2005, Vol.8, No.1, pp.10-18
In this work a new approach to studies in quantum and
statistical mechanics of the Early Universe (at Plank scale) is
proposed - the density matrix deformation approach. A deformation
of a particular theory is understood as its extension through one
or several parameters in such a way that the initial theory
appears in the limiting transition.
The distinguishing feature of the proposed approach in comparison
to the previous ones lies in the fact that here a deformed object
is the density matrix rather than the commutators as it has been
so far in case of quantum mechanics. The deformation parameter is
dimensionless in the finite interval. The implications and
applications of the above approach are explicitly demonstrated for
the solution of the following problems: Liouville equation
modifications in processes associated with inflation and black
holes, Hawking information paradox by the different approaches
(S.Hawking and R.Penrose). It is shown that the developed methods
enable one to obtain from the basic principles the
Bekenstein-Hawking formula for the black hole entropy in
semiclassical approximation.Also it is shown that high entropy for
Planck's remnants of black holes appearing in the assumption of
the Generalized Uncertainty Relations may be explained within the
scope of the density matrix entropy introduced by the first author
previously. It is noted that the suggested paradigm is consistent
with the Holographic Principle. Because of this, a conjecture is
made about the possibility for obtaining the Generalized
Uncertainty Relations from the covariant entropy bound at high
energies in the same way as R.Bousso has derived Heisenberg's
uncertainty principle for the flat space. Deformation in
statistical mechanics at Planck scale is constructed in similar
way with the statistical density matrix as a primary object. The
principal difference is the deformation parameter that is
associated with a maximum temperature rather than with the
fundamental length like in the first case. Some obvious
implications are also presented with the formula for a
high-temperature complement to the canonical Gibbs distribution.
Besides, a generalization of the thermodynamic uncertainty
relations is proposed. It is done by introducing of an additional
term proportional to the interior energy into the standard
thermodynamic uncertainty relation that leads to existence of the
lower limit of inverse temperature.
Key words:
deformed density
matrix in Quantum and Statistical Mechanics at Plank's Scale,
density of entropy, Holographic Principle, Generalized Uncertainty
Relations in Thermodynamics
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