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The correlation function can be interpreted physically as the amplitude for propagation of a particle or excitation between y and x. In the free theory, it is simply the Feynman propagator (for n=2).<ref>{{cite book|last1=Peskin|first1=Michael|last2=Schroeder|first2=David|title=An Introduction to Quantum Field Theory|publisher=Addison-Wesley}}</ref>
The correlation function can be interpreted physically as the amplitude for propagation of a particle or excitation between y and x. In the free theory, it is simply the Feynman propagator (for n=2).<ref>{{cite book|last1=Peskin|first1=Michael|last2=Schroeder|first2=David|title=An Introduction to Quantum Field Theory|publisher=Addison-Wesley}}</ref>


Very important note : [Mohamed 15/08/2018]
* Very important note : [Mohamed 15/08/2018]
These (n) field operators at different positions , can be discribe according to Smarr's formula, the thermodynamics of black holes connect the mass M of a black hole to the surface A of its horizon and its possible kinetic moment L and electric charge Q:
These (n) field operators at different positions , can be discribe according to Smarr's formula, the thermodynamics of black holes connect the mass M of a black hole to the surface A of its horizon and its possible kinetic moment L and electric charge Q:
M=M(A,L,Q).
M=M(A,L,Q).

Revision as of 17:49, 15 August 2018

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In quantum field theory, the (real space) n-point correlation function is defined as the functional average (functional expectation value) of a product of field operators at different positions

For time-dependent correlation functions, the time-ordering operator is included.

Correlation functions are also called simply correlators. Sometimes, the phrase Green's function is used not only for two-point functions, but for any correlators.

The correlation function can be interpreted physically as the amplitude for propagation of a particle or excitation between y and x. In the free theory, it is simply the Feynman propagator (for n=2).[1]

  • Very important note : [Mohamed 15/08/2018]

These (n) field operators at different positions , can be discribe according to Smarr's formula, the thermodynamics of black holes connect the mass M of a black hole to the surface A of its horizon and its possible kinetic moment L and electric charge Q:

M=M(A,L,Q).

It is nevertheless possible, using the appropriate variable change, to use Euler's theorem, which then gives:

M= kA/4[phi] +2ΩL+VQ.

with κ: surface gravity; 2Ω: velocity of the nuclear vector of particle transport proportional to the speed of light wave = f. λ where f is the frequency of the wave and λ is its length; V is and the electric potential of the black hole. L is the quantum kinetic moment and plays a fundamental role in atomic and molecular physics, in the classification of electronic terms.

See also

References

  1. ^ Peskin, Michael; Schroeder, David. An Introduction to Quantum Field Theory. Addison-Wesley.

Further reading