Gravitational Wave Echo of Relaxion Trapping

Abhishek Banerjee, Eric Madge, Gilad Perez, Wolfram Ratzinger, Pedro Schwaller

Research output: Contribution to journalArticlepeer-review

13 Citations (Scopus)

Abstract

To solve the hierarchy problem, the relaxion must remain trapped in the correct minimum, even if the electroweak symmetry is restored after reheating. In this scenario, the relaxion starts rolling again until the backreaction potential, with its set of local minima, reappears. Depending on the time of barrier reappearance, Hubble friction alone may be insufficient to retrap the relaxion in a large portion of the parameter space. Thus, an additional source of friction is required, which might be provided by coupling to a dark photon. The dark photon experiences a tachyonic instability as the relaxion rolls, which slows down the relaxion by backreacting to its motion, and efficiently creates anisotropies in the dark photon energy-momentum tensor, sourcing gravitational waves. We calculate the spectrum of the resulting gravitational wave background from this new mechanism and evaluate its observability by current and future experiments. We further investigate the possibility that the coherently oscillating relaxion constitutes dark matter and present the corresponding constraints from gravitational waves.
Original languageEnglish
Article number055026
Number of pages17
JournalPhysical review. D
Volume104
Issue number5
DOIs
Publication statusPublished - 21 Sept 2021

Funding

Azrieli Foundation Minerva Foundation United States-Israel Binational Science Foundation National Science Foundation Friedrich Wilhelm Bessel research award German-Israeli Foundation for Scientific Research and Development Israel Science Foundation Yeda-Sela-SABRA-WRC Segre Research Award Deutsche Forschungsgemeinschaft We are grateful to Hyungjin Kim for collaboration at the early stages of this paper and participating in numerous vital discussions that seeded this work. We thank Edoardo Vitagliano for pointing out the updated fifth force bounds. The work of A. B. is supported by the Azrieli Foundation. The work of E. M. is supported by the Minerva Foundation. The work of G. P. is supported by grants from BSF-NSF, Friedrich Wilhelm Bessel research award, GIF, ISF, Minerva, Yeda-Sela-SABRA-WRC, and the Segre Research Award. The work of W. R. and P. S. is supported by the Deutsche Forschungsgemeinschaft (DFG), Project No. 438947057 and by the Cluster of Excellence “Precision Physics, Fundamental Interactions, and Structure of Matter” ( 2118/1) funded by the German Research Foundation (DFG) within the German Excellence Strategy (Project No. 39083149).

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