Phase Transition to RS: Cool, not Supercool

Rashmish K. Mishra; Lisa Randall

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arXiv · 2401.09633

Phase Transition to RS: Cool, not Supercool

Rashmish K. Mishra·Lisa Randall

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Abstract

Motivated by the warped conifold compactification, we model the infrared (IR) dynamics of confining gauge theories in a Randall-Sundrum (RS)-like setup by modifying the stabilizing Goldberger-Wise (GW) potential so that it becomes large (in magnitude) in the IR and back-reacts on the geometry. We study the high-temperature phase by considering a black brane background in which we calculate the entropy and free energy of the strongly back-reacted solution. As with Buchel's result for the conifold (arXiv:2103.15188), we find a minimum temperature beyond which the black brane phase is thermodynamically unstable. In the context of a phase transition to the confining background, our results suggest that the amount of supercooling that the metastable black brane phase undergoes can be limited. It also suggests the first-order phase transition (and the associated gravitational waves from bubble collision) is not universal. Our results therefore have important phenomenological implications for early universe model building in these scenarios.

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Rashmish K. Mishra, Lisa Randall. 2024-01-17. Phase Transition to RS: Cool, not Supercool. https://arxiv.org/abs/2401.09633

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