Gravitational waves in models with multicritical-point principle
arXiv:2202.04221 · doi:10.1140/epjc/s10052-022-10440-8
Abstract
The multicritical-point principle (MPP) provides a natural explanation of the large hierarchy between the Planck and electroweak scales. We consider a scenario in which MPP is applied to the Standard Model extended by two real singlet scalar fields and , and a dimensional transmutation occurs by the vacuum expectation value of . In this paper, we focus on the critical points that possess a symmetry and all the other fields are left invariant. Then becomes a natural dark matter (DM) candidate. Further, we concentrate on the critical points where does not possess further symmetry so that there is no cosmological domain-wall problem. Among such critical points, we focus on maximally critical one called CP-1234 that fix all the superrenormalizable parameters. We show that there remains a parameter region that satisfies the DM relic abundance, DM direct-detection bound and the current LHC constraints. In this region, we find a first-order phase transition in the early universe around the TeV-scale temperature. The resultant gravitational waves are predicted with a peak amplitude of at a frequency of - Hz, which can be tested with future space-based instruments such as DECIGO and BBO.
arXiv comment22 pages, 6 figures
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