1. Stealth dark matter confinement transition and gravitational waves
- Author
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Oliver Witzel, Anna Hasenfratz, Xiao-Yong Jin, Andrew D. Gasbarro, Ethan T. Neil, Richard C. Brower, Pavlos Vranas, Enrico Rinaldi, David Schaich, James C. Osborn, G. T. Fleming, Kimmy K. Cushman, Claudio Rebbi, and Graham D. Kribs
- Subjects
Physics ,Particle physics ,010308 nuclear & particles physics ,Gravitational wave ,530 Physics ,High Energy Physics - Lattice (hep-lat) ,Dark matter ,FOS: Physical sciences ,Fermion ,Astrophysics::Cosmology and Extragalactic Astrophysics ,First order ,01 natural sciences ,Baryon ,High Energy Physics - Phenomenology ,High Energy Physics - Phenomenology (hep-ph) ,High Energy Physics - Lattice ,Lattice (order) ,0103 physical sciences ,Fundamental representation ,010306 general physics ,Phenomenology (particle physics) - 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., Data release at doi.org/10.5281/zenodo.3921870
- Published
- 2021