Back to Search Start Over

PERTURBATIVELY DEFINED EFFECTIVE CLASSICAL POTENTIAL IN CURVED SPACE.

Authors :
Kleinert, H.
Chervyakov, A.
Source :
International Journal of Modern Physics A: Particles & Fields; Gravitation; Cosmology; Nuclear Physics; 12/10/2003, Vol. 18 Issue 30, p5521-5539, 19p
Publication Year :
2003

Abstract

The partition function of a quantum statistical system in flat space can always be written as an integral over a classical Boltzmann factor exp[-βV[sup eff cl](x[sub 0])], where V[sup eff cl](x[sub 0]) is the so-called effective classical potential containing the effects of all quantum fluctuations. The variable of integration is the temporal path average [formula]. We show how to generalize this concept to paths q[sup μ](τ) in curved space with metric g[sub μν](q), and calculate perturbatively the high-temperature expansion of V[sup eff cl](q[sub 0]). The requirement of independence under coordinate transformations q[sup μ](τ)→ q′[sup μ](τ) introduces subtleties in the definition and treatment of the path average [formula], and covariance is achieved only with the help of a suitable Faddeev–Popov procedure. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
0217751X
Volume :
18
Issue :
30
Database :
Complementary Index
Journal :
International Journal of Modern Physics A: Particles & Fields; Gravitation; Cosmology; Nuclear Physics
Publication Type :
Academic Journal
Accession number :
11727592
Full Text :
https://doi.org/10.1142/S0217751X03016471