Probing the baryogenesis and dark matter relaxed in phase transition by gravitational waves and colliders

Abstract

The cosmological phase transition with Q-balls production mechanism can explain the baryogenesis and dark matter simultaneously, where constraints on dark matter masses and reverse dilution are significantly relaxed. We study how to probe this scenario by collider signals at QCD next-to-leading order and gravitational wave signals.

arXiv comment22 pages,9 figures,4 tables, published in Phys.Rev.D

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Cited by in corpus (50)

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• On the Maximal Strength of a First-Order Electroweak Phase Transition and its Gravitational Wave Signal
• Gravitational wave energy budget in strongly supercooled phase transitions
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• Fermi-ball dark matter from a first-order phase transition
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• Phase transition dynamics and gravitational wave spectra of strong first-order phase transition in supercooled universe
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• Gravitational wave and collider probes of a triplet Higgs sector with a low cutoff
• Electroweak phase transition with composite Higgs models: calculability, gravitational waves and collider searches
• Exploring dynamical CP violation induced baryogenesis by gravitational waves and colliders
• Gravitational waves from scale-invariant vector dark matter model: Probing below the neutrino-floor
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• First-order phase transition and fate of false vacuum remnants
• Gravitation waves from QCD and electroweak phase transitions
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• Dark Matter and Gravity Waves from a Dark Big Bang
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• Filtered pseudo-scalar dark matter and gravitational waves from first order phase transition
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• Testing clockwork axion with gravitational waves
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• Detailed Calculation of Primordial Black Hole Formation During First-Order Cosmological Phase Transitions
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