Results 91 to 100 of about 372 (179)

Diffuse neutrino background from past core collapse supernovae. [PDF]

open access: yesProc Jpn Acad Ser B Phys Biol Sci, 2023
Ando S, Ekanger N, Horiuchi S, Koshio Y.
europepmc   +1 more source

87th Annual Meeting of the Meteoritical Society 2025: Abstracts

open access: yes
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley   +1 more source

Performance of SK-Gd’s Upgraded Real-time Supernova Monitoring System

open access: yesThe Astrophysical Journal
Among multimessenger observations of the next Galactic core-collapse supernova, Super-Kamiokande (SK) plays a critical role in detecting the emitted supernova neutrinos, determining the direction to the supernova (SN), and notifying the astronomical ...
Y. Kashiwagi   +239 more
doaj   +1 more source

A Core-collapse Supernova Neutrino Parameterization with Enhanced Physical Interpretability

open access: yesThe Astrophysical Journal Supplement Series
We introduce a novel parameterization of supernova neutrino energy spectra with a clear physical motivation. Its central parameter, τ ( t ), quantifies the characteristic thermal-diffusion area during the explosion.
Haihao Shi   +4 more
doaj   +1 more source

Supernova neutrinos

open access: yes
Plenary talk at the Neutrino 2024 conference. Session 10: Neutrino cosmology.
openaire   +2 more sources

Supernova Neutrinos and the Neutrino Masses

open access: yes, 1999
Core-collapse supernovae emit of order $10^{58}$ neutrinos and antineutrinos of all flavors over several seconds, with average energies of 10--25 MeV. In the Sudbury Neutrino Observatory (SNO), a future Galactic supernova at a distance of 10 kpc would cause several hundred events.
openaire   +2 more sources

86th Annual Meeting of the Meteoritical Society (2024)

open access: yes
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley   +1 more source

A Theory for Neutron Star and Black Hole Kicks and Induced Spins

open access: yesThe Astrophysical Journal
Using 20 long-term 3D core-collapse supernova simulations, we find that lower compactness progenitors that explode quasi-spherically due to the short delay to explosion experience smaller neutron star recoil kicks in the ∼100−200 km s ^−1 range, while ...
Adam Burrows   +3 more
doaj   +1 more source

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