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Scattering Theory: Revised and corrected

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1 Scattering Theory: Revised and corrected 2004-2007
Classical Scattering: Differential and total cross section Examples: Hard sphere and Coulomb scattering Quantal Scattering: Formulated as a stationary problem Integral Equation Born Approximation Examples: Hard sphere and Coulomb scattering

2 The Scattering Cross Section
out N out Number of scattered particles into : Differential Cross Section: Total Cross Section:

3 Quantal Scattering - No Trajectory
Quantal Scattering - No Trajectory! (A plane wave hits some object and a spherical wave emerges) Procedure: Solve the time independent Schrödinger equation Approximate the solution to one which is valid far away from the scattering center Write the solution as a sum of an incoming plane wave and an outgoing spherical wave. Must find a relation between the wavefunction and the current densities that defines the cross section.

4 Current Density: Incomming current density: Outgoing spherical current density:

5

6 Example - Classical scattering:
Hard Sphere scattering: = Geometrical Cross sectional area of sphere! Independent of angles!

7

8

9 The Schrödinger equation - scattering form:
Now we must define the current densities from the wave function…

10 The final expression:

11 Summary Write the Schrödinger equation as: Asymptotics: Then we have:
…. Now we can start to work

12 Integral equation where we require: because….
With the rewritten Schrödinger equation we can introducea Greens function, which (almost) solves the problem for a delta-function potential: Then a solution of: can be written: where we require: because….

13 This term is 0 This equals Integration over the delta function gives result: Formal solution: Useless so far!

14 Note: solves the problem! Must find G(r) in and: Then: The function:
”Proof”: The integral can be evaluated, and the result is:

15 Inserting G(r), we obtain:
implies that: Inserting G(r), we obtain: At large r this can be recast to an outgoing spherical wave….. The Born series: And so on…. Not necesarily convergent!

16 Write the Schrödinger equation as:
Asymptotics: SUMMARY We obtains: At large r this can be recast to an outgoing spherical wave….. The Born series: And so on…. Not necesarily convergent!

17 Asymptotics - Detector is at near infinite r
The potential is assumed to have short range, i.e. Active only for small r’ : 1) 2) Asymptotic excact result: Still Useless!

18 The Born approximation:
Use incomming wave instead of Under integration sign: The scattering amplitude is then: :) The momentum change Fourier transform of the potential! Valid when: Weak potentials and/or large energies!

19 Spheric Symmetric potentials:
Total Cross Section:

20 Summary - 1’st. Born Approximation:
Best at large energies!

21 Example - Hard sphere 1. Born scattering:
Classical Hard Sphere scattering: Quantal Hard Sphere potential: Thats it! Depends on angles - but roughly independent when qR << 1

22 Approximation methods in Quantum Mechanics
Kap. 7-lect2 Introduction to Approximation methods in Quantum Mechanics Time dependent Time-independent methods: Methods to obtain an approximate eigen energy, E and wave function: Golden Rule perturbation methods Methods to obtain an approximate expression for the expansion amplitudes. Ground/Bound states Continuum states Perturbation theory Variational method Scattering theory Non degenerate states Degenerate states


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