Evaporating the Milky Way halo and its satellites with inelastic self-interacting dark matter

Self-interacting dark matter provides a promising alternative for the cold dark matter paradigm to solve potential small-scale galaxy formation problems. Nearly all self-interacting dark matter simulations so far have considered only elastic collisions. Here we present simulations of a galactic halo...

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Bibliographic Details
Main Authors: Vogelsberger, Mark (Author), Zavala, Jesús (Author), Schutz, Katelin (Author), Slatyer, Tracy Robyn (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), Massachusetts Institute of Technology. Center for Theoretical Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2020-10-06T22:42:05Z.
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