Studying Green's function in many body physics

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SUMMARY

This discussion focuses on Green's function in many-body physics, addressing its definition, the physical meaning of self-energy, and its relation to experimental observables. The spectral function, derived from the retarded two-point correlation function, connects Green's function to physical quantities, revealing energy levels of the many-body system. Piers Coleman's textbook is recommended for in-depth understanding, particularly regarding the relationship between spectral functions and experimental observables, such as those obtained through Angle-Resolved Photoemission Spectroscopy (ARPES).

PREREQUISITES
  • Understanding of Green's function in quantum mechanics
  • Familiarity with many-body physics concepts
  • Knowledge of spectral functions and their significance
  • Basic principles of quantum field theory
NEXT STEPS
  • Study Piers Coleman's textbook on many-body physics for detailed insights
  • Learn about the derivation and applications of spectral functions
  • Research the role of self-energy in quasiparticle interactions
  • Explore experimental techniques like Angle-Resolved Photoemission Spectroscopy (ARPES)
USEFUL FOR

Physicists, graduate students in condensed matter physics, and researchers interested in many-body systems and their experimental implications.

Jeff Chen
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Hi,everyone. Recently, I am studying green's function in many body physics and suffer from trouble.Following are my problems.
(1) What is the origin of the definition of green's function in many body physics?
(2) What is the physical meaning of self energy ? It seems like it is the correction due to interaction with environment and is it similar to the concept of quasi-particle and mass renormolization ?
(3)If we know the green's function for a certain system,what physical quantity can we obtain?
 
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It seems that all three of your questions concern what the relation is between the Green's function in many-body physics and physical/experimental observables. One very clear connection is the fact that the spectral function is obtained from the retarded two-point correlation function as
$$
\rho(\omega) = \mathrm{Im} G_{\mathrm{R}}(\omega) = \pi \sum_{\alpha} | \langle \alpha | \psi | 0 \rangle|^2 \left[ \delta(\omega - E_{\alpha} + E_0) \mp \delta(\omega + E_{\alpha} - E_0) \right]
$$
where the upper (lower) sign is for bosons (fermions). But this form - a matrix element times a delta function constraining energy conservation - is precisely the form of Fermi's Golden Rule which computes the transition rate of time-dependent processes which couple to the operator ##\psi#. In addition, this object is only nonzero at precisely the frequencies where the many-body system has energy levels, so it tells you about the spectrum of your system. These two facts result in a lot of relations between experimental observables and spectral functions.

For more details, Piers Coleman's many-body textbook has about half a chapter devoted to relating spectral functions to various experimental observables in different systems. It is far more detailed and clear than anything I could write up here, so I highly recommend checking it out.
 
You get the single-particle spectral function A(k,ω) from the imaginary part of the Green's function. This spectral function is useful because it is accessible via experiment (example: ARPES).

The self-energies in A(k,ω) contains the type of scattering or interactions that surrounds the quasiparticle. The imaginary part of the self-energy, for example, allows us to see the origin of the broadening of A(k,ω) peaks and gives us information about the underlying interactions that are going on.

Zz.
 

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