At finite temperatures, one assumes that the particle, either electron or
phonon, is interacting with a bath of other particles. The exact state of all
these other particles is not known, since they are fluctuating between
different configurations. At finite temperature under thermodynamic equilibrium
the state of a system is described by the equilibrium density operator
(see Appendix C). In treating such
systems, it will be most convenient to use the grand canonical ensemble, which
allows for a variable number of particles. Therefore, the system is considered
to be in contact with a heat bath of temperature and a particle reservoir
characterized by the FERMI energy
. With the definition
, where is the particle
number operator, the statistical operator can be written as
(3.10)
where the short-hand notation
is used. The operator
may be interpreted as a grand canonical HAMILTONian. Given
the density operator, the ensemble average of any operator can be
calculated as
(3.11)
Therefore, the single-particle GREEN's function at finite temperature can be
defined as
(3.12)
At this stage, this form of the GREEN's function does not admit the
WICK decomposition, because the WICK theorem described in Section 3.4.1
requires a dependence on the non-interacting HAMILTONian for both
the field operators and the thermal average. A way around this problem is the
MATSUBARA technique [193], where one introduces a complex time
and a new physical quantity, the MATSUBARA (imaginary time) GREEN's
function
. The representation of
operators with imaginary time arguments is given
in Appendix B.5.