Results 11 to 20 of about 155,831 (295)
Supernova neutrinos and nucleosynthesis [PDF]
Journal of Physics G: Nuclear and Particle Physics, 2013 Observations of metal-poor stars indicate that at least two different nucleosynthesis sites contribute to the production of r-process elements. One site is responsible for the production of light r-process elements Z ?
G. Martínez-Pinedo +2 more
semanticscholar +7 more sources
Decays of supernova neutrinos [PDF]
Nuclear Physics B, 2002 33 pages, 10 figures, Elsevier LaTeX.
Tommy Ohlsson +3 more
openaire +8 more sources
Discovery potential for supernova relic neutrinos with slow liquid scintillator detectors
Physics Letters B, 2017 Detection of supernova relic neutrinos could provide key support for our current understanding of stellar and cosmological evolution, and precise measurements of these neutrinos could yield novel insights into the universe.
Hanyu Wei, Zhe Wang, Shaomin Chen
doaj +4 more sources
Neutrino astronomy with supernova neutrinos [PDF]
Journal of Cosmology and Astroparticle Physics, 2018 Modern neutrino facilities will be able to detect a large number of neutrinos from the next Galactic supernova. We investigate the viability of the triangulation method to locate a core-collapse supernova by employing the neutrino arrival time ...
V. Brdar, M. Lindner, Xun-Jie Xu
semanticscholar +6 more sources
Geotomography with solar and supernova neutrinos [PDF]
Journal of High Energy Physics, 2005 35 pages, 7 figures; minor textual changes in section ...
Akhmedov, Evgeny Kh. +2 more
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Detection of Supernova Neutrinos [PDF]
, 2004 Matter effects on neutrino oscillations in both, a supernova and the Earth, change the observed supernova neutrino spectra. We calculate the expected number of supernova neutrino interactions for ICARUS, SK and SNO detectors as a function of the distance which they traveled in the Earth.
Bekman, B., Holeczek, Jacek, Kisiel, Jan
openaire +7 more sources
Acquiring information about neutrino parameters by detecting supernova neutrinos [PDF]
, 2010 We consider the supernova shock effects, the Mikheyev-Smirnov-Wolfenstein effects, the collective effects, and the Earth matter effects in the detection of type II supernova neutrinos on the Earth. It is found that the event number of supernova neutrinos
Ming-Yang Huang, Xin-Heng Guo, B. Young
semanticscholar +3 more sources
Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background [PDF]
Proceedings of 40th International Conference on High Energy physics — PoS(ICHEP2020), 2018 Sterile neutrinos with mass in the eV-scale and large mixings of order θ0≃ 0.1 could explain some anomalies found in short-baseline neutrino oscillation data.
Y. S. Jeong +3 more
semanticscholar +3 more sources
KamLAND SENSITIVITY TO NEUTRINOS FROM PRE-SUPERNOVA STARS [PDF]
, 2015 In the late stages of nuclear burning for massive stars (M > 8 M⊙), the production of neutrino–antineutrino pairs through various processes becomes the dominant stellar cooling mechanism.
K. Asakura +61 more
semanticscholar +3 more sources
Decoherence and oscillations of supernova neutrinos [PDF]
The European Physical Journal C, 2015 Supernova neutrinos have several exceptional features which can lead to interesting physical consequences. At the production point their wave packets have an extremely small size $$\sigma _{x} \sim 10^{-11}$$σx∼10-11 cm; hence the energy uncertainty can ...
J. Kersten, A. Smirnov
semanticscholar +7 more sources