Results 1 to 10 of about 146,178 (259)

Sensitivity of the PICO-500 bubble chamber to supernova neutrinos through coherent nuclear elastic scattering [PDF]

Astroparticle physics, 2018
Ton-scale direct dark matter search experiments should be sensitive to neutrino-induced recoil events from either 8B solar neutrinos or the brief but intense flux from a core collapse supernova in the Milky Way.
Tetiana Kozynets, S. Fallows, C. Krauss
semanticscholar   +1 more source

Fast flavor conversions of supernova neutrinos: Classifying instabilities via dispersion relations [PDF]

, 2017
Supernova neutrinos can exhibit a rich variety of flavor conversion mechanisms. In particular, they can experience "fast" self-induced flavor conversions almost immediately above the core.
F. Capozzi, B. Dasgupta, E. Lisi, A. Marrone, U. AlessandroMirizziOhioState, Tifr, U. INFNBari   +6 more
semanticscholar   +1 more source

Fundamental physics with the diffuse supernova background neutrinos [PDF]

Physical Review D, 2020
The Universe is awash with tens-of-MeV neutrinos of all species coming from all past core-collapse supernovae. These have never been observed, but this state of affairs will change in the near future.
A. de Gouvêa, I. Martínez-Soler, Y. Perez-Gonzalez, M. Sen   +3 more
semanticscholar   +1 more source

Theory and phenomenology of supernova neutrinos

AIP Conference Proceedings, 2015
Cecilia Lunardini
exaly   +2 more sources

Fast Pairwise Conversion of Supernova Neutrinos: A Dispersion Relation Approach. [PDF]

Physical Review Letters, 2016
Collective pair conversion ν_{e}ν[over ¯]_{e}↔ν_{x}ν[over ¯]_{x} by forward scattering, where x=μ or τ, may be generic for supernova neutrino transport.
I. Izaguirre, G. Raffelt, I. Tamborra
semanticscholar   +1 more source

Lifting the core-collapse supernova bounds on keV-mass sterile neutrinos [PDF]

Journal of Cosmology and Astroparticle Physics, 2020
We explore the energy and entropy transport as well as the lepton number variation induced from the mixing between electron and sterile neutrinos with keV mass in the supernova core.
A. M. Suliga, I. Tamborra, Meng-Ru Wu
semanticscholar   +1 more source

Supernova neutrino detection [PDF]

AIP Conference Proceedings, 2001
A core-collapse supernova will produce an enormous burst of neutrinos of all flavors in the few-tens-of-MeV range. Measurement of the flavor, time, and energy structure of a nearby core-collapse neutrino burst will yield answers to many physics and astrophysics questions.
openaire   +7 more sources

Neutrinos and nucleosynthesis in supernova

Journal of Physics: Conference Series, 2006
The type II supernova is considered as a candidate site for the production of heavy elements. The nucleosynthesis occurs in an intense neutrino flux, we calculate the electron fraction in this environment.
Solis, U., D'Olivo, J. C., Cabral-Rosetti, L. G.   +2 more
openaire   +2 more sources

Heavy sterile neutrinos and supernova explosions [PDF]

, 2008
We consider sterile neutrinos with rest masses ∼0.2 GeV and with vacuum flavor mixing angles θ2>10−8 for mixing with τ-neutrinos, or 10 ...
Petraki, Kalliopi, Fuller, George M., Kusenko, Alexander, Alexander Kusenko, Kalliopi Petraki, Fuller, George M, George M. Fuller   +6 more
core   +1 more source

The continuous readout stream of the MicroBooNE liquid argon time projection chamber for detection of supernova burst neutrinos [PDF]

Journal of Instrumentation, 2020
The MicroBooNE continuous readout stream is a parallel readout of the MicroBooNE liquid argon time projection chamber (LArTPC) which enables detection of non-beam events such as those from a supernova neutrino burst.
P. Abratenko, M. Alrashed, Rui An, J. Anthony, J. Asaadi, A. Ashkenazi, S. Balasubramanian, B. Baller, C. Barnes, G. Barr, V. Basque, L. Bathe-Peters, O. Rodrigues, S. Berkman, A. Bhanderi, A. Bhat, M. Bishai, A. Blake, T. Bolton, L. Camilleri, D. Caratelli, I. Terrazas, R. C. Fernández, F. Cavanna, G. Cerati, Y. Chen, E. Church, D. Cianci, E. Cohen, J. Conrad, M. Convery, L. Cooper-Troendle, J. I. Crespo-Anadón, M. Tutto, D. Devitt, R. Diurba, L. Dominé, R. Dorrill, K. Duffy, S. Dytman, B. Eberly, A. Ereditato, L. E. Sanchez, J. Evans, A. Fadeeva, G. A. F. Aguirre, R. Fitzpatrick, B. Fleming, N. Foppiani, D. Franco, A. Furmanski, D. Garcia-Gamez, S. Gardiner, S. Gollapinni, O. Goodwin, E. Gramellini, P. Green, H. Greenlee, L. Gu, W. Gu, R. Guenette, P. Guzowski, E. Hall, P. Hamilton, O. Hen, G. Horton-Smith, A. Hourlier, E. Huang, R. Itay, C. James, J. de Vries, X. Ji, L. Jiang, J. Jo, R.A. Johnson, Y. Jwa, N. Kamp, G. Karagiorgi, W. Ketchum, B. Kirby, M. Kirby, T. Kobilarcik, I. Kreslo, R. LaZur, I. Lepetic, K. Li, Y. Li, B. Littlejohn, D. Lorca, W. Louis, X. Luo, A. Marchionni, S. Marcocci, C. Mariani, D. Marsden, J. Marshall, J. Martín-Albo, D. A. Caicedo, K. Mason, A. Mastbaum, N. McConkey, V. Meddage, T. Mettler, K. Miller, J. Mills, K. Mistry, A. Mogan, T. Mohayai, J. Moon, M. Mooney, A. Moor, C. Moore, J. Mousseau, M. Murphy, D. Naples, A. Navrer-Agasson, R. Neely, P. Nienaber, J. Nowak, O. Palamara, V. Paolone, A. Papadopoulou, V. Papavassiliou, S. Pate, A. Paudel, Z. Pavlovic, E. Piasetzky, I. Ponce-Pinto, D. Porzio, S. Prince, X. Qian, J. Raaf, V. Radeka, A. Rafique, M. Reggiani-Guzzo, L. Ren, L. Rochester, J. Rondon, H. Rogers, M. Rosenberg, M. Ross-Lonergan, B. Russell, G. Scanavini, D. Schmitz, A. Schukraft, M. Shaevitz, R. Sharankova, J. Sinclair, A. Smith, E. Snider, M. Soderberg, S. Söldner-Rembold, P. Spentzouris, J. Spitz, M. Stancari, J. St. John, T. Strauss, K. Sutton, S. Sword-Fehlberg, A. Szelc, N. Tagg, W. Tang, K. Terao, R. Thornton, C. Thorpe, M. Toups, Y. Tsai, S. Tufanli, M. Uchida, T. Usher, W. Van De Pontseele, R. G. Van de Water, B. Viren, M. Weber, H. Wei, Z. Williams, S. Wolbers, T. Wongjirad, M. Wospakrik, W. Wu, T. Yang, G. Yarbrough, L. Yates, G. Zeller, J. Zennamo, C. Zhang   +185 more
semanticscholar   +1 more source