Time dependent pertubation theory

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SUMMARY

The discussion centers on time-dependent perturbation theory in quantum mechanics, specifically the equation iħ∂/∂t c_n(t) = ∑_m V_nm e^(iω_nm t)c_m(t), where ω_nm = (E_n - E_m)/ħ. This equation arises from the time-dependent Schrödinger equation and describes how the expansion coefficients c_n evolve over time. The interaction potential V_nm represents the coupling between states m and n, with larger values indicating stronger coupling. Understanding this equation is crucial for calculating approximate values of coefficients and average physical quantities.

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  • Quantum Mechanics fundamentals
  • Time-dependent Schrödinger equation
  • Complex exponential functions
  • Understanding of scattering theory
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  • Study the derivation of the time-dependent Schrödinger equation
  • Explore the implications of scattering channels in quantum mechanics
  • Learn about the interaction picture in quantum mechanics
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Students of quantum mechanics, physicists exploring perturbation theory, and researchers interested in quantum state interactions and scattering processes.

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Okey, so I´m taking a course in QM and I feel that I got a grip of most of it.
But then we arrive at this formulea <br /> i\hbar\frac{\partial}{\partial t} c_n(t) = \sum_m \hat{V}_{nm} e^{i\omega_{nm} t}c_m(t),<br /> where <br /> \omega_{nm} \equiv \frac{(E_n - E_m)}{\hbar}.<br />
In other words time dependent pertubation theory. And I just feel confused. I don't know how to start tackle it with my intuition.

What are, in your opinion, the first intuitional things I should remark when it comes to this equation? What does it tell about my physics without having to do some big derivations?

Thanks!
 
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The equation is a consequence of time-dependent Schrödinger equation. It is a rule that the expansion coefficients c_n obey. This equation can be used to find approximate values of c's, and afterwards these can be used to find average values of physical quantities.
Does this help?
 
I think intuitively Vnm represents scattering channels, a coupling of an m state to an n state in the interaction picture. The bigger the V, the bigger the coupling.

The fact that V nm depends on time is not that important.
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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