Diffuse Supernova Neutrinos with Secret Neutrino Interactions
hep-ph, astro-ph.HE
Submitted: 2026-06-22
Updated: 2026-10-01
Comments: 28 pages, 9 figures, Comments are welcome
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Diffuse supernova neutrinos at underground laboratories
- The Diffuse Supernova Neutrino Background
- Diffuse neutrino background from past core-collapse supernovae
- Diffuse Supernova Neutrino Background Search at Super-Kamiokande
- Supernova Relic Neutrino Search at Super-Kamiokande
- Imprint of Explosion Mechanism on Supernova Relic Neutrinos
- Supernova Neutrinos: Production, Oscillations and Detection
- What can be learned from a future supernova neutrino detection?
- Measuring the supernova unknowns at the next-generation neutrino telescopes through the diffuse neutrino background
- Constraining properties of the next nearby core-collapse supernova with multi-messenger signals
- Core-Collapse Supernova Explosion Theory
- Towards Probing the Diffuse Supernova Neutrino Background in All Flavors
- Effect of Collective Flavor Oscillations on the Diffuse Supernova Neutrino Background
- Diffuse supernova neutrinos: oscillation effects, stellar cooling and progenitor mass dependence
- Fundamental physics with the diffuse supernova background neutrinos
- The diffuse supernova neutrino background as a probe of late-time neutrino mass generation
- Search for Diffuse Supernova Neutrino Background with 956.2 days of Super-Kamiokande Gadolinium Dataset
- The Sun and core-collapse supernovae are leading probes of the neutrino lifetime
- Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background
- Constraining sterile neutrinos by core-collapse supernovae with multiple detectors
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