Electron scattering

{{Short description|Deviation of electrons from their original trajectories}}

{{distinguish|Electron diffraction}}

{{ infobox

|abovestyle = background:#CEF2E0;

|above = Types of Scattering

|image = File:Electron-beam interaction and transmission with sample.jpg

|caption = Pictorial description of how an electron beam may interact with a sample with nucleus N, and electron cloud of electron shells K,L,M. Showing transmitted electrons and elastic/inelastically scattered electrons. SE is a Secondary Electron ejected by the beam electron, emitting a characteristic photon (X-Ray) γ. BSE is a Back-Scattered Electron, an electron which is scattered backwards instead of being transmitted through the sample.

|headerstyle = background:#CEF2E0;

|header1 = Electron ({{SubatomicParticle|Electron}}, {{SubatomicParticle|beta-}})

|label2 = Particle

|data2 = Electron

|label3 = Mass

|data3 = {{val|9.10938291|(40)|e=-31|ul=kg}}{{cite web|title=CODATA Internationally recommended values of the Fundamental Physical Constants|url=http://physics.nist.gov/cuu/Constants/index.html|work=NIST Standard Reference Database 121|publisher=National Institute of Standards and Technology|access-date=23 November 2013}}
{{val|5.4857990946|(22)|e=-4|ul=Da}}
[{{val|1822.8884845|(14)}}]−1 DaThe fractional version's denominator is the inverse of the decimal value (along with its relative standard uncertainty of {{val|4.2|e=-13|ul=Da}}).
{{val|0.510998928|(11)|ul=MeV/c2}}

|label4 = Electric Charge

|data4 = {{val|-1|ul=e}}The electron's charge is the negative of elementary charge, which has a positive value for the proton.
{{val|-1.602176565|(35)|e=-19|ul=C}}
{{val|-4.80320451|(10)|e=-10|u=esu}}

|label5 = Magnetic Moment

|data5 = {{gaps|−1.001|159|652|180|76(27)|u=μB}}

|label6 = Spin

|data6 = {{frac|1|2}}

|header7 = Scattering

|label8 = Forces/Effects

|data8 = Lorentz force, Electrostatic force, Gravitation, Weak interaction

|label9 = Measures

|data9 = Charge, Current

|label10 = Categories

|data10 = Elastic collision, Inelastic collision, High energy, Low energy

|label11 = Interactions

|data11 = Electron scattering#Møller scattering
Electron scattering#Compton scattering
Electron scattering#Bhabha scattering
ElectronProton
ElectronNeutron
Electronnucleus

|label12 = Types

|data12 = Compton scattering
Møller scattering
Mott scattering
Bhabha scattering
Bremsstrahlung
Deep inelastic scattering
Synchrotron emission
Thomson scattering

}}

Electron scattering occurs when electrons are displaced from their original trajectory. This is due to the electrostatic forces within matter interaction or,{{cite encyclopedia|title=electron scattering|url=http://www.britannica.com/EBchecked/topic/183635/electron-scattering|encyclopedia=Encyclopædia Britannica|publisher=Encyclopædia Britannica, Inc.|access-date=13 October 2013}}{{cite web|title=Electron scattering in solids|url=http://www.ioffe.rssi.ru/ES/|work=Ioffe Institute|publisher=Department of Applied Mathematics and Mathematical Physics|access-date=13 October 2013}} if an external magnetic field is present, the electron may be deflected by the Lorentz force.{{cite book|last1=Howe|first2=Brent|last2=Fultz|first1=James|author2-link=Brent Fultz|title=Transmission electron microscopy and diffractometry of materials|year=2008|publisher=Springer|location=Berlin|isbn=978-3-540-73885-5|edition=3rd}}{{cite book|last=Kohl|first=L. Reimer, H.|title=Transmission electron microscopy physics of image formation|year=2008|publisher=Springer|location=New York|isbn=978-0-387-34758-5|edition=5th}} This scattering typically happens with solids such as metals, semiconductors and insulators;{{cite web|title=Electron scattering|url=http://www.matter.org.uk/tem/electron_scattering.htm|work=MATTER|publisher=The University of Liverpool|access-date=13 October 2013|archive-url=https://web.archive.org/web/20131015121537/http://www.matter.org.uk/tem/electron_scattering.htm|archive-date=15 October 2013|url-status=dead}} and is a limiting factor in integrated circuits and transistors.

Electron scattering has many applications ranging from the use of swift electron in electron microscopes to very high energies for hadronic systems that allows the measurement of the distribution of charges for nucleons and nuclear structure.{{cite book|editor=B. Frois|editor2=I. Sick|title=Modern topics in electron scattering|year=1991|publisher=World Scientific|location=Singapore|isbn=978-9971509750|bibcode=1991mtes.book.....F|url-access=registration|url=https://archive.org/details/moderntopicsinel0000unse}}{{cite journal |last1=Drechsel |first1=D. |last2=Giannini |first2=M. M. |title=Electron scattering off nuclei |year=1989 |volume=52 |journal=Reports on Progress in Physics |issue=9 |doi=10.1088/0034-4885/52/9/002 |pages=1083|bibcode = 1989RPPh...52.1083D |s2cid=250912319 }} The scattering of electrons has allowed us to understand many details about the atomic structure, from the ordering of atoms to that protons and neutrons are made up of the smaller elementary subatomic particles called quarks.

Electrons may be scattered through a solid in several ways:

  • Not at all: no electron scattering occurs at all and the beam passes straight through.
  • Single scattering: when an electron is scattered just once.
  • Plural scattering: when electron(s) scatter several times.
  • Multiple scattering: when electron(s) scatter many times over.

The likelihood of an electron scattering and the degree of the scattering is a function of the specimen thickness and the mean free path.

History

The principle of the electron was first theorised in the period of 1838–1851 by a natural philosopher by the name of Richard Laming who speculated on the existence of sub-atomic, unit charged particles; he also pictured the atom as being an 'electrosphere' of concentric shells of electrical particles surrounding a material core.{{cite book|last=Arabatzis|first=Theodore|title=Representing Electrons A Biographical Approach to Theoretical Entities.|year=2005|publisher=University of Chicago Press|location=Chicago|isbn=978-0226024219}}Further notes can be found in Laming, R. (1845): "Observations on a paper by Prof. Faraday concerning electric conduction and the nature of matter", Phil. Mag. 27, 420–423 and in {{cite journal | last1 = Farrar | first1 = W. F. | year = 1969 | title = Richard Laming and the coal-gas industry, with his views on the structure of matter | journal = Annals of Science | volume = 25 | issue = 3| pages = 243–53 | doi=10.1080/00033796900200141}}

It is generally accepted that J. J. Thomson first discovered the electron in 1897, although other notable members in the development in charged particle theory are George Johnstone Stoney (who coined the term "electron"), Emil Wiechert (who was first to publish his independent discovery of the electron), Walter Kaufmann, Pieter Zeeman and Hendrik Lorentz.{{cite book|editor-last=Springford|editor-first=Michael|title=Electron : a centenary volume|year=1997|publisher=Cambridge Univ. Press|location=Cambridge [u.a.]|isbn=978-0521561303|edition=1st}}

Compton scattering was first observed at Washington University in St. Louis in 1923 by Arthur Compton who earned the 1927 Nobel Prize in Physics for the discovery; his graduate student Y. H. Woo who further verified the results is also of mention. Compton scattering is usually cited in reference to the interaction involving the electrons of an atom, however nuclear Compton scattering does exist.{{citation needed|date=November 2013}}

The first electron diffraction experiment was conducted in 1927 by Clinton Davisson and Lester Germer using what would come to be a prototype for modern LEED system.{{cite book|last=Pendry|first=J. B.|title=Low energy electron diffraction: the theory and its application to determination of surface structure|url=https://archive.org/details/lowenergyelectro0000pend|url-access=registration|year=1974|publisher=Academic Press|location=London|isbn=978-0125505505}} The experiment was able to demonstrate the wave-like properties of electrons,Details can be found in Ritchmeyer, Kennard and Lauritsen's (1955) book on atomic physics thus confirming the de Broglie hypothesis that matter particles have a wave-like nature.{{citation needed|date=November 2013}} However, after this the interest in LEED diminished in favour of high-energy electron diffraction until the early 1960s when an interest in LEED was revived; of notable mention during this period is H. E. Farnsworth who continued to develop LEED techniques.

High energy electron-electron beams for collisions history begins in 1956 when K. O'Neill of Princeton University became interested in high energy collisions, and introduced the idea of accelerator(s) injecting into storage ring(s). While the idea of beam-beam collisions had been around since approximately the 1920s, it was not until 1953 that a German patent for a colliding beam apparatus was obtained by Rolf Widerøe.{{cite journal|last=PANOFSKY|first=W.K.H.|title=SOME REMARKS ON THE EARLY HISTORY OF HIGH ENERGY ELECTRON–ELECTRON SCATTERING|journal=International Journal of Modern Physics A|date=10 June 1998|volume=13|issue=14|pages=2429–2430|doi=10.1142/S0217751X98001219|bibcode = 1998IJMPA..13.2429P }}

Phenomena

{{see also|Quantum electrodynamics}}

Electrons can be scattered by other charged particles through the electrostatic Coulomb forces. Furthermore, if a magnetic field is present, a traveling electron will be deflected by the Lorentz force. An extremely accurate description of all electron scattering, including quantum and relativistic aspects, is given by the theory of quantum electrodynamics.

= Lorentz force =

File:Action of the Lorentz force bending the path of an electron in a magnetic field.gif

{{Main|Lorentz force}}

The Lorentz force, named after Dutch physicist Hendrik Lorentz, for a charged particle q is given (in SI units) by the equation:{{cite web|last=Fitzpatrick|first=Richard|title=The Lorentz force|url=http://farside.ph.utexas.edu/teaching/em/lectures/node33.html|publisher=University of Texas}}

: \boldsymbol{F} = q\boldsymbol{E} + q\boldsymbol{v} \times \boldsymbol{B}

where qE describes the electric force due to a present electric field, E, acting on q.

{{br}}And qv × B describes the magnetic force due to a present magnetic field, B, acting on q when q is moving with velocity v.{{cite web|last=Nave|first=R.|title=Lorentz Force Law|url=http://hyperphysics.phy-astr.gsu.edu/hbase/magnetic/magfor.html|work=hyperphysics|publisher=Georgia State University|access-date=1 November 2013}}

This can also be written as:

: \boldsymbol{F} = q[- \nabla \phi - \frac{d\boldsymbol{A}}{dt} + \nabla(\boldsymbol{A} \cdot \boldsymbol{v})]

where \phi is the electric potential, and A is the magnetic vector potential.{{cite web|last=Weisstein|first=Eric W.|title=Lorentz Force|url=http://scienceworld.wolfram.com/physics/LorentzForce.html|work=scienceworld|publisher=wolfram research|access-date=1 November 2013}}

It was Oliver Heaviside who is considered to be the first in 1885 and 1889 to derive the correct expression for the Lorentz force of qv × B.{{cite book|last=Darrigol|first=Olivier|title=Electrodynamics from Ampère to Einstein|year=2000|publisher=Oxford Univ. Press|location=Oxford [u.a.]|isbn=978-0198505945|edition=Repr.|url-access=registration|url=https://archive.org/details/electrodynamicsf0000darr}} Hendrik Lorentz derived and refined the concept in 1892 and gave it his name,{{cite web|last=Kurtus |first=Ron |title=Lorentz Force on Electrical Charges in Magnetic Field |url=http://www.school-for-champions.com/science/magnetic_force_lorentz.htm |work=Ron Kurtus' School for Champions |publisher=School for Champions |access-date=6 November 2013 |url-status=dead |archive-url=https://web.archive.org/web/20130916180922/http://school-for-champions.com/science/magnetic_force_lorentz.htm |archive-date=16 September 2013 }} incorporating forces due to electric fields.

{{br}}Rewriting this as the equation of motion for a free particle of charge q mass m, this becomes:

: m\frac{d\boldsymbol{v}}{dt} = q\boldsymbol{E} + q\boldsymbol{v} \times \boldsymbol{B}

or

: m\frac{d\gamma\boldsymbol{v}}{dt} = q\boldsymbol{E} + q\boldsymbol{v} \times \boldsymbol{B}

in the relativistic case including the Lorentz contraction where γ is:{{cite book|last=Sands|first=Feynman, Leighton|title=Mainly electromagnetism and matter|year=2010|publisher=Basic Books|location=New York|isbn=9780465024162|edition=New millennium}}

: \gamma (v) \equiv \frac{1}{\sqrt{1-v^2/c^2}}

this equation of motion was first verified in 1897 in J. J. Thomson's experiment investigating cathode rays, which confirmed, through bending of the rays in a magnetic field, that these rays were a stream of charged particles now known as electrons.

Variations on this basic formula describe the magnetic force on a current-carrying wire (sometimes called Laplace force), the electromotive force in a wire loop moving through a magnetic field (an aspect of Faraday's law of induction), and the force on a particle which might be traveling near the speed of light (relativistic form of the Lorentz force).

= Electrostatic Coulomb force =

Image:CoulombsLaw.svgs q and Q relates to the distance r between the point charges and to the simple product of their charges. The diagram shows that like charges repel each other, and opposite charges attract each other.]]

[[Image:Coulombslawgraph.svg|thumb|right|upright=1.5|alt=A graphical representation of Coulomb's law|In the image, the vector F1 is the force experienced by q1, and the vector F2 is the force experienced by q2. When q1q2 > 0, the forces are repulsive (as in the image) and when q1q2 < 0 the forces are attractive (opposite to the image). The magnitude of the forces will always be equal.

In this case:

\mathbf{F} = k \frac{q_1 q_2}

\mathbf{r}_{12}|^2}\mathbf{\hat{r_{12}}} = \frac{q_1 q_2}{4 \pi \epsilon_0 |\mathbf{r_{12}}|^2}\mathbf{\hat{r_{12}}}

{{br}}where the vector,

{{br}}\boldsymbol{r_{12}}=\boldsymbol{r_1-r_2}

{{br}}is the vectorial distance between the charges and,

\boldsymbol{\hat{r}_{12}}={\boldsymbol{r_{12}}/|\boldsymbol{r_{12}}

{{br}}(a unit vector pointing from q2 to q1).

{{br}}The vector form of the equation above calculates the force F1 applied on q1 by q2. If r21 is used instead, then the effect on q2 can be found. It can be also calculated using Newton's third law: F2 = −F1.]]

{{Main|Coulomb's law}}

Electrostatic Coulomb force also known as Coulomb interaction and electrostatic force, named for Charles-Augustin de Coulomb who published the result in 1785, describes the attraction or repulsion of particles due to their electric charge.{{cite encyclopedia|title=Coulomb force|url=http://www.britannica.com/EBchecked/topic/140084/Coulomb-force|encyclopedia=Encyclopædia Britannica|access-date=21 November 2013}}

Coulomb's law states that:

: The magnitude of the electric force between two point charges is directly proportional to the product of the charges and inversely proportional to the square of the distance between them.{{cite book|author=Hugh D. Young|author2=Roger A. Freedman|author3=A. Lewis Ford|title=Sears and Zemansy's university physics : with modern physics|year=2007|publisher=Pearson Addison Wesley|location=San Francisco|isbn=9780321501301|pages=716–719, 830|edition=12e}}In – Coulomb (1785a) [https://books.google.com/books?id=by5EAAAAcAAJ&pg=PA569 "Premier mémoire sur l'électricité et le magnétisme,"] Histoire de l’Académie Royale des Sciences, pages 569–577 – Coulomb studied the repulsive force between bodies having electrical charges of the same sign:

Page 574 : Il résulte donc de ces trois essais, que l'action répulsive que les deux balles électrifées de la même nature d'électricité exercent l'une sur l'autre, suit la raison inverse du carré des distances.
Translation : It follows therefore from these three tests, that the repulsive force that the two balls – [that were] electrified with the same kind of electricity – exert on each other, follows the inverse proportion of the square of the distance.
In – Coulomb (1785b) [https://books.google.com/books?id=by5EAAAAcAAJ&pg=PA578 "Second mémoire sur l’électricité et le magnétisme"], Histoire de l’Académie Royale des Sciences, pages 578–611. – Coulomb showed that oppositely charged bodies obey an inverse-square law of attraction.

The magnitude of the electrostatic force is proportional to the scalar multiple of the charge magnitudes, and inversely proportional to the square of the distance (i.e. inverse-square law), and is given by:

: F = \frac

q_1 q_2
{4 \pi \epsilon_0 r^2}

or in vector notation:

: \boldsymbol{F} = \frac{q_1 q_2}{4 \pi \epsilon_0 |\boldsymbol{r}|^2}\boldsymbol{\hat{r}}

where q1, q2 are two point charges; {{overset|^|r|lh=0.4}} being the unit vector direction of the distance r between charges and ε0 is the permittivity of free space, given in SI units by:

: \epsilon_0 \approx \mathrm{8.854 \times 10^{-12}~C^2{\cdot}N^{-1}{\cdot}m^{-2}}

The directions of the forces exerted by the two charges on one another are always along the straight line joining them (the shortest distance), and are vector forces of infinite range, and they obey Newton's third law, being of equal magnitude and opposite direction. When both charges q1 and q2 have the same sign (either both positive or both negative) the forces between them are repulsive, if they are of opposite sign then the forces are attractive.{{cite web|last=Nave|first=R.|title=Coulomb's Law|url=http://hyperphysics.phy-astr.gsu.edu/hbase/electric/elefor.html|work=hyperphysics|publisher=Georgia State University|access-date=21 November 2013}} These forces obey an important property called the principle of superposition of forces, which states that if a third charge were introduced then the total force acting on that charge is the vector sum of the forces that would be exerted by the other charges individually; this holds for any number of charges. Coulomb's law has been stated for charges in a vacuum, if the space between point charges contains matter then the permittivity of the matter between the charges must be accounted for as follows:

: F = \frac

q_1 q_2
{4\pi\varepsilon_0\varepsilon_\text{r} r^2}

where εr is the relative permittivity of the space the force acts through, and is dimensionless.

= Collisions =

If two particles interact with one another in a scattering process there are two results possible after the interaction:{{cite book|last=Kopaleishvili|first=Teimuraz|title=Collision theory: (a short course)|year=1995|publisher=World Scientific|location=Singapore [u.a.]|isbn=978-9810220983|bibcode=1995ctsc.book.....K}}

== Elastic ==

{{see also|Elastic scattering}}

Elastic scattering is when the collisions between target and incident particles have total conservation of kinetic energy.{{cite web|title=Elastic and Inelastic Collisions in Particle Physics|url=http://hypernews.slac.stanford.edu/slacsite/aux/HiPPP/scattering/|work=SLAC|publisher=Stanford University|access-date=21 October 2013}} This implies that there is no fragmentation of the particles or energy loss,{{cite web|title=Scattering |url=http://www.physics.ox.ac.uk/documents/PUS/dis/scattering.htm |work=physics.ox |publisher=Oxford University |access-date=21 October 2013 |url-status=dead |archive-url=https://web.archive.org/web/20131023022419/http://www.physics.ox.ac.uk/documents/PUS/dis/scattering.htm |archive-date=23 October 2013 }} that is to say that the internal states of each of the particles remains unchanged. Due to the fact that there is no fragmentation elastic collisions can as a first approximation be modeled as occurring between point-like particles, a principle that is very useful for an elementary particle such as the electron.

== Inelastic ==

{{see also|Inelastic scattering}}

Inelastic scattering is when the collisions do not conserve kinetic energy, and as such the internal states of one or both of the particles has changed. This is due to energy being converted into heat, waves (sound), or vibrations between constituent particles of either collision party or other excitations such as light. Particles may also split apart, and energy can be converted into breaking the chemical bonds between components.

Momentum is conserved in both elastic and inelastic scattering. Other results than scattering are reactions, in which the structure of the interacting particles is changed producing two or more generally complex particles, and the creation of new particles that are not constituent elementary particles of the interacting particles.

Other types of scattering

= Electron–molecule scattering =

Electron scattering by isolated atoms and molecules occurs in the gas phase. It plays a key role in plasma physics and chemistry and it's important for such applications as semiconductor physics. Electron-molecule/atom scattering is normally treated by means of quantum mechanics. The leading approach to compute the cross sections is using R-matrix method.

= Compton scattering =

File:Photoscat feyn.png

{{Main|Compton scattering}}

Compton scattering, so named for Arthur Compton who first observed the effect in 1922 and which earned him the 1927 Nobel Prize in Physics;{{cite web|last=Nave|first=R.|title=Compton Scattering|url=http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/comptint.html|work=hyperphysics|publisher=Georgia State University|access-date=28 November 2013}} is the inelastic scattering of a high-energy photon by a free charged particle.{{cite web|last1=Neakrase|first1=Jennifer|last2=Neal|first2=Jennifer|last3=Venables|first3=John|title=Photoelectrons, Compton and Inverse Compton Scattering|url=http://venables.asu.edu/quant/proj/compton.html|work=Dept of Physics and Astronomy|publisher=Arizona State University|access-date=28 November 2013}}An electron in this case. Where the notion of "free" results from considering if the energy of the photon is large compared to the binding energy of the electron; then one could make the approximation that the electron as free.

This was demonstrated in 1923 by firing radiation of a given wavelength (X-rays in the given case) through a foil (carbon target), which was scattered in a manner inconsistent with classical radiation theory.For example, x-ray photons have an energy value of several keV. So, both conservation of momentum and energy could be observed. To show this, Compton scattered x-ray radiation off a graphite block and measured the wavelength of the x-rays before and after they were scattered as a function of the scattering angle. He discovered that the scattered x-rays had a longer wavelength than that of the incident radiation. Compton published

a paper in the Physical Review explaining the phenomenon: A quantum theory of the scattering of X-rays by light elements.{{cite journal|last=Compton|first=Arthur|title=A Quantum Theory of the Scattering of X-rays by Light Elements|journal=Physical Review|date=May 1923|volume=21|issue=5|pages=483–502|doi=10.1103/PhysRev.21.483|bibcode = 1923PhRv...21..483C |doi-access=free}} The Compton effect can be understood as high-energy photons scattering in-elastically off individual electrons, when the incoming photon gives part of its energy to the electron, then the scattered photon has lower energy and lower frequency and longer wavelength according to the Planck relation:{{cite web|last=Nave|first=R.|title=Compton Scattering|url=http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/compton.html|work=hyperphysics|publisher=Georgia State University|access-date=28 November 2013}}

: E = h \nu = h f

which gives the energy E of the photon in terms of frequency f or ν, and the Planck constant h ({{val|6.626|e=-34|u=J.s}} = {{val|4.136|e=-15|u=eV⋅s}}).{{cite web|last=Nave|first=R.|title=The Planck Hypothesis|url=http://hyperphysics.phy-astr.gsu.edu/hbase/mod2.html#c3|work=hyperphysics|publisher=Georgia State University|access-date=28 November 2013}}

The wavelength change in such scattering depends only upon the angle of scattering for a given target particle.{{cite web|title=Compton Scattering|url=http://www.ndt-ed.org/EducationResources/CommunityCollege/Radiography/Physics/comptonscattering.htm|work=NDT Education Resource Center|publisher=Iowa State University|access-date=28 November 2013}}

This was an important discovery during the 1920s when the particle (photon) nature of light suggested by the photoelectric effect was still being debated, the Compton experiment gave clear and independent evidence of particle-like behavior.

The formula describing the Compton shift in the wavelength due to scattering is given by:

: \lambda_\text{f} - \lambda_\text{i} = \frac{h}{m_\text{e}c}(1 - \cos\theta)

where λf is the final wavelength of the photon after scattering, λi is the initial wavelength of the photon before scattering, h is the Planck constant, me is the rest mass of the electron, c is the speed of light and θ is the scattering angle of the photon.

The coefficient of (1 − cos θ) is known as the Compton wavelength, but is in fact a proportionality constant for the wavelength shift.{{cite web|last=Jones|first=Andrew Zimmerman|title=The Compton Effect|url=http://physics.about.com/od/quantumphysics/a/comptoneffect.htm|work=About.com Physics|publisher=About.com|access-date=28 November 2013|archive-date=3 December 2013|archive-url=https://web.archive.org/web/20131203054755/http://physics.about.com/od/quantumphysics/a/comptoneffect.htm|url-status=dead}} The collision causes the photon wavelength to increase by somewhere between 0 (for a scattering angle of 0°) and twice the Compton wavelength (for a scattering angle of 180°).{{cite web|last1=Duffy|first1=Andrew|last2=Loewy|first2=Ali|title=The Compton Effect|url=http://physics.bu.edu/~duffy/semester2/c35_compton.html|work=Boston University's Physics department|publisher=Boston University|access-date=28 November 2013}}

Thomson scattering is the classical elastic quantitative interpretation of the scattering process, and this can be seen to happen with lower, mid-energy, photons. The classical theory of an electromagnetic wave scattered by charged particles, cannot explain low intensity shifts in wavelength.

Inverse Compton scattering takes place when the electron is moving, and has sufficient kinetic energy compared to the photon. In this case net energy may be transferred from the electron to the photon. The inverse Compton effect is seen in astrophysics when a low energy photon (e.g. of the cosmic microwave background) bounces off a high energy (relativistic) electron. Such electrons are produced in supernovae and active galactic nuclei.

= Møller scattering =

File:Moller scattering t-channel.svg

{{Main|Møller scattering}}

= Mott scattering =

{{Main|Mott scattering}}

= Bhabha scattering =

{{Main|Bhabha scattering}}

= Bremsstrahlung scattering =

{{Main|Bremsstrahlung}}

= Deep inelastic scattering =

{{Main|Deep inelastic scattering}}

= Synchrotron emission =

{{Main|Synchrotron emission}}

If a charged particle such as an electron is accelerated – this can be acceleration in a straight line or motion in a curved path – electromagnetic radiation is emitted by the particle. Within electron storage rings and circular particle accelerators known as synchrotrons, electrons are bent in a circular path and emit X-rays typically. This radially emitted (\boldsymbol{a}\perp \boldsymbol{v}) electromagnetic radiation when charged particles are accelerated is called synchrotron radiation.{{cite web|last=Nave|first=R.|title=Synchrotron Radiation|url=http://hyperphysics.phy-astr.gsu.edu/hbase/particles/synchrotron.html|work=hyperphysics|publisher=Georgia State University|access-date=5 December 2013}} It is produced in synchrotrons using bending magnets, undulators and/or wigglers.{{citation needed|date=December 2013}}

The first observation came at the General Electric Research Laboratory in Schenectady, New York, on April 24, 1947, in the synchrotron built by a team of Herb Pollack to test the idea of phase-stability principle for RF accelerators.The mass of particles in a cyclotron grows as the energy increases into the relativistic range. The heavier particles then arrive too late at the electrodes for a radio-frequency (RF) voltage of fixed frequency to accelerate them, thereby limiting the maximum particle energy. To deal with this problem, in 1945 McMillan in the U. S. and Veksler in the Soviet Union independently proposed decreasing the frequency of the RF voltage as the energy increases to keep the voltage and the particle synchronized. This was a specific application of their phase-stability principle for RF accelerators, which explains how particles that are too fast get less acceleration and slow down relative to their companions while particles that are too slow get more and speed up, thereby resulting in a stable bunch of particles that are accelerated together. When the technician was asked to look around the shielding with a large mirror to check for sparking in the tube, he saw a bright arc of light coming from the electron beam. Robert Langmuir is credited as recognizing it as synchrotron radiation or, as he called it, "Schwinger radiation" after Julian Schwinger.{{cite web|last=Robinson|first=Arthur L|title=HISTORY of SYNCHROTRON RADIATION|url=http://xdb.lbl.gov/Section2/Sec_2-2.html|work=Center for X-ray Optics and Advanced Light Source|publisher=Lawrence Berkeley National Laboratory|access-date=5 December 2013}}

Classically, the radiated power P from an accelerated electron is:

: P=\frac{2}{3}\frac{e^2}{4\pi \varepsilon_0 c^2} a^2

this comes from the Larmor formula; where ε0 is the vacuum permittivity, e is elementary charge, c is the speed of light, and a is the acceleration.

Within a circular orbit such as a storage ring, the non-relativistic case is simply the centripetal acceleration. However within a storage ring the acceleration is highly relativistic, and can be obtained as follows:

: a_\text{non-relativistic} = \frac{v^2}{r} \rightarrow a_\text{relativistic} = \frac{1}{m} \frac{dp}{d\tau} = \frac{1}{m} \gamma \frac{d(\gamma m v)}{dt} = \gamma^2 \frac{dv}{dt} = \gamma^2 \frac{v^2}{r} ,

where v is the circular velocity, r is the radius of the circular accelerator, m is the rest mass of the charged particle, p is the momentum, τ is the Proper time (t/γ), and γ is the Lorentz factor.

Radiated power then becomes:

: P=\frac{2}{3} \frac{e^2}{4\pi\varepsilon_0 c^2} \left( \frac{\gamma^2 v^2}{r} \right)^2 = \frac{2}{3} \frac{e^2}{4\pi\varepsilon_0 c^2} \frac{\gamma^4 v^4}{r^2}

For highly relativistic particles, such that velocity becomes nearly constant, the factor γ4 becomes the dominant variable in determining loss rate, which means that the loss scales as the fourth power of the particle energy γmc2; and the inverse dependence of synchrotron radiation loss on radius argues for building the accelerator as large as possible.

Facilities

= SLAC =

{{see also|SLAC National Accelerator Laboratory}}

Image:Stanford-linear-accelerator-usgs-ortho-kaminski-5900.jpg

Stanford Linear Accelerator Center is located near Stanford University, California.{{cite web|last1=Walder |first1=James |last2=O'Sullivan |first2=Jack |title=The Stanford Linear Accelerator Center (SLAC) |url=http://www.physics.ox.ac.uk/documents/PUS/dis/SLAC.htm |work=Physics Department. |publisher=University Of Oxford |access-date=16 November 2013 |url-status=dead |archive-url=https://web.archive.org/web/20130823223714/http://www.physics.ox.ac.uk/documents/PUS/dis/SLAC.htm |archive-date=23 August 2013 }} Construction began on the {{convert|3|km|mi|0|adj=mid|-long}} linear accelerator in 1962 and was completed in 1967, and in 1968 the first experimental evidence of quarks was discovered resulting in the 1990 Nobel Prize in Physics, shared by SLAC's Richard Taylor and Jerome I. Friedman and Henry Kendall of MIT.{{cite web|title=SLAC History|url=https://www6.slac.stanford.edu/about/slac-history.aspx|work=SLAC National Accelerator Laboratory|publisher=Stanford University|access-date=16 November 2013}} The accelerator came with a 20 GeV capacity for the electron acceleration, and while similar to Rutherford's scattering experiment, that experiment operated with alpha particles at only 7 MeV. In the SLAC case the incident particle was an electron and the target a proton, and due to the short wavelength of the electron (due to its high energy and momentum) it was able to probe into the proton.

The Stanford Positron Electron Asymmetric Ring (SPEAR) addition to the SLAC made further such discoveries possible, leading to the discovery in 1974 of the J/psi particle, which consists of a paired charm quark and anti-charm quark, and another Nobel Prize in Physics in 1976.

This was followed up with Martin Perl's announcement of the discovery of the tau lepton, for which he shared the 1995 Nobel Prize in Physics.

The SLAC aims to be a premier accelerator laboratory,{{cite web|title=Our Vision and Mission |url=https://www6.slac.stanford.edu/about/vision-and-mission.aspx |work=SLAC National Accelerator Laboratory |publisher=Stanford University |access-date=16 November 2013 |url-status=dead |archive-url=https://web.archive.org/web/20131128065649/https://www6.slac.stanford.edu/about/vision-and-mission.aspx |archive-date=28 November 2013 }} to pursue strategic programs in particle physics, particle astrophysics and cosmology, as well as the applications in discovering new drugs for healing, new materials for electronics and new ways to produce clean energy and clean up the environment.{{cite web|title=SLAC Overview|url=https://www6.slac.stanford.edu/about/slac-overview.aspx|work=SLAC National Accelerator Laboratory|publisher=Stanford University|access-date=16 November 2013}} Under the directorship of Chi-Chang Kao the SLAC's fifth director (as of November 2012), a noted X-ray scientist who came to SLAC in 2010 to serve as associate laboratory director for the Stanford Synchrotron Radiation Lightsource.{{cite web|title=Director's Office|url=https://www6.slac.stanford.edu/about/directors-office.aspx|work=SLAC National Accelerator Laboratory|publisher=Stanford University|access-date=16 November 2013}}

== BaBar ==

{{see also|BaBar experiment}}

== SSRL – Stanford Synchrotron Radiation Lightsource ==

{{see also|Stanford Synchrotron Radiation Lightsource}}

Other scientific programs run at SLAC include:{{cite web|title=Scientific Programs|url=https://www6-stage.slac.stanford.edu/research/scientific-programs.aspx|work=SLAC National Accelerator Laboratory|publisher=Stanford University|access-date=16 November 2013|archive-url=https://web.archive.org/web/20150915110117/https://www6-stage.slac.stanford.edu/research/scientific-programs.aspx|archive-date=15 September 2015|url-status=dead}}

  • Advanced Accelerator Research
  • ATLAS/Large Hadron Collider
  • Elementary Particle Theory
  • EXO – Enriched Xenon Observatory
  • FACET – Facility for Advanced Accelerator Experimental Tests
  • Fermi Gamma-ray Space Telescope
  • Geant4
  • KIPAC – Kavli Institute for Particle Astrophysics and Cosmology
  • LCLS – Linac Coherent Light Source
  • LSST – Large Synoptic Survey Telescope
  • NLCTA – Next Linear Collider Test Accelerator
  • Stanford PULSE Institute
  • SIMES – Stanford Institute for Materials and Energy Sciences
  • SUNCAT Center for Interface Science and Catalysis
  • Super CDMS – Super Cryogenic Dark Matter Search

= RIKEN RI Beam Factory =

{{see also|Radioactive Isotope Beam Factory}}

RIKEN was founded in 1917 as a private research foundation in Tokyo, and is Japan's largest comprehensive research institution. Having grown rapidly in size and scope, it is today renowned for high-quality research in a diverse range of scientific disciplines, and encompasses a network of world-class research centers and institutes across Japan.{{cite web|title=About RIKEN|url=http://www.riken.jp/en/about/|work=RIKEN|publisher=RIKEN, Japan|access-date=11 December 2013}}

The RIKEN RI Beam Factory, otherwise known as the RIKEN Nishina Centre (for Accelerator-Based Science), is a cyclotron-based research facility which began operating in 2007; 70 years after the first in Japanese cyclotron, from Dr. Yoshio Nishina whose name is given to the facility.{{cite web|title=About Nishina Center - Greeting|url=http://www.rarf.riken.go.jp/Eng/about/greeting.html|work=Nishina Center|publisher=RIKEN Nishina Center for Accelerator-Based Science|access-date=11 December 2013}}

As of 2006, the facility has a world-class heavy-ion accelerator complex. This consists of a K540-MeV ring cyclotron (RRC) and two different injectors: a variable-frequency heavy-ion linac (RILAC) and a K70-MeV AVF cyclotron (AVF). It has a projectile-fragment separator (RIPS) which provides RI (Radioactive Isotope) beams of less than 60 amu, the world's most intense light-atomic-mass RI beams.{{cite web|title=Facilities - RI Beam Factory (RIBF)|url=http://www.rarf.riken.go.jp/Eng/facilities/RIBF.html|work=Nishina Center|publisher=RIKEN Nishina Center for Accelerator-Based Science|access-date=11 December 2013}}

Overseen by the Nishina Centre, the RI Beam Factory is utilized by users worldwide promoting research in nuclear, particle and hadron physics. This promotion of accelerator applications research is an important mission of the Nishina Centre, and implements the use of both domestic and oversea accelerator facilities.{{cite web|title=About Nishina Center - Research Groups|url=http://www.rarf.riken.go.jp/Eng/about/group.html|work=Nishina Center|publisher=RIKEN Nishina Center for Accelerator-Based Science|access-date=11 December 2013}}

== SCRIT ==

{{see also|SCRIT}}

The SCRIT (Self-Confining Radioactive isotope Ion Target) facility, is currently under construction at the RIKEN RI beam factory (RIBF) in Japan. The project aims to investigate short-lived nuclei through the use of an elastic electron scattering test of charge density distribution, with initial testing done with stable nuclei. With the first electron scattering off unstable Sn isotopes to take place in 2014.{{cite journal |last1=Suda |first1=T. |last2=Adachi |first2=T. |last3=Amagai |first3=T. |last4=Enokizono |first4=A. |last5=Hara |first5=M. |last6=Hori |first6=T. |last7=Ichikawa |first7=S. |last8=Kurita |first8=K. |last9=Miyamoto |first9=T. |last10=Ogawara |first10=R. |last11=Ohnishi |first11=T. |last12=Shimakura |first12=Y. |last13=Tamae |first13=T. |last14=Togasaki |first14=M. |last15=Wakasugi |first15=M. |last16=Wang |first16=S. |last17=Yanagi |first17=K. |title=Nuclear physics at the SCRIT electron scattering facility |journal=Progress of Theoretical and Experimental Physics |date=17 December 2012 |volume=2012 |issue=1 |pages=3C008–0 |doi=10.1093/ptep/pts043 |bibcode=2012PTEP.2012cC008S|doi-access= }}

The investigation of short-lived radioactive nuclei (RI) by means of electron scattering has never been performed because of an inability to make these nuclei a target,{{cite web|last=Wakasugi|first=Masanori|title=SCRIT Team|url=http://www.riken.jp/en/research/labs/rnc/instrum_dev/scrit/|work=RIKEN Research|publisher=RIKEN Nishina Center for Accelerator-Based Science|access-date=19 November 2013}} now with the advent of a novel self-confining RI technique at the world's first facility dedicated to the study of the structure of short-lived nuclei by electron scattering this research becomes possible.

The principle of the technique is based around the ion trapping phenomenon which is observed at electron storage ring facilities,The residual gases in a storage ring are ionized by the circulating electron beam. Once they are ionized, they are trapped transversely by the electron beam. Since the trapped ions stay on the electron beam and kick electrons out of orbit, the results of this ion trapping are harmful for the performance of electron storage rings. This leads to shorter beam lifetime, and even beam instability when the trapping becomes severe. Thus, much effort has been paid so far to reducing the negative effects of ion trapping which has an adverse effect on the performance of electron storage rings.

The novel idea to be employed at SCRIT is to use the ion trapping to allow short-lived RI's to be made a target, as trapped ions on the electron beam, for the scattering experiments. This idea was first given a proof-of-principle study using the electron storage ring of Kyoto University, KSR; this was done using a stable nucleus of 133Cs as a target in an experiment of 120MeV electron beam energy, 75mA typical stored beam current and a 100 seconds beam lifetime. The results of this study were favorable with elastically scattered electrons from the trapped Cs being clearly visible.

See also

Notes

{{reflist|group=note}}

References

{{reflist|30em}}