Self-Interacting Dark Matter Subhalos in the Milky Way’s Tides
© 2020 American Physical Society. We study evolution of self-interacting dark matter subhalos in the Milky Way tidal field. The interaction between the subhalos and the Milky Way's tides lead to more diverse dark matter distributions in the inner region, compared to their cold dark matter count...
| Main Authors: | , , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
American Physical Society (APS)
2021
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| Online Access: | https://hdl.handle.net/1721.1/135939 |
| _version_ | 1811079736272617472 |
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| author | Sameie, Omid Yu, Hai-Bo Sales, Laura V Vogelsberger, Mark Zavala, Jesús |
| author2 | Massachusetts Institute of Technology. Department of Physics |
| author_facet | Massachusetts Institute of Technology. Department of Physics Sameie, Omid Yu, Hai-Bo Sales, Laura V Vogelsberger, Mark Zavala, Jesús |
| author_sort | Sameie, Omid |
| collection | MIT |
| description | © 2020 American Physical Society. We study evolution of self-interacting dark matter subhalos in the Milky Way tidal field. The interaction between the subhalos and the Milky Way's tides lead to more diverse dark matter distributions in the inner region, compared to their cold dark matter counterparts. We test this scenario with two Milky Way satellite galaxies, Draco and Fornax, opposite extremes in the inner dark matter content, and find that they can be accommodated within the self-interacting dark matter model proposed to explain the diverse rotation curves of spiral galaxies in the field. |
| first_indexed | 2024-09-23T11:19:44Z |
| format | Article |
| id | mit-1721.1/135939 |
| institution | Massachusetts Institute of Technology |
| language | English |
| last_indexed | 2024-09-23T11:19:44Z |
| publishDate | 2021 |
| publisher | American Physical Society (APS) |
| record_format | dspace |
| spelling | mit-1721.1/1359392023-02-17T19:40:46Z Self-Interacting Dark Matter Subhalos in the Milky Way’s Tides Sameie, Omid Yu, Hai-Bo Sales, Laura V Vogelsberger, Mark Zavala, Jesús Massachusetts Institute of Technology. Department of Physics MIT Kavli Institute for Astrophysics and Space Research © 2020 American Physical Society. We study evolution of self-interacting dark matter subhalos in the Milky Way tidal field. The interaction between the subhalos and the Milky Way's tides lead to more diverse dark matter distributions in the inner region, compared to their cold dark matter counterparts. We test this scenario with two Milky Way satellite galaxies, Draco and Fornax, opposite extremes in the inner dark matter content, and find that they can be accommodated within the self-interacting dark matter model proposed to explain the diverse rotation curves of spiral galaxies in the field. 2021-10-27T20:30:02Z 2021-10-27T20:30:02Z 2020 2021-07-09T15:39:22Z Article http://purl.org/eprint/type/JournalArticle https://hdl.handle.net/1721.1/135939 en 10.1103/PHYSREVLETT.124.141102 Physical Review Letters Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Physical Society (APS) APS |
| spellingShingle | Sameie, Omid Yu, Hai-Bo Sales, Laura V Vogelsberger, Mark Zavala, Jesús Self-Interacting Dark Matter Subhalos in the Milky Way’s Tides |
| title | Self-Interacting Dark Matter Subhalos in the Milky Way’s Tides |
| title_full | Self-Interacting Dark Matter Subhalos in the Milky Way’s Tides |
| title_fullStr | Self-Interacting Dark Matter Subhalos in the Milky Way’s Tides |
| title_full_unstemmed | Self-Interacting Dark Matter Subhalos in the Milky Way’s Tides |
| title_short | Self-Interacting Dark Matter Subhalos in the Milky Way’s Tides |
| title_sort | self interacting dark matter subhalos in the milky way s tides |
| url | https://hdl.handle.net/1721.1/135939 |
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