Dark cosmic rays
If dark matter particles have an electric charge, as in models of millicharged dark matter, such particles should be accelerated in the same astrophysical accelerators that produce ordinary cosmic rays, and their spectra should have a predictable rigidity dependence. Depending on the charge, the res...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
Elsevier
2017-05-01
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| Series: | Physics Letters B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269317301387 |
| _version_ | 1818032599887511552 |
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| author | Ping-Kai Hu Alexander Kusenko Volodymyr Takhistov |
| author_facet | Ping-Kai Hu Alexander Kusenko Volodymyr Takhistov |
| author_sort | Ping-Kai Hu |
| collection | DOAJ |
| description | If dark matter particles have an electric charge, as in models of millicharged dark matter, such particles should be accelerated in the same astrophysical accelerators that produce ordinary cosmic rays, and their spectra should have a predictable rigidity dependence. Depending on the charge, the resulting “dark cosmic rays” can be detected as muon-like or neutrino-like events in Super-Kamiokande, IceCube, and other detectors. We present new limits and propose several new analyses, in particular, for the Super-Kamiokande experiment, which can probe a previously unexplored portion of the millicharged dark matter parameter space. Most of our results are fairly general and apply to a broad class of dark matter models. |
| first_indexed | 2024-12-10T06:09:56Z |
| format | Article |
| id | doaj.art-6774502e8386446fbace0ca3b5498f2b |
| institution | Directory Open Access Journal |
| issn | 0370-2693 1873-2445 |
| language | English |
| last_indexed | 2024-12-10T06:09:56Z |
| publishDate | 2017-05-01 |
| publisher | Elsevier |
| record_format | Article |
| series | Physics Letters B |
| spelling | doaj.art-6774502e8386446fbace0ca3b5498f2b2022-12-22T01:59:36ZengElsevierPhysics Letters B0370-26931873-24452017-05-01768C182210.1016/j.physletb.2017.02.035Dark cosmic raysPing-Kai Hu0Alexander Kusenko1Volodymyr Takhistov2Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA 90095-1547, USADepartment of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA 90095-1547, USADepartment of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA 90095-1547, USAIf dark matter particles have an electric charge, as in models of millicharged dark matter, such particles should be accelerated in the same astrophysical accelerators that produce ordinary cosmic rays, and their spectra should have a predictable rigidity dependence. Depending on the charge, the resulting “dark cosmic rays” can be detected as muon-like or neutrino-like events in Super-Kamiokande, IceCube, and other detectors. We present new limits and propose several new analyses, in particular, for the Super-Kamiokande experiment, which can probe a previously unexplored portion of the millicharged dark matter parameter space. Most of our results are fairly general and apply to a broad class of dark matter models.http://www.sciencedirect.com/science/article/pii/S0370269317301387 |
| spellingShingle | Ping-Kai Hu Alexander Kusenko Volodymyr Takhistov Dark cosmic rays Physics Letters B |
| title | Dark cosmic rays |
| title_full | Dark cosmic rays |
| title_fullStr | Dark cosmic rays |
| title_full_unstemmed | Dark cosmic rays |
| title_short | Dark cosmic rays |
| title_sort | dark cosmic rays |
| url | http://www.sciencedirect.com/science/article/pii/S0370269317301387 |
| work_keys_str_mv | AT pingkaihu darkcosmicrays AT alexanderkusenko darkcosmicrays AT volodymyrtakhistov darkcosmicrays |