Klein–Nishina formula explained

In particle physics, the Klein–Nishina formula gives the differential cross section (i.e. the "likelihood" and angular distribution) of photons scattered from a single free electron, calculated in the lowest order of quantum electrodynamics. It was first derived in 1928 by Oskar Klein and Yoshio Nishina, constituting one of the first successful applications of the Dirac equation.^[1] The formula describes both the Thomson scattering of low energy photons (e.g. visible light) and the Compton scattering of high energy photons (e.g. x-rays and gamma-rays), showing that the total cross section and expected deflection angle decrease with increasing photon energy.

Formula

For an incident unpolarized photon of energy

E _{\gamma} , the differential cross section is:^[2] (d\sigma)/(d\Omega) = (1)/(2) r ^{2} _{e} \left( (λ)/(λ ') \right) ^{2} \left[ (λ)/(λ ') + (λ ')/(λ) - \sin ^{2(\theta)\right]}

where

r _{e} is the classical electron radius (~2.82 fm, r ^{2} _{e} is about 7.94 × 10⁻³⁰ m² or 79.4 mb)λ / λ ' is the ratio of the wavelengths of the incident and scattered photons\theta is the scattering angle (0 for an undeflected photon).

The angular dependent photon wavelength (or energy, or frequency) ratio is

(λ)/(λ ') = (E _{\gamma'})/(E _{\gamma}) = (\omega')/(\omega) = (1)/(1+ \epsilon( 1- \cos\theta))

as required by the conservation of relativistic energy and momentum (see Compton scattering). The dimensionless quantity

\epsilon = E _{\gamma/m} _{e} c ^{2} expresses the energy of the incident photon in terms of the electron rest energy (~511 keV), and may also be expressed as \epsilon = λ _{c/λ} , where λ _{c} = h/m _{e} c is the Compton wavelength of the electron (~2.42 pm). Notice that the scatter ratio λ '/ λ increases monotonically with the deflection angle, from 1 (forward scattering, no energy transfer) to 1+2 \epsilon (180 degree backscatter, maximum energy transfer).

In some cases it is convenient to express the classical electron radius in terms of the Compton wavelength:

r _{e=\alpha} \bar λ _{c} = \alpha λ _{c/2\pi} , where \alpha is the fine structure constant (~1/137) and \bar λ _{c=\hbar/m} _{e} c is the reduced Compton wavelength of the electron (~0.386 pm), so that the constant in the cross section may be given as:(1)/(2) r ^{2} _{e} = (1)/(2) \alpha ^{2} _{c} = (\alpha ^{2} _{c})/(8 \pi ^{2}) = (\alpha ^{2\hbar} ^{2})/(2 m ^{2 c} _{e} ^{2})

Polarized photons

If the incoming photon is polarized, the scattered photon is no longer isotropic with respect to the azimuthal angle. For a linearly polarized photon scattered with a free electron at rest, the differential cross section is instead given by:

(d\sigma)/(d\Omega) = (1)/(2) r ^{2} _{e} \left( (λ)/(λ ') \right) ^{2} \left[ (λ)/(λ ') + (λ ')/(λ) - 2 \sin ^{2(\theta)} \cos ^{2} (\phi)\right] where \phi is the azimuthal scattering angle. Note that the unpolarized differential cross section can be obtained by averaging over \cos ^{2} (\phi) .

Limits

Low energy

For low energy photons the wavelength shift becomes negligible (

λ / λ ' ≈ 1 ) and the Klein–Nishina formula reduces to the classical Thomson expression:(d\sigma)/(d\Omega) ≈ (1)/(2) r ^{2} _{e} \left( 1 + \cos ^{2(\theta)\right)} (\epsilon \ll 1 ) which is symmetrical in the scattering angle, i.e. the photon is just as likely to scatter backwards as forwards. With increasing energy this symmetry is broken and the photon becomes more likely to scatter in the forward direction.

High energy

For high energy photons it is useful to distinguish between small and large angle scattering. For large angles, where

\epsilon( 1- \cos\theta) \gg 1 , the scatter ratio λ '/ λ is large and(d\sigma)/(d\Omega) ≈ (1)/(2) r ^{2} _{e} (λ)/(λ ') ≈ (1)/(2) r ^{2} _{e} (1)/(1+ \epsilon( 1- \cos\theta)) (\epsilon \gg 1 , \theta \gg \epsilon ^{-1/2} ) showing that the (large angle) differential cross section is inversely proportional to the photon energy.

The differential cross section has a constant peak in the forward direction:

\left( (d\sigma)/(d\Omega) \right) _{\theta=0} = r ^{2} _{e} independent of \epsilon . From the large angle analysis it follows that this peak can only extend to about \theta _{c} ≈ \epsilon ^{-1/2} . The forward peak is thus confined to a small solid angle of approximately \pi\theta ^{2} _{c} , and we may conclude that the total small angle cross section decreases with \epsilon ^{-1} .

Total cross section

The differential cross section may be integrated to find the total cross section:

\sigma = 2 \pi r ^{2} _{e} l [ (1+ \epsilon)/(\epsilon ^{3}) l ( (2 \epsilon ( 1+ \epsilon))/(1+2 \epsilon) - ln {( 1 + 2 \epsilon)} r ) + (ln {( 1+2 \epsilon))/() } - \frac \Biggr]

In the low-energy limit there is no energy dependence, and we recover the Thomson cross section (~66.5 fm²):

\sigma ≈ (8)/(3) \pi r ^{2} _{e} (E _{\gamma} \ll m _{e} c ^{2)}

History

The Klein–Nishina formula was derived in 1928 by Oskar Klein and Yoshio Nishina, and was one of the first results obtained from the study of quantum electrodynamics. Consideration of relativistic and quantum mechanical effects allowed development of an accurate equation for the scattering of radiation from a target electron. Before this derivation, the electron cross section had been classically derived by the British physicist and discoverer of the electron, J.J. Thomson. However, scattering experiments showed significant deviations from the results predicted by the Thomson cross section. Further scattering experiments agreed perfectly with the predictions of the Klein–Nishina formula.

See also

• Synchrotron radiation
• Yoshio Nishina
• Oskar Klein

Further reading

• Book: Evans, R. D. . The Atomic Nucleus . McGraw-Hill . New York . 1955 . 674–676 . 542611 .
• Book: Melissinos, A. C. . Experiments in Modern Physics . Academic Press . New York . 1966 . 252–265 . 0-12-489850-5 .
• Book: O. . Klein . Y. . Nishina . On the Scattering of Radiation by Free Electrons According to Dirac's New Relativistic Quantum Dynamics . The Oskar Klein Memorial Lectures, Vol. 2: Lectures by Hans A. Bethe and Alan H. Guth with Translated Reprints by Oskar Klein . Gösta . Ekspong . World Scientific . Singapore . 1994 . 113–139 . 1994okml.book.....E .

Notes and References

1. 10.1007/BF01366453 . Klein, O . Nishina, Y . Über die Streuung von Strahlung durch freie Elektronen nach der neuen relativistischen Quantendynamik von Dirac. Z. Phys.. 52 . 11–12 . 1929. 853 and 869. 1929ZPhy...52..853K . 123905506 .
2. Book: Weinberg, Steven . The Quantum Theory of Fields. I. 1995. 362–9.