Results 71 to 80 of about 155,831 (295)
Estimating the core compactness of massive stars with Galactic supernova neutrinos [PDF]
, 2017 We suggest the future detection of neutrinos from a Galactic core-collapse supernova can be used to infer the progenitor's inner mass density structure.
S. Horiuchi +3 more
semanticscholar +1 more source
Measuring the neutron star compactness and binding energy with supernova neutrinos [PDF]
, 2017 We investigate the precision with which a neutron star gravitational binding energy can be measured through the supernova neutrino signal, without assuming any prior such as the energy equipartition hypothesis, mean energies hierarchy or constraints on ...
A. G. Rosso, F. Vissani, M. Volpe
semanticscholar +1 more source
Roles of Fast Neutrino-Flavor Conversion on the Neutrino-Heating Mechanism of Core-Collapse Supernova. [PDF]
Physical Review Letters, 2023 One of the greatest uncertainties in any modeling of the inner engine of core-collapse supernova (CCSN) is neutrino-flavor conversions driven by neutrino self-interactions.
H. Nagakura
semanticscholar +1 more source
Supernova neutrinos and the ντ mass [PDF]
Astroparticle Physics, 1997 25 pages - 1 LaTeX file and 14 (E)PS figures in a tarred, gzipped, uuencoded file - figures included via EPSFIG commands - submitted to Astroparticle ...
Camillo Acerbi +2 more
openaire +3 more sources
Advances in Astronomy, 2012 Core-collapse supernovae are dramatic explosions marking the catastrophic end of massive stars. The only means to get direct information about the supernova engine is from observations of neutrinos emitted by the forming neutron star, and through ...
Kei Kotake +6 more
doaj +1 more source
SciPost Physics Proceedings, 2023 The upcoming Hyper-Kamiokande (HyperK) experiment is expected to detect the Diffuse Supernova Neutrino Background (DSNB). This requires to ponder all possible sources of background.
Sandra Robles
doaj +1 more source
Nucleosynthesis in neutrino-driven supernovae [PDF]
New Astronomy Reviews, 2006 Core collapse supernovae are the leading actor in the story of the cosmic origin of the chemical elements. Existing models, which generally assume spherical symmetry and parameterize the explosion, have been able to broadly replicate the observed elemental pattern.
Froehlich, C +7 more
openaire +5 more sources
Neutrino Probes of Galactic and Extragalactic Supernovae [PDF]
, 2007 Neutrinos are a messenger of extreme condition inside a supernova core and a new-born neutron star. Since current ground-based detectors have potential to detect ~10,000 neutrinos from supernova at the galactic center, they could tell us lots of ...
Ando, Shin'ichiro
core +1 more source
Neutrino Physics and Astrophysics with the JUNO Detector
Universe, 2018 The Jiangmen Underground Neutrino Observatory (JUNO) is a 20 kton liquid scintillator multi-purpose underground detector, under construction near the Chinese city of Jiangmen, with data collection expected to start in 2021.
Lino Miramonti
doaj +1 more source
Examining Neutrino–Matter Interactions in the Cassiopeia A Supernova
The Astrophysical Journal, 2023 Neutrino interactions with stellar material are widely believed to be fundamental to the explosion of massive stars. However, this important process has remained difficult to confirm observationally.
Toshiki Sato +6 more
doaj +1 more source