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81
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82
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83por Vagins, Mark“…--HTML-->A core-collapse supernova is a nearly perfect neutrino bomb. While capable of outshining its entire host galaxy, this stunning light show represents just a small portion of the explosion. …”
Publicado 2016
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84por Aglietta, M, Alpat, B, Alyea, E D, Antonioli, P, Anzivino, Giuseppina, Badino, G, Ban, Y, Bari, G, Basile, M, Benelli, A, Berezinsky, Veniamin Sergeevich, Bergamasco, L, Bianco, S, Bizzeti, A, Bruni, G, Cao, Y, Cara Romeo, G, Casaccia, R, Castagnoli, C, Castellina, A, Chen, K, Chen, R, Chinellato, J A, Cifarelli, Luisa, Cini, G, Cong, S, Contin, A, Dadikin, V L, Dardo, M, De Silva, A, Deutsch, M, Dos Santos, L G, Enikeev, R I, Fabbri, Franco Luigi, Fulgione, W, Galeotti, P, Ghia, P L, Giusti, P, Grianti, F, Gu, S, Hafen, E S, Haridas, P, Iacobucci, G, Inoue, N, Khalchukov, F F, Korolkova, E V, Kortchaguin, P V, Kortchaguin, V B, Kudryavtsev, V A, Landi, G, Lau, K, Lin, X, Lü, L, Ma, J, Ma, Z, Maccarrone, G D, Malguin, A S, Mao, Z, Markov, M A, Massam, Thomas, Mayes, B W, Mengotti-Silva, N, Misaki, A, Mo, G H, Monteleoni, B, Morello, C, Moromisato, J H, Nania, R, Navarra, G, Panaro, L, Parks, D P, Pelfer, P G, Periale, L, Picchi, P, Pinna, P, Pinsky, L, Pless, I A, Pu, M, Pyrlik, J, Qiu, J, Ryasny, V G, Ryazhskaya, O G, Saavedra, O, Saitô, K, Sanders, D, Sartorelli, G, Sarwar, S, Shen, D, Susinno, G, Talochkin, V P, Tang, H, Tang, J, Tian, W, Trinchero, G C, Turtelli, A, Uman, I, Vallania, P, Vernetto, S, von Goeler, E, Votano, L, Wada, T, Wang, F, Wang, H, Wang, S, Weathers, R, Weinstein, R, Widgoff, M, Xu, L, Xu, Z, Yakushev, V F, Yamamoto, I, Yi, G, Zallo, A, Zatsepin, G T, Zhou, X, Zhu, X, Zhuang, B, Zichichi, AntoninoEnlace del recurso
Publicado 1992
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85
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86
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87
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88“…Nearby supernova explosions may cause geological isotope anomalies via the direct deposition of debris or by cosmic-ray spallation in the earth's atmosphere. …”
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89
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90
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91
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92“…We reconsider the impact of $\bar\nu_e \leftrightarrow \bar\nu_{\mu,\tau}$ neutrino oscillations on the observed $\bar\nu_e$ signal of supernova SN 1987A. Performing a maximum-likelihood analysis using as fit parameters the released binding energy $\Eb$ and the average neutrino energy $\Ee$, we find as previous analyses that $\bar\nu_e \leftrightarrow \bar\nu_{\mu,\tau}$ oscillations with large mixing angles have lower best-fit values for $\Ee$ than small-mixing angle (SMA) oscillations. …”
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93por Dighe, Amol S.“…We explore the earth matter effects on the energy spectra of neutrinos from a supernova. We show that the observations of the energy spectra of $\nu_e$ and $\bar{\nu}_e$ from a galactic supernova may enable us to identify the solar neutrino solution, to determine the sign of $\Delta m^2_{32}$, and to probe the mixing matrix element $|U_{e3}|^2$ to values as low as $10^{-3}$. …”
Publicado 2001
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94
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95“…Nevertheless, the supernova core evolution is significantly modified. …”
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96Publicado 2003“…"A unique set of 11 distant Type Ia supernovae studied with the Hubble Space Telescope sheds new light on dark energy, according to the latest findings of the Supernova Cosmology Project" (2 pages).…”
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97Publicado 2003“…It appears to prove that gamma ray bursts originate in supernovae (1 page)…”
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98“…The mean iron abundance observed in the intracluster medium of galaxy clusters is consistent with the mean amount of iron injected in the universe per unit volume by standard supernova (SN) explosions with a rate proportional to the cosmic star-formation rate. …”
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99
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100