Renormalization-Group Improved Effective Potential for Finite Grand Unified Theories in Curved Spacetime
E. Elizalde, S.D. Odintsov

TL;DR
This paper constructs a renormalization-group improved effective potential for finite theories in curved spacetime, revealing an exponential-like structure and exploring implications for cosmology such as curvature-induced phase transitions.
Contribution
It introduces a novel effective potential in curved spacetime for finite theories, highlighting its unique exponential form and potential cosmological applications.
Findings
Effective potential has exponential-like structure in curved spacetime.
Potential for curvature-induced phase transitions.
Implications for gravitational and cosmological constants.
Abstract
The renormalization-group improved effective potential ---to leading-log and in the linear curvature approximation--- is constructed for ``finite'' theories in curved spacetime. It is not trivial and displays a quite interesting, exponential-like structure ---in contrast with the case of flat spacetime where it coincides with the classical potential. Several possible cosmological applications, as curvature-induced phase transitions and modifications of the values of the gravitational and cosmological constants, are briefly discussed.
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