IMPROVED EFFECTIVE POTENTIAL IN CURVED SPACETIME AND QUANTUM MATTER HIGHER-DERIVATIVE GRAVITY THEORY

被引:37
作者
ELIZALDE, E
ODINTSOV, SD
ROMEO, A
机构
[1] UNIV BARCELONA, FAC PHYS, DEPT ESTRUCTURA & CONSTITUENTS MAT, E-08028 BARCELONA, SPAIN
[2] UNIV BARCELONA, FAC PHYS, INST FIS ALTES ENERGIES, E-08028 BARCELONA, SPAIN
关键词
D O I
10.1103/PhysRevD.51.1680
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We develop a general formalism to study the renormalization-group- (RG-)improved effective potential for renormalizable gauge theories, including matter-R2-gravity, in curved spacetime. The result is given up to quadratic terms in curvature, and one-loop effective potentials may be easily obtained from it. As an example, we consider scalar QED, where dimensional transmutation in curved space and the phase structure of the potential (in particular, curvature-induced phase transitions) are discussed. For scalar QED with higher-derivative quantum gravity (QG), we examine the influence of QG on dimensional transmutation and calculate QG corrections to the scalar-to-vector mass ratio. The phase structure of the RG-improved effective potential is also studied in this case, and the values of the induced Newton and cosmological coupling constants at the critical point are estimated. The stability of the running scalar coupling in the Yukawa theory with conformally invariant higher-derivative QG, and in the standard model with the same addition, is numerically analyzed. We show that, in these models, QG tends to make the scalar sector less unstable. © 1995 The American Physical Society.
引用
收藏
页码:1680 / 1691
页数:12
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