Core-collapse supernova explosions hindered by eV-mass sterile neutrinos
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| Main Authors: | , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866908328012021760 |
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| author | Mori, Kanji Takiwaki, Tomoya Kohri, Kazunori Nagakura, Hiroki |
| author_facet | Mori, Kanji Takiwaki, Tomoya Kohri, Kazunori Nagakura, Hiroki |
| contents | Light sterile neutrinos, $ν_s$, are often introduced to explain an anomalous deficit in the electron antineutrino flux from nuclear reactors. If they exist, sterile neutrinos would also be produced in collapsing massive stars through the active-sterile neutrino oscillation. In order to investigate the impacts of sterile neutrinos on supernova dynamics, we perform two-dimensional neutrino-radiation hydrodynamic simulations of stellar core-collapse coupled with the active-sterile oscillation through the Mikheyev-Smirnov-Wolfenstein effect. As the initial condition of our simulations, we adopt a blue supergiant model that is tuned to reproduce observational features of the SN 1987A progenitor to compare our models with observations of the event. It is found that the active-sterile oscillation reduces the $ν_{e}$ and $\barν_e$ fluxes and decreases the explosion energy. We also find that, if the mixing angle $θ$ and the mass difference $δm_\mathrm{s}^2$ between $ν_e$ and $ν_s$ are large enough, the star fails to explode. This suggests that these mixing parameters relevant to sterile neutrinos could be constrained by supernova explodability, though other uncertainties in supernova theory need to be addressed to refine them. In addition, we predict neutrino signals from a nearby supernova event and find that the neutrino event number can significantly decrease because the $ν_e$ and $\barν_e$ fluxes are reduced. In particular, DUNE observations of $ν_e$ will be useful to search for a signature of sterile neutrinos with a tiny mixing angle because a smaller mixing angle leads to a larger effect on the $ν_e$ flux. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2503_14027 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Core-collapse supernova explosions hindered by eV-mass sterile neutrinos Mori, Kanji Takiwaki, Tomoya Kohri, Kazunori Nagakura, Hiroki High Energy Astrophysical Phenomena High Energy Physics - Phenomenology Light sterile neutrinos, $ν_s$, are often introduced to explain an anomalous deficit in the electron antineutrino flux from nuclear reactors. If they exist, sterile neutrinos would also be produced in collapsing massive stars through the active-sterile neutrino oscillation. In order to investigate the impacts of sterile neutrinos on supernova dynamics, we perform two-dimensional neutrino-radiation hydrodynamic simulations of stellar core-collapse coupled with the active-sterile oscillation through the Mikheyev-Smirnov-Wolfenstein effect. As the initial condition of our simulations, we adopt a blue supergiant model that is tuned to reproduce observational features of the SN 1987A progenitor to compare our models with observations of the event. It is found that the active-sterile oscillation reduces the $ν_{e}$ and $\barν_e$ fluxes and decreases the explosion energy. We also find that, if the mixing angle $θ$ and the mass difference $δm_\mathrm{s}^2$ between $ν_e$ and $ν_s$ are large enough, the star fails to explode. This suggests that these mixing parameters relevant to sterile neutrinos could be constrained by supernova explodability, though other uncertainties in supernova theory need to be addressed to refine them. In addition, we predict neutrino signals from a nearby supernova event and find that the neutrino event number can significantly decrease because the $ν_e$ and $\barν_e$ fluxes are reduced. In particular, DUNE observations of $ν_e$ will be useful to search for a signature of sterile neutrinos with a tiny mixing angle because a smaller mixing angle leads to a larger effect on the $ν_e$ flux. |
| title | Core-collapse supernova explosions hindered by eV-mass sterile neutrinos |
| topic | High Energy Astrophysical Phenomena High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2503.14027 |