Gauge-independent effective potential for minimally coupled quantum fields in curved space

1992 ◽  
Vol 46 (10) ◽  
pp. 4413-4420 ◽  
Author(s):  
J. Balakrishnan ◽  
D. J. Toms
1994 ◽  
Vol 49 (10) ◽  
pp. 5257-5265 ◽  
Author(s):  
David Hochberg ◽  
Thomas W. Kephart ◽  
James W. York

2013 ◽  
Vol 28 (12) ◽  
pp. 1350042 ◽  
Author(s):  
XAVIER CALMET ◽  
TING-CHENG YANG

We show how to map gravitational theories formulated in the Jordan frame to the Einstein frame at the quantum field theoretical level considering quantum fields in curved space–time. As an example, we consider gravitational theories in the Jordan frame of the type F(ϕ, R) = f(ϕ)R-V(ϕ) and perform the map to the Einstein frame. Our results can easily be extended to any gravitational theory. We consider the Higgs inflation model as an application of our results.


1988 ◽  
Vol 303 (4) ◽  
pp. 728-750 ◽  
Author(s):  
Ikuo Shirai ◽  
Sumio Wada

Author(s):  
N. D. Birrell ◽  
P. C. W. Davies
Keyword(s):  

Author(s):  
Iosif L. Buchbinder ◽  
Ilya L. Shapiro

As the main purpose of renormalization is not to remove divergences but to get essential information about the finite part of effective action, this chapter discusses some of the existing methods of solving this problem; such methods can be denoted the renormalization group. First, the minimal subtraction renormalization group in curved space is formulated. Next, the chapter shows how the overall μ‎-independence of the effective action enables one to interpret μ‎-dependence in some situations. As an example, the effective potential is restored from the renormalization group and compared with the expression calculated directly in chapter 13. In addition, the global conformal (scaling) anomaly is derived from the renormalization group.


1996 ◽  
Vol 74 (9-10) ◽  
pp. 626-633
Author(s):  
Anjana Sinha ◽  
Rajkumar Roychoudhury

The effective potential for the sine-Gordon model in a curved space-time, given by [Formula: see text], has been calculated using the Schrödinger picture formalism. It has been shown that when α(x) → 1 our method reproduces the flat-space results. To show the effect of the curvature term, the effective potential Veff has been calculated numerically for several values of the parameter M, where α(x) has been taken to be of the form [Formula: see text].


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