20071005011853/http://www.genealogy.ams.org/id.php?id=34227 |date=5 October 2007 }} North Dakota State University. Retrieved April 2008.

= Death =

In 1912, Poincaré underwent surgery for a prostate problem and subsequently died from an embolism on 17 July 1912, in Paris. He was 58 years of age. He is buried in the Poincaré family vault in the Cemetery of Montparnasse, Paris, in section 16, close to the Rue Émile-Richard.

A former French Minister of Education, Claude Allègre, proposed in 2004 that Poincaré be reburied in the Panthéon in Paris, which is reserved for French citizens of the highest honour.{{cite web |url = http://www.lexpress.fr/idees/tribunes/dossier/allegre/dossier.asp?ida=430274 |title = Lorentz, Poincaré et Einstein |archive-url=https://web.archive.org/web/20041127160356/http://www.lexpress.fr/idees/tribunes/dossier/allegre/dossier.asp?ida=430274 |archive-date=27 November 2004 |url-status=dead}}File:Poincaré gravestone.jpg]]

Work

=Summary=

Poincaré made many contributions to different fields of pure and applied mathematics such as: celestial mechanics, fluid mechanics, optics, electricity, telegraphy, capillarity, elasticity, thermodynamics, potential theory, Quantum mechanics, theory of relativity and physical cosmology.

Among the specific topics he contributed to are the following:

=Three-body problem=

The problem of finding the general solution to the motion of more than two orbiting bodies in the Solar System had eluded mathematicians since Newton's time. This was known originally as the three-body problem and later the n-body problem, where n is any number of more than two orbiting bodies. The n-body solution was considered very important and challenging at the close of the 19th century. Indeed, in 1887, in honour of his 60th birthday, Oscar II, King of Sweden, advised by Gösta Mittag-Leffler, established a prize for anyone who could find the solution to the problem. The announcement was quite specific:

Given a system of arbitrarily many mass points that attract each according to Newton's law, under the assumption that no two points ever collide, try to find a representation of the coordinates of each point as a series in a variable that is some known function of time and for all of whose values the series converges uniformly.

In case the problem could not be solved, any other important contribution to classical mechanics would then be considered to be prizeworthy. The prize was finally awarded to Poincaré, even though he did not solve the original problem. One of the judges, the distinguished Karl Weierstrass, said, "This work cannot indeed be considered as furnishing the complete solution of the question proposed, but that it is nevertheless of such importance that its publication will inaugurate a new era in the history of celestial mechanics." (The first version of his contribution even contained a serious error; for details see the article by Diacu{{Citation

| last=Diacu|first= Florin | year=1996 | title=The solution of the n-body Problem | journal=The Mathematical Intelligencer | volume =18 | pages =66–70 | doi=10.1007/BF03024313

| issue=3|s2cid= 119728316 }} and the book by Barrow-Green{{Cite book|title=Poincaré and the three body problem|title-link= Poincaré and the Three-Body Problem |last=Barrow-Green|first=June|publisher=American Mathematical Society|year=1997|isbn=978-0821803677|location=Providence, RI|series=History of Mathematics|volume=11|oclc=34357985}}). The version finally printed{{Cite book|title=The three-body problem and the equations of dynamics: Poincaré's foundational work on dynamical systems theory|last=Poincaré|first=J. Henri|publisher=Springer International Publishing|others=Popp, Bruce D. (Translator)|year=2017|isbn=9783319528984|location=Cham, Switzerland|oclc=987302273}} contained many important ideas which led to the theory of chaos. The problem as stated originally was finally solved by Karl F. Sundman for n = 3 in 1912 and was generalised to the case of n > 3 bodies by Qiudong Wang in the 1990s. The series solutions have very slow convergence. It would take millions of terms to determine the motion of the particles for even very short intervals of time, so they are unusable in numerical work.

=Work on relativity=

{{Main|Lorentz ether theory|History of special relativity}}

Image:Curie and Poincare 1911 Solvay.jpg and Poincaré talk at the 1911 Solvay Conference.]]

==Local time==

Poincaré's work at the Bureau des Longitudes on establishing international time zones led him to consider how clocks at rest on the Earth, which would be moving at different speeds relative to absolute space (or the "luminiferous aether"), could be synchronised. At the same time Dutch theorist Hendrik Lorentz was developing Maxwell's theory into a theory of the motion of charged particles ("electrons" or "ions"), and their interaction with radiation. In 1895 Lorentz had introduced an auxiliary quantity (without physical interpretation) called "local time" t^\prime = t-v x/c^2 \,{{Citation|title=A broader view of relativity: general implications of Lorentz and Poincaré invariance|volume=10|first1=Jong-Ping|last1=Hsu|first2=Leonardo|last2=Hsu|publisher=World Scientific|year=2006|isbn=978-981-256-651-5|page=37

|url=https://books.google.com/books?id=amLqckyrvUwC}}, [https://books.google.com/books?id=amLqckyrvUwC&pg=PA37 Section A5a, p 37] and introduced the hypothesis of length contraction to explain the failure of optical and electrical experiments to detect motion relative to the aether (see Michelson–Morley experiment).{{Citation

| last=Lorentz|first= Hendrik A. | author-link=Hendrik Lorentz| year=1895 | title=Versuch einer theorie der electrischen und optischen erscheinungen in bewegten Kõrpern | place =Leiden| publisher=E.J. Brill| title-link=s:de:Versuch einer Theorie der electrischen und optischen Erscheinungen in bewegten Körpern }} Poincaré was a constant interpreter (and sometimes friendly critic) of Lorentz's theory. Poincaré as a philosopher was interested in the "deeper meaning". Thus he interpreted Lorentz's theory and in so doing he came up with many insights that are now associated with special relativity. In The Measure of Time (1898), Poincaré said, "A little reflection is sufficient to understand that all these affirmations have by themselves no meaning. They can have one only as the result of a convention." He also argued that scientists have to set the constancy of the speed of light as a postulate to give physical theories the simplest form.{{Citation

| last=Poincaré|first= Henri | year=1898 | title=The Measure of Time | journal=Revue de Métaphysique et de Morale | volume =6 | pages =1–13| title-link=s:The Measure of Time }}

Based on these assumptions he discussed in 1900 Lorentz's "wonderful invention" of local time and remarked that it arose when moving clocks are synchronised by exchanging light signals assumed to travel with the same speed in both directions in a moving frame.{{Citation

| last=Poincaré|first= Henri | year=1900 | title=La théorie de Lorentz et le principe de réaction | journal=Archives Néerlandaises des Sciences Exactes et Naturelles | volume =5 | pages =252–278| title-link=s:fr:La théorie de Lorentz et le principe de réaction }}. See also the [http://www.physicsinsights.org/poincare-1900.pdf English translation]

==Principle of relativity and Lorentz transformations==

{{Further|History of Lorentz transformations}}

In 1881 Poincaré described hyperbolic geometry in terms of the hyperboloid model, formulating transformations leaving invariant the Lorentz interval x^2+y^2-z^2=-1, which makes them mathematically equivalent to the Lorentz transformations in 2+1 dimensions.{{Cite journal|author=Poincaré, H.|year=1881|title=Sur les applications de la géométrie non-euclidienne à la théorie des formes quadratiques|journal=Association Française Pour l'Avancement des Sciences|volume=10|pages=132–138|url=http://henripoincarepapers.univ-nantes.fr/chp/hp-pdf/hp1881af.pdf|archive-url=https://web.archive.org/web/20200801124731/http://henripoincarepapers.univ-nantes.fr/chp/hp-pdf/hp1881af.pdf|url-status=dead|archive-date=1 August 2020}}{{Cite journal|author=Reynolds, W. F.|year=1993|title=Hyperbolic geometry on a hyperboloid|journal=The American Mathematical Monthly|volume=100|issue=5|pages=442–455|jstor=2324297|doi=10.1080/00029890.1993.11990430|s2cid=124088818 }} In addition, Poincaré's other models of hyperbolic geometry (Poincaré disk model, Poincaré half-plane model) as well as the Beltrami–Klein model can be related to the relativistic velocity space (see Gyrovector space).

In 1892 Poincaré developed a mathematical theory of light including polarization. His vision of the action of polarizers and retarders, acting on a sphere representing polarized states, is called the Poincaré sphere.{{Cite book|author=Poincaré, H. |year=1892|title=Théorie mathématique de la lumière II|location=Paris|publisher=Georges Carré|chapter-url=https://archive.org/details/thoriemathma00poin|chapter=Chapitre XII: Polarisation rotatoire}} It was shown that the Poincaré sphere possesses an underlying Lorentzian symmetry, by which it can be used as a geometrical representation of Lorentz transformations and velocity additions.{{Cite journal|author=Tudor, T.|year=2018|title=Lorentz Transformation, Poincaré Vectors and Poincaré Sphere in Various Branches of Physics|journal=Symmetry|volume=10|issue=3|pages=52|doi=10.3390/sym10030052|bibcode=2018Symm...10...52T|doi-access=free}}

He discussed the "principle of relative motion" in two papers in 1900{{Citation

| author=Poincaré, H. | year=1900 | title= Les relations entre la physique expérimentale et la physique mathématique | journal=Revue Générale des Sciences Pures et Appliquées | volume =11 | pages =1163–1175 | url=http://gallica.bnf.fr/ark:/12148/bpt6k17075r/f1167.table}}. Reprinted in "Science and Hypothesis", Ch. 9–10.

and named it the principle of relativity in 1904, according to which no physical experiment can discriminate between a state of uniform motion and a state of rest.{{Citation|author=Poincaré, Henri|year=1913|chapter=The Principles of Mathematical Physics|title=The Foundations of Science (The Value of Science)|pages=297–320|publisher=Science Press|place=New York|others= Article translated from 1904 original}} available in [https://books.google.com/books/about/The_Foundations_of_Science.html?id=mBvNabP35zoC&pg=PA297 online chapter from 1913 book]

In 1905 Poincaré wrote to Lorentz about Lorentz's paper of 1904, which Poincaré described as a "paper of supreme importance". In this letter he pointed out an error Lorentz had made when he had applied his transformation to one of Maxwell's equations, that for charge-occupied space, and also questioned the time dilation factor given by Lorentz.

{{Citation | author=Poincaré, H. | year=2007 | editor=Walter, S. A. | contribution= 38.3, Poincaré to H. A. Lorentz, May 1905 | title=La correspondance entre Henri Poincaré et les physiciens, chimistes, et ingénieurs |pages=255–257 |place=Basel | publisher=Birkhäuser|contribution-url=http://henripoincarepapers.univ-nantes.fr/chp/text/lorentz3.html}}

In a second letter to Lorentz, Poincaré gave his own reason why Lorentz's time dilation factor was indeed correct after all—it was necessary to make the Lorentz transformation form a group—and he gave what is now known as the relativistic velocity-addition law.{{Citation | author=Poincaré, H. | year=2007 | editor=Walter, S. A. | contribution= 38.4, Poincaré to H. A. Lorentz, May 1905 | title=La correspondance entre Henri Poincaré et les physiciens, chimistes, et ingénieurs |pages=257–258 |place=Basel | publisher=Birkhäuser|contribution-url=http://henripoincarepapers.univ-nantes.fr/chp/text/lorentz4.html}}

Poincaré later delivered a paper at the meeting of the Academy of Sciences in Paris on 5 June 1905 in which these issues were addressed. In the published version of that he wrote:[http://www.academie-sciences.fr/pdf/dossiers/Poincare/Poincare_pdf/Poincare_CR1905.pdf] (PDF) Membres de l'Académie des sciences depuis sa création : Henri Poincare. Sur la dynamique de l' electron. Note de H. Poincaré. C.R. T.140 (1905) 1504–1508.

The essential point, established by Lorentz, is that the equations of the electromagnetic field are not altered by a certain transformation (which I will call by the name of Lorentz) of the form:

::x^\prime = k\ell\left(x + \varepsilon t\right)\!,\;t^\prime = k\ell\left(t + \varepsilon x\right)\!,\;y^\prime = \ell y,\;z^\prime = \ell z,\;k = 1/\sqrt{1-\varepsilon^2}.

and showed that the arbitrary function \ell\left(\varepsilon\right) must be unity for all \varepsilon (Lorentz had set \ell = 1 by a different argument) to make the transformations form a group. In an enlarged version of the paper that appeared in 1906 Poincaré pointed out that the combination x^2+ y^2+ z^2- c^2t^2 is invariant. He noted that a Lorentz transformation is merely a rotation in four-dimensional space about the origin by introducing ct\sqrt{-1} as a fourth imaginary coordinate, and he used an early form of four-vectors.{{Citation

| author=Poincaré, H. | year=1906 | title=Sur la dynamique de l'électron (On the Dynamics of the Electron) | journal=Rendiconti del Circolo Matematico Rendiconti del Circolo di Palermo | volume =21 | pages =129–176

| doi=10.1007/BF03013466| bibcode=1906RCMP...21..129P| hdl=2027/uiug.30112063899089 | s2cid=120211823 | url=https://zenodo.org/record/1428444| hdl-access=free }} (Wikisource translation) Poincaré expressed a lack of interest in a four-dimensional reformulation of his new mechanics in 1907, because in his opinion the translation of physics into the language of four-dimensional geometry would entail too much effort for limited profit.{{cite book | last=Walter | first=Scott | title=The Genesis of General Relativity | chapter=Breaking in the 4-Vectors: The Four-Dimensional Movement in Gravitation, 1905–1910 |volume=3| publisher=Springer Netherlands |publication-place=Dordrecht | date=2007 | isbn=978-1-4020-3999-7 | doi=10.1007/978-1-4020-4000-9_18 | pages=1118–1178}} So it was Hermann Minkowski who worked out the consequences of this notion in 1907.{{cite journal | last = Minkowski | first = Hermann | date = September 1908 | title = Raum und Zeit | url = https://math.nyu.edu/~tschinke/papers/yuri/14minkowski/raum-und-zeit.pdf | journal = Jahresbericht der Deutschen Mathematiker-Vereinigung | volume = 18 | pages = 75–88 | access-date=11 May 2024 }}

==Mass–energy relation==

Like others before, Poincaré (1900) discovered a relation between mass and electromagnetic energy. While studying the conflict between the action/reaction principle and Lorentz ether theory, he tried to determine whether the center of gravity still moves with a uniform velocity when electromagnetic fields are included. He noticed that the action/reaction principle does not hold for matter alone, but that the electromagnetic field has its own momentum. Poincaré concluded that the electromagnetic field energy of an electromagnetic wave behaves like a fictitious fluid (fluide fictif) with a mass density of E/c2. If the center of mass frame is defined by both the mass of matter and the mass of the fictitious fluid, and if the fictitious fluid is indestructible—it's neither created or destroyed—then the motion of the center of mass frame remains uniform. But electromagnetic energy can be converted into other forms of energy. So Poincaré assumed that there exists a non-electric energy fluid at each point of space, into which electromagnetic energy can be transformed and which also carries a mass proportional to the energy. In this way, the motion of the center of mass remains uniform. Poincaré said that one should not be too surprised by these assumptions, since they are only mathematical fictions.

However, Poincaré's resolution led to a paradox when changing frames: if a Hertzian oscillator radiates in a certain direction, it will suffer a recoil from the inertia of the fictitious fluid. Poincaré performed a Lorentz boost (to order v/c) to the frame of the moving source. He noted that energy conservation holds in both frames, but that the law of conservation of momentum is violated. This would allow perpetual motion, a notion which he abhorred. The laws of nature would have to be different in the frames of reference, and the relativity principle would not hold. Therefore, he argued that also in this case there has to be another compensating mechanism in the ether.

Poincaré himself came back to this topic in his St. Louis lecture (1904). He rejectedMiller 1981, Secondary sources on relativity the possibility that energy carries mass and criticized his own solution to compensate the above-mentioned problems:

{{blockquote|The apparatus will recoil as if it were a cannon and the projected energy a ball, and that contradicts the principle of Newton, since our present projectile has no mass; it is not matter, it is energy. [..] Shall we say that the space which separates the oscillator from the receiver and which the disturbance must traverse in passing from one to the other, is not empty, but is filled not only with ether, but with air, or even in inter-planetary space with some subtile, yet ponderable fluid; that this matter receives the shock, as does the receiver, at the moment the energy reaches it, and recoils, when the disturbance leaves it? That would save Newton's principle, but it is not true. If the energy during its propagation remained always attached to some material substratum, this matter would carry the light along with it and Fizeau has shown, at least for the air, that there is nothing of the kind. Michelson and Morley have since confirmed this. We might also suppose that the motions of matter proper were exactly compensated by those of the ether; but that would lead us to the same considerations as those made a moment ago. The principle, if thus interpreted, could explain anything, since whatever the visible motions we could imagine hypothetical motions to compensate them. But if it can explain anything, it will allow us to foretell nothing; it will not allow us to choose between the various possible hypotheses, since it explains everything in advance. It therefore becomes useless. }}

In the above quote he refers to the Hertz assumption of total aether entrainment that was falsified by the Fizeau experiment but that experiment does indeed show that light is partially "carried along" with a substance. Finally in 1908{{cite book

|author=Poincaré, Henri

|year=1908–1913

|title=The foundations of science (Science and Method)

|chapter=The New Mechanics

|location=New York |publisher=Science Press

|pages=486–522}} he revisits the problem and ends with abandoning the principle of reaction altogether in favor of supporting a solution based in the inertia of aether itself.

{{blockquote|But we have seen above that Fizeau's experiment does not permit of our retaining the theory of Hertz; it is necessary therefore to adopt the theory of Lorentz, and consequently to renounce the principle of reaction. }}

He also discussed two other unexplained effects: (1) non-conservation of mass implied by Lorentz's variable mass \gamma m, Abraham's theory of variable mass and Kaufmann's experiments on the mass of fast moving electrons and (2) the non-conservation of energy in the radium experiments of Marie Curie.

It was Albert Einstein's concept of mass–energy equivalence (1905) that a body losing energy as radiation or heat was losing mass of amount m = E/c2 that resolvedDarrigol 2005, Secondary sources on relativity Poincaré's paradox, without using any compensating mechanism within the ether.{{Citation|author=Einstein, A. |year=1905b |title=Ist die Trägheit eines Körpers von dessen Energieinhalt abhängig? |journal=Annalen der Physik |volume=18 |issue=13 |pages=639–643 |bibcode=1905AnP...323..639E |doi= 10.1002/andp.19053231314 |doi-access=free }}. See also [http://www.fourmilab.ch/etexts/einstein/specrel/www English translation]. The Hertzian oscillator loses mass in the emission process, and momentum is conserved in any frame. However, concerning Poincaré's solution of the Center of Gravity problem, Einstein noted that Poincaré's formulation and his own from 1906 were mathematically equivalent.{{Citation|author=Einstein, A. |year=1906 |title=Das Prinzip von der Erhaltung der Schwerpunktsbewegung und die Trägheit der Energie |journal=Annalen der Physik |volume=20 |pages=627–633 |doi=10.1002/andp.19063250814 |issue=8 |bibcode=1906AnP...325..627E |s2cid=120361282 |url= http://www.physik.uni-augsburg.de/annalen/history/papers/1906_20_627-633.pdf |archive-url=https://web.archive.org/web/20060318060830/http://www.physik.uni-augsburg.de/annalen/history/papers/1906_20_627-633.pdf |url-status=dead |archive-date=18 March 2006}}

==Gravitational waves==

In 1905 Poincaré first proposed gravitational waves (ondes gravifiques) emanating from a body and propagating at the speed of light. He wrote:

{{blockquote|It has become important to examine this hypothesis more closely and in particular to ask in what ways it would require us to modify the laws of gravitation. That is what I have tried to determine; at first I was led to assume that the propagation of gravitation is not instantaneous, but happens with the speed of light."Il importait d'examiner cette hypothèse de plus près et en particulier de rechercher quelles modifications elle nous obligerait à apporter aux lois de la gravitation. C'est ce que j'ai cherché à déterminer; j'ai été d'abord conduit à supposer que la propagation de la gravitation n'est pas instantanée, mais se fait avec la vitesse de la lumière."}}

==Poincaré and Einstein==

Einstein's first paper on relativity was published three months after Poincaré's short paper, but before Poincaré's longer version. Einstein relied on the principle of relativity to derive the Lorentz transformations and used a similar clock synchronisation procedure (Einstein synchronisation) to the one that Poincaré (1900) had described, but Einstein's paper was remarkable in that it contained no references at all. Poincaré never acknowledged Einstein's work on special relativity. However, Einstein expressed sympathy with Poincaré's outlook obliquely in a letter to Hans Vaihinger on 3 May 1919, when Einstein considered Vaihinger's general outlook to be close to his own and Poincaré's to be close to Vaihinger's.{{cite book|series=The Collected Papers of Albert Einstein |url=http://einsteinpapers.press.princeton.edu/vol9-trans/52 |publisher=Princeton U.P. |volume = 9|title = The Berlin Years: Correspondence, January 1919 – April 1920 (English translation supplement)|page = 30}} See also this letter, with commentary, in {{cite journal |last=Sass |first=Hans-Martin | author-link = Hans-Martin Sass|date=1979 |title=Einstein über "wahre Kultur" und die Stellung der Geometrie im Wissenschaftssystem: Ein Brief Albert Einsteins an Hans Vaihinger vom Jahre 1919 |journal=Zeitschrift für allgemeine Wissenschaftstheorie |volume=10 |issue=2 |pages=316–319 |jstor=25170513 |language=de |doi=10.1007/bf01802352|s2cid=170178963 }} In public, Einstein acknowledged Poincaré posthumously in the text of a lecture in 1921 titled "Geometrie und Erfahrung (Geometry and Experience)" in connection with non-Euclidean geometry, but not in connection with special relativity. A few years before his death, Einstein commented on Poincaré as being one of the pioneers of relativity, saying "Lorentz had already recognized that the transformation named after him is essential for the analysis of Maxwell's equations, and Poincaré deepened this insight still further ....".Darrigol 2004, Secondary sources on relativity

==Assessments on Poincaré and relativity==

{{Further|History of special relativity|Relativity priority dispute}}

Poincaré's work in the development of special relativity is well recognised, though most historians stress that despite many similarities with Einstein's work, the two had very different research agendas and interpretations of the work.Galison 2003 and Kragh 1999, Secondary sources on relativity Poincaré developed a similar physical interpretation of local time and noticed the connection to signal velocity, but contrary to Einstein he continued to use the ether-concept in his papers and argued that clocks at rest in the ether show the "true" time, and moving clocks show the local time. So Poincaré tried to keep the relativity principle in accordance with classical concepts, while Einstein developed a mathematically equivalent kinematics based on the new physical concepts of the relativity of space and time.Holton (1988), 196–206{{cite thesis |last=Hentschel|first=Klaus |date=1990 |title=Interpretationen und Fehlinterpretationen der speziellen und der allgemeinen Relativitätstheorie durch Zeitgenossen Albert Einsteins |degree=PhD |publisher=University of Hamburg|pages=3–13}}Miller (1981), 216–217Darrigol (2005), 15–18Katzir (2005), 286–288

While this is the view of most historians, a minority go much further, such as E. T. Whittaker, who held that Poincaré and Lorentz were the true discoverers of relativity.Whittaker 1953, Secondary sources on relativity

=Algebra and number theory=

Poincaré introduced group theory to physics, and was the first to study the group of Lorentz transformations.Poincaré, Selected works in three volumes. page = 682{{full citation needed|date=September 2019}}{{cite journal | last = Poincaré | first = Henri | date = 1905 | title = Sur la dynamique de l'électron | journal = Comptes rendus des séances de l'Académie des Sciences | volume = 140 | pages = 1504–1508 }} He also made major contributions to the theory of discrete groups and their representations.

Image:Mug and Torus morph.gif

File:Poincaré-7.jpg

=Topology=

The subject is clearly defined by Felix Klein in his "Erlangen Program" (1872): the geometry invariants of arbitrary continuous transformation, a kind of geometry. The term "topology" was introduced, as suggested by Johann Benedict Listing, instead of previously used "Analysis situs". Some important concepts were introduced by Enrico Betti and Bernhard Riemann. But the foundation of this science, for a space of any dimension, was created by Poincaré. His first article on this topic appeared in 1894.{{sfn|Stillwell|2010|pp=419–435}}

His research in geometry led to the abstract topological definition of homotopy and homology. He also first introduced the basic concepts and invariants of combinatorial topology, such as Betti numbers and the fundamental group. Poincaré proved a formula relating the number of edges, vertices and faces of n-dimensional polyhedron (the Euler–Poincaré theorem) and gave the first precise formulation of the intuitive notion of dimension.{{cite journal | last=Aleksandrov | first=P S | title=Poincaré and topology | journal=Russian Mathematical Surveys | volume=27 | issue=1 | date=28 February 1972 | issn=0036-0279 | doi=10.1070/RM1972v027n01ABEH001365 | pages=157–168| bibcode=1972RuMaS..27..157A }}

=Astronomy and celestial mechanics=

File:N-body problem (3).gif

Poincaré published two now classical monographs, "New Methods of Celestial Mechanics" (1892–1899) and "Lectures on Celestial Mechanics" (1905–1910). In them, he successfully applied the results of their research to the problem of the motion of three bodies and studied in detail the behavior of solutions (frequency, stability, asymptotic, and so on). They introduced the small parameter method, fixed points, integral invariants, variational equations, the convergence of the asymptotic expansions. Generalizing a theory of Bruns (1887), Poincaré showed that the three-body problem is not integrable. In other words, the general solution of the three-body problem can not be expressed in terms of algebraic and transcendental functions through unambiguous coordinates and velocities of the bodies. His work in this area was the first major achievement in celestial mechanics since Isaac Newton.J. Stillwell, Mathematics and its history, [https://books.google.com/books?id=V7mxZqjs5yUC&pg=PA254 p. 254]

These monographs include an idea of Poincaré, which later became the basis for mathematical "chaos theory" (see, in particular, the Poincaré recurrence theorem) and the general theory of dynamical systems.

Poincaré authored important works on astronomy for the equilibrium figures of a gravitating rotating fluid. He introduced the important concept of bifurcation points and proved the existence of equilibrium figures such as the non-ellipsoids, including ring-shaped and pear-shaped figures, and their stability. For this discovery, Poincaré received the Gold Medal of the Royal Astronomical Society (1900).{{cite journal |author-last=Darwin | author-first=G.H.| title=Address Delivered by the President, Professor G. H. Darwin, on presenting the Gold Medal of the Society to M. H. Poincaré | journal=Monthly Notices of the Royal Astronomical Society | volume=60 | issue=5 | date=1900 | issn=0035-8711 | doi=10.1093/mnras/60.5.406 | pages=406–416| doi-access=free}}

=Differential equations and mathematical physics=

After defending his doctoral thesis on the study of singular points of the system of differential equations, Poincaré wrote a series of memoirs under the title "On curves defined by differential equations" (1881–1882).French: "Mémoire sur les courbes définies par une équation différentielle" In these articles, he built a new branch of mathematics, called "qualitative theory of differential equations". Poincaré showed that even if the differential equation can not be solved in terms of known functions, yet from the very form of the equation, a wealth of information about the properties and behavior of the solutions can be found. In particular, Poincaré investigated the nature of the trajectories of the integral curves in the plane, gave a classification of singular points (saddle, focus, center, node), introduced the concept of a limit cycle and the loop index, and showed that the number of limit cycles is always finite, except for some special cases. Poincaré also developed a general theory of integral invariants and solutions of the variational equations. For the finite-difference equations, he created a new direction – the asymptotic analysis of the solutions. He applied all these achievements to study practical problems of mathematical physics and celestial mechanics, and the methods used were the basis of its topological works.{{cite book|editor1-last=Kolmogorov|editor1-first = A.N.|editor2-first = A.P.|editor2-last= Yushkevich|title = Mathematics of the 19th century |volume= 3| pages = 162–174, 283|isbn= 978-3764358457|date = 24 March 1998| publisher=Springer }}

File: Phase Portrait Sadle.svg | Saddle

File: Phase Portrait Stable Focus.svg | Focus

File: Phase portrait center.svg | Center

File: Phase Portrait Stable Node.svg | Node

Character

File:Henri Poincaré by H Manuel.jpg

Poincaré's work habits have been compared to a bee flying from flower to flower. Poincaré was interested in the way his mind worked; he studied his habits and gave a talk about his observations in 1908 at the Institute of General Psychology in Paris. He linked his way of thinking to how he made several discoveries.

The mathematician Darboux claimed he was un intuitif (an intuitive), arguing that this is demonstrated by the fact that he worked so often by visual representation. Jacques Hadamard wrote that Poincaré's research demonstrated marvelous clarityJ. Hadamard. L'oeuvre de H. Poincaré. Acta Mathematica, 38 (1921), p. 208 and Poincaré himself wrote that he believed that logic was not a way to invent but a way to structure ideas and that logic limits ideas.

=Toulouse's characterisation=

Poincaré's mental organisation was interesting not only to Poincaré himself but also to Édouard Toulouse, a psychologist of the Psychology Laboratory of the School of Higher Studies in Paris. Toulouse wrote a book entitled Henri Poincaré (1910).{{cite book| url = http://name.umdl.umich.edu/AAS9989.0001.001| title = Toulouse, Édouard, 1910. Henri Poincaré, E. Flammarion, Paris| year = 2005}}{{cite book|title=Henri Poincare|author=Toulouse, E.|date=2013|publisher=MPublishing|isbn=9781418165062|url=https://books.google.com/books?id=mpjWPQAACAAJ|access-date=10 October 2014}} In it, he discussed Poincaré's regular schedule:

  • He worked during the same times each day in short periods of time. He undertook mathematical research for four hours a day, between 10 a.m. and noon then again from 5 p.m. to 7 p.m.. He would read articles in journals later in the evening.
  • His normal work habit was to solve a problem completely in his head, then commit the completed problem to paper.
  • He was ambidextrous and nearsighted.
  • His ability to visualise what he heard proved particularly useful when he attended lectures, since his eyesight was so poor that he could not see properly what the lecturer wrote on the blackboard.

These abilities were offset to some extent by his shortcomings:

In addition, Toulouse stated that most mathematicians worked from principles already established while Poincaré started from basic principles each time (O'Connor et al., 2002).

His method of thinking is well summarised as:

{{blockquote|text=Habitué à négliger les détails et à ne regarder que les cimes, il passait de l'une à l'autre avec une promptitude surprenante et les faits qu'il découvrait se groupant d'eux-mêmes autour de leur centre étaient instantanément et automatiquement classés dans sa mémoire (accustomed to neglecting details and to looking only at mountain tops, he went from one peak to another with surprising rapidity, and the facts he discovered, clustering around their center, were instantly and automatically pigeonholed in his memory).|sign=Belliver (1956)}}

Publications

  • {{Cite book|title=Leçons sur la théorie mathématique de la lumière|volume=|publisher=Carrè|location=Paris|year=1889|language=fr|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=6569792}}
  • {{Cite book|title=Solutions periodiques, non-existence des integrales uniformes, solutions asymptotiques|volume=1|publisher=Gauthier-Villars|location=Paris|year=1892|language=fr|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=10996590}}
  • {{Cite book|title=Methodes de mm. Newcomb, Gylden, Lindstedt et Bohlin|volume=2|publisher=Gauthier-Villars|location=Paris|year=1893|language=fr|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=10997817}}
  • {{Cite book|title=Oscillations électriques|volume=|publisher=Carrè|location=Paris|year=1894|language=fr|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=6571067}}
  • {{Cite book|title=Invariants integraux, solutions periodiques du deuxieme genre, solutions doublement asymptotiques|volume=3|publisher=Gauthier-Villars|location=Paris|year=1899|language=fr|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=10999338}}
  • {{Cite book|title=Valeur de la science|volume=|publisher=Flammarion|location=Paris|year=1900|language=fr|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=3901099}}
  • {{Cite book|title=Electricité et optique|volume=|publisher=Carrè & Naud|location=Paris|year=1901|language=fr|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=7156481}}
  • {{Cite book|title=Science et l'hypothèse|volume=|publisher=Flammarion|location=Paris|year=1902|language=fr|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=3901686}}
  • {{Cite book|title=Thermodynamique|volume=|publisher=Gauthier-Villars|location=Paris|year=1908|language=fr|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=6568325}}
  • {{Cite book|title=Dernières pensées|volume=|publisher=Flammarion|location=Paris|year=1913|language=fr|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=3902281}}
  • {{Cite book|title=Science et méthode|volume=|publisher=Nelson and Sons|location=London|year=1914|language=en|url=https://gutenberg.beic.it/webclient/DeliveryManager?pid=10947130}}

Legacy

Poincaré is credited with laying the foundations of special relativity,{{Citation |last=Marchal |first=C. |title=Henri Poincaré: A Decisive Contribution to Special Relativity |date=1997 |work=The Dynamical Behaviour of our Planetary System |pages=403–413 |editor-last=Dvorak |editor-first=R. |url=http://link.springer.com/10.1007/978-94-011-5510-6_30 |access-date=2024-12-02 |place=Dordrecht |publisher=Springer Netherlands |language=en |doi=10.1007/978-94-011-5510-6_30 |isbn=978-94-010-6320-3 |editor2-last=Henrard |editor2-first=J.|url-access=subscription }}{{Cite book |last=Ginoux |first=Jean-Marc |url=https://books.google.com/books?id=MI4CEQAAQBAJ&pg=PA47 |title=Poincaré, Einstein and the Discovery of Special Relativity: An End to the Controversy |date=2024 |publisher=Springer |isbn=978-3-031-51386-2 |series=History of Physics |location= |pages=47 |language=en}} with some arguing that he should be credited with its creation.{{Citation |last=Logunov |first=A. A. |title=Henri Poincare and Relativity Theory |date=2004 |pages=3, 63, 187 |arxiv=physics/0408077 |bibcode=2004physics...8077L |author-link=Anatoly Logunov}} He is said to have "dominated the mathematics and the theoretical physics of his time", and that "he was without a doubt the most admired mathematician while he was alive, and he remains today one of the world's most emblematic scientific figures."{{Cite book |url=https://books.google.com/books?id=9F7bY_ltzxIC&pg=PA1 |title=The Scientific Legacy of Poincaré |date=2010 |publisher=The London Mathematical Society |isbn=978-0-8218-4718-3 |editor-last=Charpentier |editor-first=Éric |series=History of Mathematics |location= |pages=1–2 |language=en |translator-last=Bowman |translator-first=Joshua |editor-last2=Ghys |editor-first2=E. |editor-last3=Lesne |editor-first3=Annick}} Poincaré is regarded as a "universal specialist", as he refined celestial mechanics, he progressed nearly all parts of mathematics of his time, including creating new subjects, is a father of special relativity, participated in all the great debates of his time in physics, was a major actor in the great epistemological debates of his day in relation to philosophy of science, and Poincaré was the one who investigated the 1879 Magny shaft firedamp explosion as an engineer. Due to the breadth of his research, Poincaré was the only member to be elected to every section of the French Academy of Sciences of the time, those being geometry, mechanics, physics, astronomy and navigation.{{Cite book |last=Krantz |first=Steven G. |url=https://books.google.com/books?id=ulmAH-6IzNoC&pg=PA291 |title=An Episodic History of Mathematics: Mathematical Culture Through Problem Solving |date=2010 |publisher=Mathematical Association of America |isbn=978-0-88385-766-3 |series= |location=Washington, DC |pages=291 |language=en |oclc=501976977}}

Physicist Henri Becquerel nominated Poincaré for a Nobel Prize in 1904, as Becquerel took note that "Poincaré's mathematical and philosophical genius surveyed all of physics and was among those that contributed most to human progress by giving researchers a solid basis for their journeys into the unknown."{{Cite book |last=Gray |first=Jeremy |title=Henri Poincaré: A Scientific Biography |date=2013 |publisher=Princeton University Press |isbn=978-0-691-15271-4 |location= |pages=195 |language=en}} After his death, he was praised by many intellectual figures of his time, as the author Marie Bonaparte wrote to his widowed wife Louise that "He was – as you know better than anyone – not only the greatest thinker, the most powerful genius of our time – but also a deep and incomparable heart; and having been close to him remains the precious memory of a whole life."{{Cite journal |last=Rollet |first=Laurent |date=2023-06-19 |title="My sincere condolences" |url=https://euromathsoc.org/magazine/articles/141 |journal=European Mathematical Society Magazine |issue=128 |pages=41–50 |doi=10.4171/mag/141 |issn=2747-7894|doi-access=free }}

Mathematician E.T. Bell titled Poincaré as "The Last Universalist", and noted his prowess in many fields, stating that:{{Cite book |last=Bell |first=E.T. |author-link=Eric Temple Bell |title=Men of Mathematics |publisher=Penguin Books |year=1937 |volume=II |pages=581, 584 |language=en}}

{{blockquote|Poincaré was the last man to take practically all mathematics, both pure and applied, as his province . . . few mathematicians have had the breadth of philosophical vision that Poincaré had and none is his superior in the gift of clear exposition.}}

When philosopher and mathematician Bertrand Russell was asked who was the greatest man that France had produced in modern times, he instantly replied "Poincaré". Bell noted that if Poincaré had been as strong in practical science as he was in theoretical, he might have "made a fourth with the incomparable three, Archimedes, Newton, and Gauss."

Bell further noted his powerful memory, one that was even superior to Leonhard Euler's, stating that:{{Cite book |last=Bell |first=E.T. |author-link=Eric Temple Bell |title=Men of Mathematics |publisher=Penguin Books |year=1937 |volume=II |pages=587 |language=en}}

{{blockquote|His principal diversion was reading, where his unusual talents first showed up. A book once read - at incredible speed - became a permanent possession, and he could always state the page and line where a particular thing occurred. He retained this powerful memory all his life. This rare faculty, which Poincaré shared with Euler who had it in a lesser degree, might be called visual or spatial memory. In temporal memory - the ability to recall with uncanny precision a sequence of events long passed — he was also unusually strong.}}

Bell notes the terrible eyesight of Poincaré, he almost completely remembered formulas and theorems by ear, and "unable to see the board distinctly when he became a student of advanced mathematics, he sat back and listened, following and remembering perfectly without taking notes - an easy feat for him, but one incomprehensible to most mathematicians."

Honours

Awards

Named after him

Henri Poincaré did not receive the Nobel Prize in Physics, but he had influential advocates like Henri Becquerel or committee member Gösta Mittag-Leffler.{{cite book|last1=Gray|first1=Jeremy|title=Henri Poincaré: A Scientific Biography|date=2013|publisher=Princeton University Press|pages=194–196|chapter=The Campaign for Poincaré}}{{cite book|last1=Crawford|first1=Elizabeth|title=The Beginnings of the Nobel Institution: The Science Prizes, 1901–1915|year= 1987|publisher=Cambridge University Press|pages=141–142}} The nomination archive reveals that Poincaré received a total of 51 nominations between 1904 and 1912, the year of his death.{{cite web|title=Nomination database|url=https://www.nobelprize.org/nomination/archive/list.php|website=Nobelprize.org|publisher=Nobel Media AB|access-date=24 September 2015}} Of the 58 nominations for the 1910 Nobel Prize, 34 named Poincaré. Nominators included Nobel laureates Hendrik Lorentz and Pieter Zeeman (both of 1902), Marie Curie (of 1903), Albert Michelson (of 1907), Gabriel Lippmann (of 1908) and Guglielmo Marconi (of 1909).

The fact that renowned theoretical physicists like Poincaré, Boltzmann or Gibbs were not awarded the Nobel Prize is seen as evidence that the Nobel committee had more regard for experimentation than theory.{{cite journal|last1=Crawford |first1= Elizabeth |title=Nobel: Always the Winners, Never the Losers|journal=Science|date=13 November 1998|volume=282|issue=5392|pages=1256–1257|doi=10.1126/science.282.5392.1256|bibcode = 1998Sci...282.1256C |s2cid= 153619456 }}{{dead link|date=July 2016}}{{cite journal|last1=Nastasi|first1=Pietro|title=A Nobel Prize for Poincaré? |journal=Lettera Matematica|date=16 May 2013|volume=1|issue=1–2|pages=79–82|doi=10.1007/s40329-013-0005-1 |doi-access=free}} In Poincaré's case, several of those who nominated him pointed out that the greatest problem was to name a specific discovery, invention, or technique.

Philosophy

File:Poincaré-16.jpg

Poincaré had philosophical views opposite to those of Bertrand Russell and Gottlob Frege, who believed that mathematics was a branch of logic. Poincaré strongly disagreed, claiming that intuition was the life of mathematics. Poincaré gives an interesting point of view in his 1902 book Science and Hypothesis:

{{blockquote|text=For a superficial observer, scientific truth is beyond the possibility of doubt; the logic of science is infallible, and if the scientists are sometimes mistaken, this is only from their mistaking its rule.}}

Poincaré believed that arithmetic is synthetic. He argued that Peano's axioms cannot be proven non-circularly with the principle of induction (Murzi, 1998), therefore concluding that arithmetic is a priori synthetic and not analytic. Poincaré then went on to say that mathematics cannot be deduced from logic since it is not analytic. His views were similar to those of Immanuel Kant (Kolak, 2001, Folina 1992). He strongly opposed Cantorian set theory, objecting to its use of impredicative definitions.{{Cite book |last=Folina |first=Janet |url=https://books.google.com/books?id=EPW-DAAAQBAJ&pg=PA145 |title=Poincaré and the Philosophy of Mathematics |date=1992 |publisher=Palgrave Macmillan UK |isbn=978-1-349-22121-9 |location=London |pages=145 |language=en |doi=10.1007/978-1-349-22119-6}}

However, Poincaré did not share Kantian views in all branches of philosophy and mathematics. For example, in geometry, Poincaré believed that the structure of non-Euclidean space can be known analytically. Poincaré held that convention plays an important role in physics. His view (and some later, more extreme versions of it) came to be known as "conventionalism".Yemima Ben-Menahem, Conventionalism: From Poincare to Quine, Cambridge University Press, 2006, p. 39. Poincaré believed that Newton's first law was not empirical but is a conventional framework assumption for mechanics (Gargani, 2012).{{Citation|author=Gargani Julien|title=Poincaré, le hasard et l'étude des systèmes complexes|publisher=L'Harmattan|year=2012|page=124|url=http://www.editions-harmattan.fr/index.asp?navig=catalogue&obj=livre&no=38754|access-date=5 June 2015|archive-url=https://web.archive.org/web/20160304140554/http://www.editions-harmattan.fr/index.asp?navig=catalogue&obj=livre&no=38754|archive-date=4 March 2016|url-status=dead}} He also believed that the geometry of physical space is conventional. He considered examples in which either the geometry of the physical fields or gradients of temperature can be changed, either describing a space as non-Euclidean measured by rigid rulers, or as a Euclidean space where the rulers are expanded or shrunk by a variable heat distribution. However, Poincaré thought that we were so accustomed to Euclidean geometry that we would prefer to change the physical laws to save Euclidean geometry rather than shift to non-Euclidean physical geometry.{{Citation|title=Science and Hypothesis|first1=Henri |last1=Poincaré |publisher=Cosimo, Inc. Press|year=2007|isbn=978-1-60206-505-5 |page=50

|url=https://books.google.com/books?id=2QXqHaVbkgoC&pg=PA50}}

=Free will=

Poincaré's famous lectures before the Société de Psychologie in Paris (published as Science and Hypothesis, The Value of Science, and Science and Method) were cited by Jacques Hadamard as the source for the idea that creativity and invention consist of two mental stages, first random combinations of possible solutions to a problem, followed by a critical evaluation.Hadamard, Jacques. An Essay on the Psychology of Invention in the Mathematical Field. Princeton Univ Press (1945)

Although he most often spoke of a deterministic universe, Poincaré said that the subconscious generation of new possibilities involves chance.

It is certain that the combinations which present themselves to the mind in a kind of sudden illumination after a somewhat prolonged period of unconscious work are generally useful and fruitful combinations... all the combinations are formed as a result of the automatic action of the subliminal ego, but those only which are interesting find their way into the field of consciousness... A few only are harmonious, and consequently at once useful and beautiful, and they will be capable of affecting the geometrician's special sensibility I have been speaking of; which, once aroused, will direct our attention upon them, and will thus give them the opportunity of becoming conscious... In the subliminal ego, on the contrary, there reigns what I would call liberty, if one could give this name to the mere absence of discipline and to disorder born of chance.{{cite book|title= Science and Method|chapter= 3: Mathematical Creation|date= 1914|chapter-url= http://ebooks.adelaide.edu.au/p/poincare/henri/science-and-method/book1.3.html|first= Henri|last= Poincaré|access-date= 4 September 2019|archive-date= 4 September 2019|archive-url= https://web.archive.org/web/20190904163001/https://ebooks.adelaide.edu.au/p/poincare/henri/science-and-method/book1.3.html|url-status= dead}}

Poincaré's two stages—random combinations followed by selection—became the basis for Daniel Dennett's two-stage model of free will.Dennett, Daniel C. 1978. Brainstorms: Philosophical Essays on Mind and Psychology. The MIT Press, p. 293

Bibliography

=Poincaré's writings in English translation=

Popular writings on the philosophy of science:

  • {{Citation

|author=Poincaré, Henri

|year=1902–1908

|title=The Foundations of Science

|place=New York

|publisher=Science Press

|url=https://archive.org/details/foundationsscie01poingoog}}; reprinted in 1921; this book includes the English translations of Science and Hypothesis (1902), The Value of Science (1905), Science and Method (1908).

  • 1905. "{{Citation |title=Science and Hypothesis | url=https://en.wikisource.org/wiki/Science_and_Hypothesis}}", The Walter Scott Publishing Co.
  • 1906. "{{Citation |title=The End of Matter | url=https://en.wikisource.org/wiki/Translation:The_End_of_Matter}}", Athenæum
  • 1913. "The New Mechanics", The Monist, Vol. XXIII.
  • 1913. "The Relativity of Space", The Monist, Vol. XXIII.
  • 1913. {{Citation | title=Last Essays. |place=New York |publisher=Dover reprint, 1963 | url=https://archive.org/details/mathematicsandsc001861mbp}}
  • 1956. Chance. In James R. Newman, ed., The World of Mathematics (4 Vols).
  • 1958. The Value of Science, New York: Dover.

On algebraic topology:

  • 1895. {{Citation |title=Analysis Situs

| url=http://www.maths.ed.ac.uk/~aar/papers/poincare2009.pdf |archive-url=https://web.archive.org/web/20120327043041/http://www.maths.ed.ac.uk/~aar/papers/poincare2009.pdf |archive-date=2012-03-27 |url-status=live}}. The first systematic study of topology.

On celestial mechanics:

  • 1890. {{cite book |last1=Poincaré |first1=Henri |translator1-last=Popp |translator1-first=Bruce D. |title=The three-body problem and the equations of dynamics: Poincaré's foundational work on dynamical systems theory |date=2017 |publisher=Springer International Publishing |location=Cham, Switzerland |isbn=978-3-319-52898-4}}
  • 1892–99. New Methods of Celestial Mechanics, 3 vols. English trans., 1967. {{isbn|1-56396-117-2}}.
  • 1905. "The Capture Hypothesis of J. J. See", The Monist, Vol. XV.
  • 1905–10. Lessons of Celestial Mechanics.

On the philosophy of mathematics:

  • Ewald, William B., ed., 1996. From Kant to Hilbert: A Source Book in the Foundations of Mathematics, 2 vols. Oxford Univ. Press. Contains the following works by Poincaré:
  • 1894, "On the Nature of Mathematical Reasoning", 972–981.
  • 1898, "On the Foundations of Geometry", 982–1011.
  • 1900, "Intuition and Logic in Mathematics", 1012–1020.
  • 1905–06, "Mathematics and Logic, I–III", 1021–1070.
  • 1910, "On Transfinite Numbers", 1071–1074.
  • 1905. "The Principles of Mathematical Physics", The Monist, Vol. XV.
  • 1910. "The Future of Mathematics", The Monist, Vol. XX.
  • 1910. "Mathematical Creation", The Monist, Vol. XX.

Other:

  • 1904. Maxwell's Theory and Wireless Telegraphy, New York, McGraw Publishing Company.
  • 1905. "The New Logics", The Monist, Vol. XV.
  • 1905. "The Latest Efforts of the Logisticians", The Monist, Vol. XV.

Exhaustive bibliography of English translations:

  • 1892–2017. {{Citation |title=Henri Poincaré Papers |url=http://henripoincarepapers.univ-nantes.fr/bibliohp/index.php?a=on&lang=en&action=Chercher |archive-url=https://web.archive.org/web/20200801151000/http://henripoincarepapers.univ-nantes.fr/bibliohp/index.php?a=on&lang=en&action=Chercher |url-status=dead |archive-date=1 August 2020 }}.

See also

=Concepts=

=Theorems=

Here is a list of theorems proved by Poincaré:

{{cols|colwidth=26em}}

{{colend}}

= Other =

References

=Footnotes=

{{Reflist}}

=Sources=

  • Bell, Eric Temple, 1986. Men of Mathematics (reissue edition). Touchstone Books. {{isbn|0-671-62818-6}}.
  • Belliver, André, 1956. Henri Poincaré ou la vocation souveraine. Paris: Gallimard.
  • Bernstein, Peter L, 1996. "Against the Gods: A Remarkable Story of Risk". (pp. 199–200). John Wiley & Sons.
  • Boyer, B. Carl, 1968. A History of Mathematics: Henri Poincaré, John Wiley & Sons.
  • Grattan-Guinness, Ivor, 2000. The Search for Mathematical Roots 1870–1940. Princeton Uni. Press.
  • {{Citation|last=Dauben|given=Joseph|author-link=Joseph Dauben|orig-year=1993|year=2004|chapter=Georg Cantor and the Battle for Transfinite Set Theory|chapter-url=http://www.acmsonline.org/journal/2004/Dauben-Cantor.pdf|title=Proceedings of the 9th ACMS Conference (Westmont College, Santa Barbara, CA)|pages=1–22|url-status=dead|archive-url=https://web.archive.org/web/20100713115605/http://www.acmsonline.org/journal/2004/Dauben-Cantor.pdf|archive-date=13 July 2010}}. Internet version published in Journal of the ACMS 2004.
  • Folina, Janet, 1992. Poincaré and the Philosophy of Mathematics. Macmillan, New York.
  • Gray, Jeremy, 1986. Linear differential equations and group theory from Riemann to Poincaré, Birkhauser {{isbn|0-8176-3318-9}}
  • Gray, Jeremy, 2013. Henri Poincaré: A scientific biography. Princeton University Press {{isbn|978-0-691-15271-4}}
  • {{Citation |url=https://www.ams.org/notices/200509/comm-mawhin.pdf |archive-url=https://web.archive.org/web/20070303185921/http://www.ams.org/notices/200509/comm-mawhin.pdf |archive-date=2007-03-03 |url-status=live

|title=Henri Poincaré. A Life in the Service of Science

|author=Jean Mawhin | author-link=Jean Mawhin |journal=Notices of the AMS

|date=October 2005 |volume=52 |issue=9 |pages=1036–1044 }}

  • Kolak, Daniel, 2001. Lovers of Wisdom, 2nd ed. Wadsworth.
  • Gargani, Julien, 2012. Poincaré, le hasard et l'étude des systèmes complexes, L'Harmattan.
  • Murzi, 1998. "Henri Poincaré".
  • O'Connor, J. John, and Robertson, F. Edmund, 2002, "Jules Henri Poincaré". University of St. Andrews, Scotland.
  • Peterson, Ivars, 1995. Newton's Clock: Chaos in the Solar System (reissue edition). W H Freeman & Co. {{isbn|0-7167-2724-2}}.
  • Sageret, Jules, 1911. [https://books.google.com/books?id=6Mu4AAAAIAAJ Henri Poincaré]. Paris: Mercure de France.
  • Toulouse, E., 1910. Henri Poincaré – (Source biography in French) at University of Michigan Historic Math Collection.
  • {{cite book |title=Mathematics and Its History |edition=3rd, illustrated |first1=John |last1=Stillwell |author-link=John Stillwell |publisher= Springer Science & Business Media |year=2010 |isbn=978-1-4419-6052-8 |url=https://books.google.com/books?id=V7mxZqjs5yUC }}
  • {{cite book|title=Papers on Topology: Analysis Situs and Its Five Supplements by Henri Poincaré, translated, with an introduction, by John Stillwell |year=2010|publisher=American Mathematical Society|isbn=978-0-8218-5234-7 |url=https://books.google.com/books?id=_WjVAwAAQBAJ}} – {{cite web|author=Satzer, William J.|date=April 26, 2011|title=Review of Papers on Topology: Analysis Situs and Its Five Supplements by Henri Poincaré, translated and edited by John Stillwell|website=MAA Reviews, Mathematical Association of America|url=https://old.maa.org/press/maa-reviews/papers-on-topology-ianalysis-situsi-and-its-five-supplements|access-date=26 January 2024|archive-date=26 January 2024|archive-url=https://web.archive.org/web/20240126002055/https://maa.org/press/maa-reviews/papers-on-topology-ianalysis-situsi-and-its-five-supplements|url-status=dead}}
  • Verhulst, Ferdinand, 2012 Henri Poincaré. Impatient Genius. N.Y.: Springer.
  • Henri Poincaré, l'œuvre scientifique, l'œuvre philosophique, by Vito Volterra, Jacques Hadamard, Paul Langevin and Pierre Boutroux, Felix Alcan, 1914.
  • Henri Poincaré, l'œuvre mathématique, by Vito Volterra.
  • Henri Poincaré, le problème des trois corps, by Jacques Hadamard.
  • Henri Poincaré, le physicien, by Paul Langevin.
  • Henri Poincaré, l'œuvre philosophique, by Pierre Boutroux.
  • {{PlanetMath attribution|id=3793|title=Jules Henri Poincaré}}

Further reading

=Secondary sources to work on relativity=

  • {{cite journal | last=Cuvaj | first=Camillo | title=Henri Poincaré's Mathematical Contributions to Relativity and the Poincaré Stresses | journal=American Journal of Physics | volume=36 | issue=12 | date=1968-12-01 | issn=0002-9505 | doi=10.1119/1.1974373 | pages=1102–1113| bibcode=1968AmJPh..36.1102C }}
  • {{cite journal | last=Darrigol | first=Olivier | title=Henri Poincaré's criticism of Fin De Siècle electrodynamics | journal=Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics | volume=26 | issue=1 | date=1995 | doi=10.1016/1355-2198(95)00003-C | pages=1–44| bibcode=1995SHPMP..26....1D }}
  • {{cite book | last=Darrigol | first=Olivier | title=Electrodynamics from Ampère to Einstein | publisher=Clarendon Press | publication-place=Oxford | year=2000 | isbn=978-0-19-850594-5 | url-access=registration | url=https://archive.org/details/electrodynamicsf0000darr }}
  • {{cite journal | last=Darrigol | first=Olivier | title=The Mystery of the Einstein–Poincaré Connection | journal=Isis | volume=95 | issue=4 | date=2004 | issn=0021-1753 | doi=10.1086/430652 | pages=614–626| pmid=16011297 }}
  • {{Citation|author=Darrigol, O. |title=The Genesis of the theory of relativity |year=2005 |journal=Séminaire Poincaré|volume=1|pages=1–22|url=http://www.bourbaphy.fr/darrigol2.pdf |archive-url=https://web.archive.org/web/20080228124558/http://www.bourbaphy.fr/darrigol2.pdf |archive-date=2008-02-28 |url-status=live|doi=10.1007/3-7643-7436-5_1|isbn=978-3-7643-7435-8 |bibcode=2006eins.book....1D }}
  • {{cite book | last=Galison | first=Peter | title=Einstein's Clocks and Poincare's Maps: Empires of Time | publisher=W. W. Norton & Company | publication-place=New York | date=2004-09-14 | isbn=978-0-393-32604-8}}
  • {{Citation|author=Giannetto, E. |title=The Rise of Special Relativity: Henri Poincaré's Works Before Einstein |year=1998 |journal=Atti del XVIII Congresso di Storia della Fisica e dell'astronomia |pages=171–207}}
  • {{cite book | last=Giedymin | first=Jerzy | title=Science and Convention: Essays on Henri Poincaré's Philosophy of Science and the Conventionalist Tradition | publisher=Pergamon | publication-place=Oxford; New York | date=1982 | isbn=978-0-08-025790-7| author-link=Jerzy Giedymin }}
  • {{cite journal | last=Goldberg | first=Stanley | title=Henri Poincare and Einstein's Theory of Relativity | journal=American Journal of Physics | volume=35 | issue=10 | date=1967-10-01 | issn=0002-9505 | doi=10.1119/1.1973643 | pages=934–944| bibcode=1967AmJPh..35..934G }}
  • {{cite journal | last=Goldberg | first=Stanley | title=Poincare's Silence and Einstein's Relativity: The Role of Theory and Experiment in Poincaré's Physics | journal=The British Journal for the History of Science | volume=5 | issue=1 | date=1970 | issn=0007-0874 | doi=10.1017/S0007087400010633 | pages=73–84}}
  • {{cite book | last=Holton | first=Gerald | orig-year=1973| year=1988 | chapter=Poincaré and Relativity| title= Thematic Origins of Scientific Thought: Kepler to Einstein | publisher=Harvard University Press|isbn=978-0-674-87747-4}}
  • {{cite journal | last=Katzir | first=Shaul | title=Poincaré's Relativistic Physics: Its Origins and Nature | journal=Physics in Perspective | volume=7 | issue=3 | date=2005 | issn=1422-6944 | doi=10.1007/s00016-004-0234-y | pages=268–292| bibcode=2005PhP.....7..268K }}
  • {{Citation| last1=Keswani | first1=G. H. | last2=Kilmister | first2=C. W. |year=1983 |journal=Br. J. Philos. Sci. |title=Intimations of Relativity: Relativity Before Einstein |pages=343–354 |volume=34 |doi=10.1093/bjps/34.4.343 |issue=4 |s2cid=65257414 |url=http://osiris.sunderland.ac.uk/webedit/allweb/news/Philosophy_of_Science/PIRT2002/Intimations%20of%20Relativity.doc |url-status=dead |archive-url=https://web.archive.org/web/20090326084436/http://osiris.sunderland.ac.uk/webedit/allweb/news/Philosophy_of_Science/PIRT2002/Intimations%20of%20Relativity.doc |archive-date=26 March 2009}}
  • {{cite journal | last=Keswani | first=G. H. | title=Origin and Concept of Relativity (I) | journal=The British Journal for the Philosophy of Science | volume=15 | issue=60 | date=1965-02-01 | issn=0007-0882 | doi=10.1093/bjps/XV.60.286 | pages=286–306}}
  • {{cite journal | last=Keswani | first=G. H. | title=Origin and Concept of Relativity (II) | journal=The British Journal for the Philosophy of Science | volume=16 | issue=61 | date=1965-05-01 | issn=0007-0882 | doi=10.1093/bjps/XVI.61.19 | pages=19–32}}
  • {{cite journal | last=Keswani | first=G. H. | title=Origin and Concept of Relativity (III) | journal=The British Journal for the Philosophy of Science | volume=16 | issue=64 | date=1966-02-01 | issn=0007-0882 | doi=10.1093/bjps/XVI.64.273 | pages=273–294}}
  • {{cite book | last=Kragh | first=Helge | title=Quantum Generations: A History of Physics in the Twentieth Century | publisher=Princeton University Press | publication-place=Princeton, NJ Chichester | year=1999 | isbn=978-0-691-09552-3}}
  • {{Citation | author=Langevin, P. | year=1913 | journal=Revue de Métaphysique et de Morale | title= L'œuvre d'Henri Poincaré: le physicien |page= 703 |volume=21|url=http://gallica.bnf.fr/ark:/12148/bpt6k111418/f93.chemindefer}}
  • {{Citation | author=Macrossan, M. N. | year=1986 | journal=Br. J. Philos. Sci. | title=A Note on Relativity Before Einstein | pages=232–234 | volume=37 | issue=2 | url=http://espace.library.uq.edu.au/view.php?pid=UQ:9560 | doi=10.1093/bjps/37.2.232 | citeseerx=10.1.1.679.5898 | s2cid=121973100 | access-date=27 March 2007 | archive-url=https://web.archive.org/web/20131029203003/http://espace.library.uq.edu.au/view.php?pid=UQ:9560 | archive-date=29 October 2013 | url-status=dead }}
  • {{cite journal | last=Miller | first=Arthur I. | title=A study of Henri Poincaré's "Sur la Dynamique de l'Electron" | journal=Archive for History of Exact Sciences | volume=10 | issue=3–5 | date=1973 | issn=0003-9519 | doi=10.1007/BF00412332 | pages=207–328|s2cid=189790975}}
  • {{cite book | last=Miller | first=Arthur I. | title=Albert Einstein's Special Theory of Relativity. Emergence (1905) and early interpretation (1905–1911) | publisher=Addison Wesley Publishing Company | publication-place=Reading, Mass | date=1981 | isbn=978-0-201-04679-3 | url-access=registration | url=https://archive.org/details/alberteinsteinss0000mill }}
  • {{cite book | author=Miller, A.I. |contribution= Why did Poincaré not formulate special relativity in 1905? |year=1996 |editor1=Jean-Louis Greffe |editor2=Gerhard Heinzmann |editor3=Kuno Lorenz | title=Henri Poincaré : science et philosophie| publisher=Akademie-Verlag| pages=69–100|publication-place=Berlin}}
  • {{cite book | last=Popp | first=Bruce D | title=Henri Poincaré: Electrons to Special Relativity | publisher=Springer | publication-place=Cham | date=2020-08-25 | isbn=978-3-030-48038-7}}
  • {{cite journal | last=Schwartz | first=H. M. | title=Poincaré's Rendiconti Paper on Relativity. Part I | journal=American Journal of Physics | volume=39 | issue=11 | date=1971-11-01 | issn=0002-9505 | doi=10.1119/1.1976641 | pages=1287–1294|bibcode = 1971AmJPh..39.1287S }}
  • {{cite journal | last=Schwartz | first=H. M. | title=Poincaré's Rendiconti Paper On Relativity. Part II | journal=American Journal of Physics | volume=40 | issue=6 | date=1972-06-01 | issn=0002-9505 | doi=10.1119/1.1986684 | doi-access=free | pages=862–872 | bibcode=1972AmJPh..40..862S | url=https://pubs.aip.org/aapt/ajp/article-pdf/40/6/862/12103533/862_1_online.pdf | access-date=2025-03-28}}
  • {{cite journal | last=Schwartz | first=H. M. | title=Poincaré's Rendiconti Paper on Relativity. Part III | journal=American Journal of Physics | volume=40 | issue=9 | date=1972-09-01 | issn=0002-9505 | doi=10.1119/1.1986815 | pages=1282–1287 |bibcode = 1972AmJPh..40.1282S }}
  • {{cite journal | last=Scribner | first=Charles | title=Henri Poincaré and the Principle of Relativity | journal=American Journal of Physics | volume=32 | issue=9 | date=1964-09-01 | issn=0002-9505 | doi=10.1119/1.1970936 | pages=672–678|bibcode =1964AmJPh..32..672S}}
  • {{Citation | author=Walter, S. | year=2005 | editor=Renn, J. | contribution= Henri Poincaré and the theory of relativity | title=Albert Einstein - Chief Engineer of the Universe: 100 Authors for Einstein |pages=162–165 | place=Berlin | publisher=Wiley-VCH|contribution-url=http://scottwalter.free.fr/papers/2005-100authors-poincare-einstein-walter.html}}
  • {{Citation | author=Walter, S. | year=2007 | editor=Renn, J. | contribution= Breaking in the 4-vectors: the four-dimensional movement in gravitation, 1905–1910 | title=The Genesis of General Relativity |pages=193–252 |volume=3 |place=Berlin | publisher=Springer|contribution-url=http://scottwalter.free.fr/papers/2007-genesis-walter.html}}
  • {{Citation | author=Whittaker, E.T.|author-link=E. T. Whittaker | year=1953 | title= A History of the Theories of Aether and Electricity: The Modern Theories 1900–1926| chapter= The Relativity Theory of Poincaré and Lorentz | place=London |publisher=Nelson}}
  • {{cite book | last=Zahar | first=Elie | title=Poincaré's Philosophy | publisher=Open Court Publishing | publication-place=Chicago, Ill. | date=2001 | isbn=978-0-8126-9435-2}}

=Non-mainstream sources=

  • {{cite book | last=Leveugle | first=Jules | title=La relativité, Poincaré et Einstein, Planck, Hilbert – Histoire véridique de la Théorie de la Relativitén | publisher=Editions L'Harmattan | publication-place=Paris | date=2004 | isbn=978-2-7475-6862-3 | language=fr}}
  • {{Citation | author=Logunov, A.A. | year=2004 | title= Henri Poincaré and relativity theory | arxiv=physics/0408077 |bibcode = 2004physics...8077L |isbn=978-5-02-033964-4}}