All Publications
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Fireball antinucleosynthesis
PHYSICAL REVIEW D
2024; 109 (12)
View details for DOI 10.1103/PhysRevD.109.123028
View details for Web of Science ID 001288604300001
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Dark Solar Wind
PHYSICAL REVIEW LETTERS
2022; 129 (21): 211101
Abstract
We study the solar emission of light dark sector particles that self-interact strongly enough to self-thermalize. The resulting outflow behaves like a fluid which accelerates under its own thermal pressure to highly relativistic bulk velocities in the solar system. Compared to the ordinary noninteracting scenario, the local outflow has at least ∼10^{3} higher number density and correspondingly at least ∼10^{3} lower average energy per particle. We show how this generic phenomenon arises in a dark sector composed of millicharged particles strongly self-interacting via a dark photon. The millicharged plasma wind emerging in this model has novel yet predictive signatures that encourages new experimental directions. This phenomenon demonstrates how a small step away from the simplest models can lead to radically different outcomes and thus motivates a broader search for dark sector particles.
View details for DOI 10.1103/PhysRevLett.129.211101
View details for Web of Science ID 000886221300005
View details for PubMedID 36461962