Non-Scaling Topological Defects and Gravitational Waves in Higgs Portal
Wen Yin

TL;DR
This paper demonstrates that in Higgs portal models, topological defects like domain walls and cosmic strings can form in the early Universe due to non-adiabatic Higgs oscillations, leading to significant gravitational waves and potential cosmological phenomena.
Contribution
It introduces lattice simulations showing defect formation without symmetry restoration and explores their gravitational wave signatures and cosmological implications.
Findings
Topological defects form even without symmetry restoration due to early Universe dynamics.
Gravitational waves from these defects can be significant and detectable.
Defects may induce miniclusters and primordial black holes.
Abstract
One of the simplest extensions of the Standard Model is the Higgs portal extension involving a dark Higgs. Dark sectors that include dark matter candidates, WIMPs, axions, and dark photons, can naturally have this type of interaction, where the dark Higgs is charged under some symmetry, which may or may not be spontaneous broken by the vacuum expectation value. In this paper, using lattice simulations, I show that if the reheating temperature of the Universe is sufficiently high, topological defects such as domain walls and cosmic strings associated with these symmetries are naturally formed even if the symmetries are never restored due to negative thermal mass squareds. This occurs due to the early Universe's non-adiabatic oscillation of the Higgs around the onset of oscillation, which overshoots the origin, and tachyonic instability that enhances fluctuations. The gravitational waves…
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Taxonomy
TopicsGeophysics and Sensor Technology · Cosmology and Gravitation Theories
