Born approximation explained

Generally in scattering theory and in particular in quantum mechanics, the Born approximation consists of taking the incident field in place of the total field as the driving field at each point in the scatterer. The Born approximation is named after Max Born who proposed this approximation in early days of quantum theory development.^[1]

It is the perturbation method applied to scattering by an extended body. It is accurate if the scattered field is small compared to the incident field on the scatterer.

For example, the scattering of radio waves by a light styrofoam column can be approximated by assuming that each part of the plastic is polarized by the same electric field that would be present at that point without the column, and then calculating the scattering as a radiation integral over that polarization distribution.

Born approximation to the Lippmann–Schwinger equation

The Lippmann–Schwinger equation for the scattering state

\vert{\Psi ^{(\pm)} _{p} }\rangle with a momentum p and out-going (+) or in-going (-) boundary conditions is\vert{\Psi ^{(\pm)} _{p} }\rangle = \vert\rangle + G^\circ(E_p \pm i\epsilon) V \vert\rangle,

where

G ^{\circ} is the free particle Green's function, \epsilon is a positive infinitesimal quantity, and V the interaction potential. \vert{\Psi ^{\circ} _{p} }\rangle is the corresponding free scattering solution sometimes called the incident field. The factor \vert{\Psi ^{(\pm)} _{p} }\rangle on the right hand side is sometimes called the driving field.

Within the Born approximation, the above equation is expressed as

\vert{\Psi ^{(\pm)} _{p} }\rangle = \vert\rangle + G^\circ(E_p \pm i\epsilon) V \vert\rangle,

which is much easier to solve since the right hand side no longer depends on the unknown state

\vert{\Psi ^{(\pm)} _{p} }\rangle.

The obtained solution is the starting point of the Born series.

Born approximation to the scattering amplitude

Using the outgoing free Green's function for a particle with mass

m in coordinate space,G ^{( + )} ( r, r')=- (2m)/(\hbar ^{2}) (e ^{+ik|r-r'|})/(4 \pi| r- r'|) one can extract the Born approximation to the scattering amplitude from the Born approximation to the Lippmann–Schwinger equation above,f _{B(\theta) =- (m)/(2 \pi\hbar ^{2})} \int d ^{3r} e ^{iq ⋅} V( r) , where \theta is the angle between the incident wavevector k and the scattered wavevector k' , q= k'- k is the transferred momentum. In the centrally symmetric potential V = V(r) , the scattering amplitude becomes^[2] f _{B(\theta) =- (2 m)/(\hbar ^{2})} \int ^{inf ty} _{0} r V(r) (\sin qr)/(q) dr where q = | q|=2k\sin(\theta/2). In the Born approximation for centrally symmetric field, the scattering amplitude and thus the cross section \sigma depends on the momentum p = k/\hbar and the scattering amplitude \theta only through the combination p\sin(\theta/ 2 ) .

Applications

The Born approximation is used in several different physical contexts.

In neutron scattering, the first-order Born approximation is almost always adequate, except for neutron optical phenomena like internal total reflection in a neutron guide, or grazing-incidence small-angle scattering. The Born approximation has also been used to calculate conductivity in bilayer graphene^[3] and to approximate the propagation of long-wavelength waves in elastic media.^[4]

The same ideas have also been applied to studying the movements of seismic waves through the Earth.^[5]

Distorted-wave Born approximation

The Born approximation is simplest when the incident waves

\vert{\Psi ^{\circ} _{p} }\rangle are plane waves. That is, the scatterer is treated as a perturbation to free space or to a homogeneous medium.

In the distorted-wave Born approximation (DWBA), the incident waves are solutions

\vert{\Psi ^{1} _{p} }^\rangle to a part V ^{1} of the problem V = V ^{1} + V ^{2} that is treated by some other method, either analytical or numerical. The interaction of interest V is treated as a perturbation V ^{2} to some system V ^{1} that can be solved by some other method. For nuclear reactions, numerical optical model waves are used. For scattering of charged particles by charged particles, analytic solutions for coulomb scattering are used. This gives the non-Born preliminary equation\vert{\Psi ^{1} _{p} }^\rangle = \vert\rangle + G^\circ(E_p \pm i0) V^ \vert^\rangle

and the Born approximation

\vert{\Psi ^{(\pm)} _{p} }\rangle = \vert^\rangle + G^1(E_p \pm i0) V^ \vert^\rangle.

Other applications include bremsstrahlung and the photoelectric effect. For a charged-particle-induced direct nuclear reaction, the procedure is used twice. There are similar methods that do not use the Born approximations. In condensed-matter research, DWBA is used to analyze grazing-incidence small-angle scattering.

See also

• Born series
• Lippmann–Schwinger equation
• Dyson series
• Electromagnetic modeling
• Rayleigh–Gans approximation

References

• Book: Sakurai, J. J. . . Addison Wesley . 1994 . 0-201-53929-2.
• Book: Roger G. Newton

. Roger G. Newton . Newton, Roger G. . Scattering Theory of Waves and Particles . Dover Publications, inc. . 2002 . 0-486-42535-5.

• Wu and Ohmura, Quantum Theory of Scattering, Prentice Hall, 1962

Notes and References

1. Quantenmechanik der Stossvorgänge. Born . Max . Zeitschrift für Physik. 1926. 38. 11–12 . 803–827. 1926ZPhy...38..803B . 10.1007/BF01397184 . 126244962 .
2. Landau, L. D., & Lifshitz, E. M. (2013). Quantum mechanics: non-relativistic theory (Vol. 3). Elsevier.
3. Transport in bilayer graphene: Calculations within a self-consistent Born approximation . Koshino . Mikito . Ando . Tsuneya . Physical Review B . 2006 . 73 . 24 . 245403 . 10.1103/physrevb.73.245403. cond-mat/0606166 . 2006PhRvB..73x5403K . 119415260 .
4. The Born approximation in the theory of the scattering of elastic waves by flaws . Gubernatis . J.E. . Domany . E. . Krumhansl . J.A. . Huberman . M. . Journal of Applied Physics . 1977 . 48 . 7 . 2812–2819 . 10.1063/1.324142. 1977JAP....48.2812G .
5. The use of the Born approximation in seismic scattering problems . Hudson . J.A. . Heritage . J.R. . Geophysical Journal of the Royal Astronomical Society . 1980 . 66 . 1 . 221–240 . 10.1111/j.1365-246x.1981.tb05954.x. 1981GeoJ...66..221H . free .