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In quantum field theory, the energy that a particle has as a result of changes that it causes in its environment defines its self-energy \Sigma. The self-energy represents the contribution to the particle's , or effective mass, due to interactions between the particle and its environment. In , the energy required to assemble the charge distribution takes the form of self-energy by bringing in the constituent charges from infinity, where the electric force goes to zero. In a context, self-energy is used to describe interaction induced renormalization of mass (dispersions) and lifetime. Self-energy is especially used to describe electron-electron interactions in Fermi liquids. Another example of self-energy is found in the context of softening due to electron-phonon coupling.


Characteristics
Mathematically, this energy is equal to the so-called on mass shell value of the proper self-energy operator (or proper mass operator) in the momentum-energy representation (more precisely, to times this value). In this, or other representations (such as the space-time representation), the self-energy is pictorially (and economically) represented by means of , such as the one shown below. In this particular diagram, the three arrowed straight lines represent particles, or particle , and the wavy line a particle-particle interaction; removing (or amputating) the left-most and the right-most straight lines in the diagram shown below (these so-called external lines correspond to prescribed values for, for instance, momentum and energy, or ), one retains a contribution to the self-energy operator (in, for instance, the momentum-energy representation). Using a small number of simple rules, each Feynman diagram can be readily expressed in its corresponding algebraic form.

In general, the on-the-mass-shell value of the self-energy operator in the momentum-energy representation is . In such cases, it is the real part of this self-energy that is identified with the physical self-energy (referred to above as particle's "self-energy"); the inverse of the imaginary part is a measure for the lifetime of the particle under investigation. For clarity, elementary excitations, or (see ), in interacting systems are distinct from stable particles in vacuum; their state functions consist of complicated superpositions of the eigenstates of the underlying many-particle system, which only momentarily, if at all, behave like those specific to isolated particles; the above-mentioned lifetime is the time over which a dressed particle behaves as if it were a single particle with well-defined momentum and energy.

The self-energy operator (often denoted by \Sigma_{}^{}, and less frequently by M_{}^{}) is related to the bare and dressed propagators (often denoted by G_0^{} and G_{}^{} respectively) via the Dyson equation (named after ):

G = G_0^{} + G_0 \Sigma G.

Multiplying on the left by the inverse G_0^{-1} of the operator G_0 and on the right by G^{-1} yields

\Sigma = G_0^{-1} - G^{-1}.

The and do not get a mass through because protects them from getting a mass. This is a consequence of the Ward identity. The and the get their masses through the ; they do undergo mass renormalization through the renormalization of the theory.

Neutral particles with internal quantum numbers can mix with each other through production. The primary example of this phenomenon is the mixing of neutral . Under appropriate simplifying assumptions this can be described without quantum field theory.


Other uses
In , the self-energy or Born energy of an ion is the energy associated with the field of the ion itself.

In solid state and condensed-matter physics self-energies and a myriad of related properties are calculated by Green's function methods and Green's function (many-body theory) of interacting low-energy excitations on the basis of electronic band structure calculations. Self-energies also find extensive application in the calculation of particle transport through open quantum systems and the embedding of sub-regions into larger systems (for example the surface of a semi-infinite crystal).


See also

  • A. L. Fetter, and J. D. Walecka, Quantum Theory of Many-Particle Systems (McGraw-Hill, New York, 1971); (Dover, New York, 2003)
  • J. W. Negele, and H. Orland, Quantum Many-Particle Systems (Westview Press, Boulder, 1998)
  • A. A. Abrikosov, L. P. Gorkov and I. E. Dzyaloshinski (1963): Methods of Quantum Field Theory in Statistical Physics Englewood Cliffs: Prentice-Hall.
  • (2025). 9780521529808, Cambridge University Press.
  • A. N. Vasil'ev The Field Theoretic Renormalization Group in Critical Behavior Theory and Stochastic Dynamics (Routledge Chapman & Hall 2004); ;
  • (2025). 9780750310420, IOP Publishing.

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