Scattering theory - phase shift - best approx.

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SUMMARY

The discussion focuses on the calculation of the phase shift \(\delta_l\) in scattering theory, specifically within quantum mechanics (QM). Two primary methods are highlighted: the semi-classical approach, defined by the integral \(\delta_l = \int^{r}_{r_0} k(r')dr' - kr\), and the first-order Born approximation, expressed as \(-\frac{\tan \delta_l}{k} = \langle u^0_l | U | u^0_l \rangle\). The first-order Born approximation is established as the preferred method due to its validity under the condition \(\frac{m | V_0 | a^2}{\hbar^2} \ll 1\), which ensures more accurate results compared to the semi-classical method. Additionally, the second Born approximation can further refine the results.

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  • Understanding of quantum mechanics principles
  • Familiarity with scattering theory concepts
  • Knowledge of phase shifts in wave functions
  • Proficiency in mathematical integration techniques
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  • Study the derivation and applications of the first-order Born approximation
  • Explore the conditions for the validity of the Born approximation in various potentials
  • Learn about the second Born approximation and its refinements in scattering calculations
  • Investigate the role of wave numbers in quantum scattering problems
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Students and researchers in quantum mechanics, particularly those focusing on scattering theory, phase shifts, and approximation methods in quantum calculations.

jonas_nilsson
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Hi all,

we're looking at scattering theory in the QM course right now, and I've got a question concerning the approximative ways of calculating the phase shift [tex]\delta_l[/tex] of the partial waves in the partial wave expansion of the scattered wave.

One way (the semi-classical) to calculate it is through
[tex]\delta_l = \int^{r}_{r_0} k(r')dr' - kr[/tex],
where [tex]r_0[/tex] is the "border" of the classically allowed area for the particle(s) and [tex]k(r)[/tex] is the "local" wave number (right choice of word :confused:).

The other way is through the 1st order Born approximation:
[tex]-\frac{tan ~\delta_l}{k} = <u^0_l | U | u^0_l>[/tex]

Now if I remember right the second method was presented as the for sure preferred one. My question is: how's that?. How can we be sure that this is the best way. The clue might be that the first is (semi-) classical, but on the other hand it seems quite rough to just use the [tex]u_l[/tex] of a free particle, that is [tex]u_l^0[/tex]. It must be very depending on the kind of scattering potential we're dealing with, or?
 
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The criterion for the validity of the Born approximation is
$$
\frac{m | V_0 | a^2}{\hbar^2} \ll 1
$$
where ##m## is the mass of the particle, ##V_0## and ##a## the height and range of the potential, respectively. Therefore, if this condition is met, then the Born approximation is a good approximation, and the result will be better than using a semi-classical approximation. One can also go further and use the second Born approximation to refine the result.
 

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