arXiv · 2006.16429
Stealth dark matter confinement transition and gravitational waves
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.
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R. C. Brower, K. Cushman, G. T. Fleming, A. Gasbarro, A. Hasenfratz, X. Y. Jin, G. D. Kribs, E. T. Neil, J. C. Osborn, C. Rebbi, E. Rinaldi, D. Schaich, P. Vranas, O. Witzel. 2020-06-29. Stealth dark matter confinement transition and gravitational waves. https://doi.org/10.1103/physrevd.103.014505
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