Scattering Rate
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A formula may be derived mathematically for the rate of
scattering Scattering is a term used in physics to describe a wide range of physical processes where moving particles or radiation of some form, such as light or sound, are forced to deviate from a straight trajectory by localized non-uniformities (including ...
when a beam of electrons passes through a material.


The interaction picture

Define the unperturbed Hamiltonian by H_0, the time dependent perturbing Hamiltonian by H_1 and total Hamiltonian by H. The eigenstates of the unperturbed Hamiltonian are assumed to be : H=H_0+H_1\ : H_0 , k\rang = E(k), k\rang In the interaction picture, the state ket is defined by : , k(t)\rang _I= e^ , k(t)\rang_S= \sum_ c_(t) , k'\rang By a
Schrödinger equation The Schrödinger equation is a linear partial differential equation that governs the wave function of a quantum-mechanical system. It is a key result in quantum mechanics, and its discovery was a significant landmark in the development of the ...
, we see : i\hbar \frac , k(t)\rang_I=H_, k(t)\rang_I which is a Schrödinger-like equation with the total H replaced by H_. Solving the
differential equation In mathematics, a differential equation is an equation that relates one or more unknown functions and their derivatives. In applications, the functions generally represent physical quantities, the derivatives represent their rates of change, an ...
, we can find the coefficient of n-state. : c_(t) =\delta_ - \frac \int_0^t dt' \;\lang k', H_1(t'), k\rang \, e^ where, the zeroth-order term and first-order term are :c_^=\delta_ :c_^=- \frac \int_0^t dt' \;\lang k', H_1(t'), k\rang \, e^


The transition rate

The probability of finding , k'\rang is found by evaluating , c_(t), ^2. In case of constant perturbation,c_^ is calculated by :c_^=\frac(1-e^) :, c_(t), ^2= , \lang\ k', H_1, k\rang , ^2\frac \frac Using the equation which is :\lim_ \frac \frac= \delta(x) The transition rate of an electron from the initial state k to final state k' is given by :P(k,k')=\frac , \lang\ k', H_1, k\rang , ^2 \delta(E_-E_k) where E_k and E_ are the energies of the initial and final states including the perturbation state and ensures the \delta-function indicate energy conservation.


The scattering rate

The scattering rate w(k) is determined by summing all the possible finite states k' of
electron scattering Electron scattering occurs when electrons are deviated from their original trajectory. This is due to the electrostatic forces within matter interaction or, if an external magnetic field is present, the electron may be deflected by the Lorentz fo ...
from an initial state k to a final state k', and is defined by :w(k)=\sum_P(k,k')=\frac \sum_ , \lang\ k', H_1, k\rang , ^2 \delta(E_-E_k) The integral form is :w(k)=\frac \frac \int d^3k' , \lang\ k', H_1, k\rang , ^2 \delta(E_-E_k)


References

* * {{DEFAULTSORT:Scattering Rate Semiconductor technology