Dark matter from Monogem
Christopher V. Cappiello, Neal P. Avis Kozar, Aaron C. Vincent
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As a supernova shock expands into space, it may collide with dark matter particles, scattering them up to velocities more than an order of magnitude larger than typical dark matter velocities in the Milky Way. If a supernova remnant is close enough to Earth, and the appropriate age, this flux of high-velocity dark matter could be detectable in direct detection experiments, particularly if the dark matter interacts vi ...
a a velocity-dependent operator. This could make it easier to detect light dark matter that would otherwise have too little energy to be detected. We show that the Monogem Ring supernova remnant is both close enough and the correct age to produce such a flux, and thus we produce novel direct detection constraints and sensitivities for future experiments.
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As a supernova shock expands into space, it may collide with dark matter particles, scattering them up to velocities more than an order of magnitude larger than typical dark matter velocities in the Milky Way.
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Evidence disclosure
Evidence graph: 2 refs, 1 links.
Utility signals: depth 65/100, grounding 58/100, status medium.
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Research context
16
Citations
109
References
Tasks
Dark matter, Supernova, Flux (metallurgy), Light dark matter, Milky Way, Supernova remnant, Scalar field dark matter, Dark energy
Methods
None detected
Domains
Physics, Astrophysics, Physics and Astronomy, Nuclear and High Energy Physics
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