arXiv · 0806.1651
Instabilities in Thermal Gravity with a Cosmological Constant
Abstract
It is shown that in quantum gravity at finite temperature, the effective potential evaluated in the tadpole approximation can have a local minimum below a certain critical temperature. However, when the leading higher order thermal loop corrections are included, one finds that no static solution exists at high temperature.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
F. T. Brandt, J. Frenkel. 2008-06-10. Instabilities in Thermal Gravity with a Cosmological Constant. https://doi.org/10.1016/j.physletb.2008.06.009
Cite the original work for its findings. Save a collection to share your selection of sources.