Detecting neutrino-boosted axion dark matter in the MeV gap
Abstract The elusive nature of Dark Matter (DM) remains a mystery far from being solved. A vast effort is dedicated to search for signatures of feeble DM interactions with Standard Model particles. In this work, we explore the signatures of axion DM boosted by interactions with Supernova neutrinos:...
Asıl Yazarlar: | , |
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Materyal Türü: | Makale |
Dil: | English |
Baskı/Yayın Bilgisi: |
SpringerOpen
2023-02-01
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Seri Bilgileri: | European Physical Journal C: Particles and Fields |
Online Erişim: | https://doi.org/10.1140/epjc/s10052-023-11248-w |
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author | Pierluca Carenza Pedro De la Torre Luque |
author_facet | Pierluca Carenza Pedro De la Torre Luque |
author_sort | Pierluca Carenza |
collection | DOAJ |
description | Abstract The elusive nature of Dark Matter (DM) remains a mystery far from being solved. A vast effort is dedicated to search for signatures of feeble DM interactions with Standard Model particles. In this work, we explore the signatures of axion DM boosted by interactions with Supernova neutrinos: Neutrino-Boosted Axion DM ( $$\nu $$ ν BADM). We focus on $$\nu $$ ν BADM converting into photons in the Galactic magnetic field, generating a peculiar gamma-ray flux. This signal falls in the poorly explored MeV energy range, that will be probed by next generation gamma-ray missions. Once more, astrophysical searches might act as a probe of fundamental physics, unveiling the nature and properties of DM. |
first_indexed | 2024-04-09T19:53:09Z |
format | Article |
id | doaj.art-7dfbc3bb4de143febf6cdacdd1e06c81 |
institution | Directory Open Access Journal |
issn | 1434-6052 |
language | English |
last_indexed | 2024-04-09T19:53:09Z |
publishDate | 2023-02-01 |
publisher | SpringerOpen |
record_format | Article |
series | European Physical Journal C: Particles and Fields |
spelling | doaj.art-7dfbc3bb4de143febf6cdacdd1e06c812023-04-03T05:37:22ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522023-02-0183211010.1140/epjc/s10052-023-11248-wDetecting neutrino-boosted axion dark matter in the MeV gapPierluca Carenza0Pedro De la Torre Luque1The Oskar Klein Centre, Department of Physics, Stockholm UniversityThe Oskar Klein Centre, Department of Physics, Stockholm UniversityAbstract The elusive nature of Dark Matter (DM) remains a mystery far from being solved. A vast effort is dedicated to search for signatures of feeble DM interactions with Standard Model particles. In this work, we explore the signatures of axion DM boosted by interactions with Supernova neutrinos: Neutrino-Boosted Axion DM ( $$\nu $$ ν BADM). We focus on $$\nu $$ ν BADM converting into photons in the Galactic magnetic field, generating a peculiar gamma-ray flux. This signal falls in the poorly explored MeV energy range, that will be probed by next generation gamma-ray missions. Once more, astrophysical searches might act as a probe of fundamental physics, unveiling the nature and properties of DM.https://doi.org/10.1140/epjc/s10052-023-11248-w |
spellingShingle | Pierluca Carenza Pedro De la Torre Luque Detecting neutrino-boosted axion dark matter in the MeV gap European Physical Journal C: Particles and Fields |
title | Detecting neutrino-boosted axion dark matter in the MeV gap |
title_full | Detecting neutrino-boosted axion dark matter in the MeV gap |
title_fullStr | Detecting neutrino-boosted axion dark matter in the MeV gap |
title_full_unstemmed | Detecting neutrino-boosted axion dark matter in the MeV gap |
title_short | Detecting neutrino-boosted axion dark matter in the MeV gap |
title_sort | detecting neutrino boosted axion dark matter in the mev gap |
url | https://doi.org/10.1140/epjc/s10052-023-11248-w |
work_keys_str_mv | AT pierlucacarenza detectingneutrinoboostedaxiondarkmatterinthemevgap AT pedrodelatorreluque detectingneutrinoboostedaxiondarkmatterinthemevgap |