Stealth dark matter confinement transition and gravitational waves



Brower, RC, Cushman, K, Fleming, GT, Gasbarro, A, Hasenfratz, A, Jin, XY, Kribs, GD, Neil, ET, Osborn, JC, Rebbi, C
et al (show 4 more authors) (2021) Stealth dark matter confinement transition and gravitational waves. Physical Review D, 103. 014505-014505.

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Abstract

We use non-perturbative lattice calculations to investigate the finite-temperature confinement transition of stealth dark matter, focusing on the regime in which this early-universe transition is first order and would generate a stochastic background of gravitational waves. Stealth dark matter extends the standard model with a new strongly coupled SU(4) gauge sector with four massive fermions in the fundamental representation, producing a stable spin-0 'dark baryon' as a viable composite dark matter candidate. Future searches for stochastic gravitational waves will provide a new way to discover or constrain stealth dark matter, in addition to previously investigated direct-detection and collider experiments. As a first step to enabling this phenomenology, we determine how heavy the dark fermions need to be in order to produce a first-order stealth dark matter confinement transition.

Item Type: Article
Additional Information: Data release at doi.org/10.5281/zenodo.3921870
Uncontrolled Keywords: hep-lat, hep-ph
Depositing User: Symplectic Admin
Date Deposited: 02 Jul 2020 09:43
Last Modified: 21 May 2023 22:39
DOI: 10.1103/PhysRevD.103.014505
Related URLs:
URI: https://livrepository.liverpool.ac.uk/id/eprint/3092510

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