Results 41 to 50 of about 189,045 (244)
Connecting neutrino physics with dark matter
New Journal of Physics, 2014 The origin of neutrino masses and the nature of dark matter are two in most pressing open questions in modern astro-particle physics. We consider here the possibility that these two problems are related, and review some theoretical scenarios which offer ...
Massimiliano Lattanzi +2 more
doaj +1 more source
Neutrino nucleosynthesis [PDF]
Physics Letters B, 2005 We study neutrino process nucleosynthesis in massive stars using newly calculated cross sections, an expanded reaction network, and complete and self-consistent models of the progenitor star. We reevaluate the production of light isotopes from abundant progenitors as well as that of rare, heavy, proton-rich isotopes.
Heger, A. +5 more
openaire +3 more sources
Frontiers in Physics, 2021 Analyses of neutrino measurements acquired by the Super-Kamiokande Neutrino Observatory (SK, in operation 1996–2001) and radon decay measurements acquired by the Geological Survey of Israel (GSI, in operation 2007–2017) yield strikingly similar ...
P. A. Sturrock +2 more
doaj +1 more source
Pseudo-Dirac neutrino scenario: Cosmic neutrinos at neutrino telescopes [PDF]
Physical Review D, 2010 24 pages, 5 ...
openaire +2 more sources
Sensors, 2021 The neutrinos of cosmic radiation, due to interaction with any known medium in which the Cherenkov detector is used, produce energy radiation phenomena in the form of a Cherenkov cone, in very large frequency spectrum. These neutrinos carry with them the
Valeriu Savu +2 more
doaj +1 more source
AIP Conference Proceedings, 2007 6 pages, 5 figures. This paper is an expanded version of a paper of the same name to appear the Proceedings of TAUP 2015 in the Journal of Physics Conference ...
Thomas K. Gaisser, Jeffrey R. Wilkes
openaire +4 more sources
Physics Letters BThe formation of the third r-process abundance peak near A ∼ 195 is highly sensitive to both nuclear structure far from stability and the astrophysical conditions that produce the heaviest elements.
Mengke Li +2 more
doaj +1 more source
Ghost particles in the universe: Neutrinos in astrophysics and cosmology
Mètode Science Studies Journal: Annual Review, 2017 Neutrinos are nearly massless and very difficult to detect because they interact so very weakly. Sixty years after seeing the first of these «ghost particles» we know a lot about their properties.
Georg Gottfried Raffelt
doaj +1 more source
Incorporating a Radiative Hydrodynamics Scheme in the Numerical-Relativity Code BAM
Universe, 2022 To study binary neutron star systems and to interpret observational data such as gravitational-wave and kilonova signals, one needs an accurate description of the processes that take place during the final stages of the coalescence, for example, through ...
Henrique Gieg +3 more
doaj +1 more source
Demystifying the PeV Cascades in IceCube: Less (Energy) is More (Events)
, 2013 The IceCube neutrino observatory has detected two cascade events with energies near 1 PeV. Without invoking new physics, we analyze the source of these neutrinos. We show that atmospheric conventional neutrinos and cosmogenic neutrinos (those produced in
Beacom, John F. +4 more
core +1 more source