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103“…The exceptional cosmic history and the fabulous destinies of exploding stars – supernovae and gamma-ray bursters – are highly fertile areas of research and are also very special tools to further our understanding of the universe. …”
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104“…A recently proposed model (arXiv:0903.2794) explains the rise in energy of the positron fraction measured by the PAMELA satellite in terms of hadronic production of positrons in aged supernova remnants, and acceleration therein. Here we present a preliminary calculation of the anti-proton flux produced by the same mechanism. …”
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105
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106
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107
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108“…Motivated by recent measurements of deposits of $^{60}$Fe on the ocean floor and the lunar surface, we model the transport of dust grains containing $^{60}$Fe from a near-Earth (i.e., within 100 pc) supernova (SN). We inject dust grains into the environment of an SN remnant (SNR) and trace their trajectories by applying a 1D hydrodynamic description assuming spherical symmetry to describe the plasma dynamics, and we include a rudimentary, 3D magnetic field description to examine its influence on charged dust grains. …”
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109
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110
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111por Fields, Brian D., Ellis, John R., Binns, Walter R., Breitschwerdt, Dieter, deNolfo, Georgia A., Diehl, Roland, Dwarkadas, Vikram V., Ertel, Adrienne, Faestermann, Thomas, Feige, Jenny, Fitoussi, Caroline, Frisch, Priscilla, Graham, David, Haley, Brian, Heger, Alexander, Hillebrandt, Wolfgang, Israel, Martin H., Janka, Thomas, Kachelreiß, Michael, Korschinek, Gunther, Limongi, Marco, Lugaro, Maria, Marinho, Franciole, Melott, Adrian, Mewaldt, Richard A., Miller, Jesse, Ogliore, Ryan C., Paul, Michael, Paulucci, Laura, Pecaut, Mark, Rauch, Brian F., Rehm, Karl E., Schulreich, Michael, Seitenzahl, Ivo, Sørensen, Mads, Thielemann, Friedrich-Karl, Timmes, Francis X., Thomas, Brian C., Wallner, Anton“…There is now solid experimental evidence of at least one supernova explosion within 100 pc of Earth within the last few million years, from measurements of the short-lived isotope 60Fe in widespread deep-ocean samples, as well as in the lunar regolith and cosmic rays. …”
Publicado 2019
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112
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113por Robles, Sandra“…--HTML-->Upcoming neutrino experiments are expected to detect the Diffuse Supernova Neutrino Background (DSNB). This requires pondering all possible sources of background. …”
Publicado 2023
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114
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115
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116
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117por Ambrosio, M, Antolini, R, Auriemma, G, Baker, R, Baldini, A, Barbarino, G C, Barish, B C, Battistoni, G, Bellotti, R, Bemporad, C, Bernardini, P, Bilokon, H, Bisi, V, Bloise, C, Bower, C, Bussino, S, Cafagna, F, Calicchio, M, Campana, D, Carboni, M, Castellano, M G, Cecchini, S, Cei, F, Celio, P, Chiarella, V, Corona, A, Coutu, S, De Benedictis, L, De Cataldo, G, Dekhissi, H, De Marzo, C, De Mitri, I, De Vincenzi, M, Di Credico, A, Erriquez, O, Favuzzi, C, Forti, C, Fusco, P, Giacomelli, G, Giannini, G, Giglietto, N, Grassi, M, Gray, L, Grillo, A, Guarino, F, Guarnaccia, P, Gustavino, C, Habig, A, Hanson, K, Hawthorne, A, Heinz, R, Hong, J T, Iarocci, Enzo, Katsavounidis, E, Kearns, E T, Kyriazopoulou, S, Lamanna, E, Lane, C, Levin, D S, Lipari, P, Liu, R, Longley, N P, Longo, M J, Ludlam, G, Maaroufi, F, Mancarella, G, Mandrioli, G, Manzoor, S, Margiotta-Neri, A, Marini, A, Martello, D, Marzari-Chiesa, A, Mazziotta, M N, Mazzotta, C, Michael, D G, Mikheyev, S P, Miller, L, Monacelli, P, Montaruli, T, Monteno, M, Mufson, S L, Musser, J, Nicoló, D, Nolty, R, Okada, C, Orth, C, Osteria, G, Palamara, O, Parlati, S, Patera, V, Patrizii, L, Pazzi, R, Peck, C W, Petrera, S, Pistilli, P, Popa, V, Rainó, A, Reynoldson, J, Ronga, F, Rubizzo, U, Sanzgiri, A, Satriano, C, Satta, L, Scapparone, E, Scholberg, K, Sciubba, A, Serra-Lugaresi, P, Severi, M, Sioli, M, Sitta, M, Spinelli, P, Spinetti, M, Spurio, M, Steinberg, R, Stone, J L, Sulak, Lawrence R, Surdo, A, Tarlé, G, Togo, V, Valente, V, Walter, C W, Webb, REnlace del recurso
Publicado 1997
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118
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119“…We reconsider the influence of these decays on the neutrino signal of supernovae in the light of recent Super-Kamiokande data on solar and atmospheric neutrinos. …”
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120