oscillator strength
{{Short description|Dimensionless quantity in spectroscopy}}
In spectroscopy, oscillator strength is a dimensionless quantity that expresses the probability of absorption or emission of electromagnetic radiation in transitions between energy levels of an atom or molecule.{{cite book|author=W. Demtröder|title=Laser Spectroscopy: Basic Concepts and Instrumentation|url=https://books.google.com/books?id=dNx1OLgn1xcC|accessdate=26 July 2013|year=2003|publisher=Springer|isbn=978-3-540-65225-0|page=31}}{{cite book|author=James W. Robinson|title=Atomic Spectroscopy|url=https://books.google.com/books?id=BNqp0RO7DXcC&pg=PA26|accessdate=26 July 2013|year=1996|publisher=MARCEL DEKKER Incorporated|isbn=978-0-8247-9742-3|pages=26–}} For example, if an emissive state has a small oscillator strength, nonradiative decay will outpace radiative decay. Conversely, "bright" transitions will have large oscillator strengths.{{Cite journal|last1=Westermayr|first1=Julia|last2=Marquetand|first2=Philipp|date=2021-08-25|title=Machine Learning for Electronically Excited States of Molecules|journal=Chemical Reviews|language=en|volume=121|issue=16|pages=9873–9926|doi=10.1021/acs.chemrev.0c00749|issn=0009-2665|pmc=8391943|pmid=33211478}} The oscillator strength can be thought of as the ratio between the quantum mechanical transition rate and the classical absorption/emission rate of a single electron oscillator with the same frequency as the transition.{{cite journal|last1=Hilborn|first1=Robert C.|title=Einstein coefficients, cross sections, f values, dipole moments, and all that|journal=American Journal of Physics|volume=50|issue=11|year=1982|pages=982–986|issn=0002-9505|doi=10.1119/1.12937|arxiv=physics/0202029|bibcode = 1982AmJPh..50..982H |s2cid=119050355}}
Theory
An atom or a molecule can absorb light and undergo a transition from
one quantum state to another.
The oscillator strength of a transition from a lower state
to an upper state may be defined by
:
f_{12} = \frac{2 }{3}\frac{m_e}{\hbar^2}(E_2 - E_1) \sum_{\alpha=x,y,z}
| \langle 1 m_1 | R_\alpha | 2 m_2 \rangle |^2,
where is the mass of an electron and is
the reduced Planck constant. The quantum states 1,2, are assumed to have several
degenerate sub-states, which are labeled by . "Degenerate" means
that they all have the same energy .
The operator is the sum of the x-coordinates
of all electrons in the system, i.e.
:
R_\alpha = \sum_{i=1}^N r_{i,\alpha}.
The oscillator strength is the same for each sub-state .
The definition can be recast by inserting the Rydberg energy and Bohr radius
:
f_{12} = \frac{E_2 - E_1}{3\, \text{Ry}} \frac{\sum_{\alpha=x,y,z}
| \langle 1 m_1 | R_\alpha | 2 m_2 \rangle |^2}{a_0^2}.
In case the matrix elements of are the same, we can get rid of the sum and of the 1/3 factor
:
f_{12} = 2\frac{m_e}{\hbar^2}(E_2 - E_1) \, | \langle 1 m_1 | R_x | 2 m_2 \rangle |^2.
Thomas–Reiche–Kuhn sum rule
To make equations of the previous section applicable to the states belonging to the continuum spectrum, they should be rewritten in terms of matrix elements of the momentum . In absence of magnetic field, the Hamiltonian can be written as , and calculating a commutator in the basis of eigenfunctions of results in the relation between matrix elements
:
x_{nk}=-\frac{i\hbar/m}{E_n-E_k}(p_x)_{nk}.
.
Next, calculating matrix elements of a commutator in the same basis and eliminating matrix elements of , we arrive at
:
\langle n|[p_x,x]|n\rangle=\frac{2i\hbar}{m}\sum_{k\neq n} \frac{|\langle n|p_x|k\rangle|^2}{E_n-E_k}.
Because , the above expression results in a sum rule
:
\sum_{k\neq n}f_{nk}=1,\,\,\,\,\,f_{nk}=-\frac{2}{m}\frac{|\langle n|p_x|k\rangle|^2}{E_n-E_k},
where are oscillator strengths for quantum transitions between the states and . This is the Thomas-Reiche-Kuhn sum rule, and the term with has been omitted because in confined systems such as atoms or molecules the diagonal matrix element due to the time inversion symmetry of the Hamiltonian . Excluding this term eliminates divergency because of the vanishing denominator.{{cite book|author1=Edward Uhler Condon|author2=G. H. Shortley|title=The Theory of Atomic Spectra|url=https://books.google.com/books?id=hPyD-Nc_YmgC|accessdate=26 July 2013|year=1951|publisher=Cambridge University Press|isbn=978-0-521-09209-8|page=108}}
Sum rule and electron effective mass in crystals
In crystals, the electronic energy spectrum has a band structure . Near the minimum of an isotropic energy band, electron energy can be expanded in powers of as where is the electron effective mass. It can be shown{{cite journal |doi=10.1103/PhysRev.97.869|title=Motion of Electrons and Holes in Perturbed Periodic Fields|journal=Physical Review|volume=97|issue=4|pages=869|year=1955|last1=Luttinger|first1=J. M.|last2=Kohn|first2=W.|bibcode=1955PhRv...97..869L}} that it satisfies the equation
:
\frac{2}{m}\sum_{k\neq n}\frac{|\langle n|p_x|k\rangle|^2}{E_k-E_n}+\frac{m}{m^*}=1.
Here the sum runs over all bands with . Therefore, the ratio of the free electron mass to its effective mass in a crystal can be considered as the oscillator strength for the transition of an electron from the quantum state at the bottom of the band into the same state.{{cite book|publisher=Springer|location=Berlin | doi=10.1007/978-3-642-91116-3_3| chapter=Elektronentheorie der Metalle| title=Aufbau Der Zusammenhängenden Materie| pages=333| year=1933| last1=Sommerfeld| first1=A.| last2=Bethe| first2=H.| isbn=978-3-642-89260-8}}