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PERTURBATIVELY DEFINED EFFECTIVE CLASSICAL POTENTIAL IN CURVED SPACE.
- 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