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281por Seo, E S, Ahn, H S, Allison, P S, Beatty, J J, Choi, M J, Conklin, N B, Coutu, S, DuVernois, M A, Ganel, O, Kim, K C, Lee, M H, Liu, L, Lutz, L, Maestro, P, Marrocchesi, P S, Minnick, S A, Min, K W, Mognet, S I, Nutter, S, Park, H, Schindhelm, E, Song, C, Swordy, S, Wu, J, Yang, J“…Ground-based indirect measurements have shown that the cosmic-ray allparticle spectrum extends many orders of magnitude beyond the energy thought possible for supernova acceleration. Our balloon-borne Cosmic Ray Energetics And Mass (CREAM) experiment is capable of extending direct measurements of cosmic-rays to the supernova energy scale of 1015 eV in a series of Ultra Long Duration Balloon (ULDB) flights. …”
Publicado 2003
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282por Helfand, D J“…"Created in a recent supernova explosion, a young neutron star reveals secrets of nuclear matter" (2 pages).…”
Publicado 2003
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283por Vannucci, François“…Concerning neutrinos, the detection is still limited to terrestrial ones (apart from supernova production). A new way to search for extragalactic neutrinos is discussed.…”
Publicado 2001
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284por Livio, M“…Adam Riess, acting on behalf of the High-Z Supernova Team at the Space Telescope Science Institute, published a paper in 1998 which concluded that the universe's expansion is actually accelerating instead of slowing down (2 pages).…”
Publicado 2002
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285Publicado 2003“…These programs, using Grid computing technology, will help astronomers detect some of the most dramatic events in the universe, such as massive supernova explosions (1 page).…”
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286por Brouet, Anne-Muriel“…A team of physicists from CERN and from Technion, the Israel Institute of Technology, used gamma rays to successfully forecast a supernova explosion (0.5 page)…”
Publicado 2003
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287“…The axion signal will be an excess in $\gamma$-rays coming either from a specific celestial place behind the Sun, e.g. the Galactic Center, or, from any other direction in the sky being associated with a violent astrophysical event, e.g. a supernova. Earth bound detectors are also of potential interest. …”
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288“…For the 1/r^3 profile typical of supernova envelopes we compare our analytical to numerical results and to earlier approximations used in the literature. …”
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289“…We find that in the regions where the neutrino-neutrino refractive index leads to collective flavor oscillations, the presence of new neutrino interactions can produce flavor equilibration in both normal and inverted neutrino mass hierarchy. In realistic supernova environments, these effects are significant if the nonstandard neutrino-neutrino interaction strength is comparable to the one expected in the standard case, dominating the ordinary matter potential. …”
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290“…Our results affect the flavour evolution of dense neutrino gases and may be of interest for collective three-flavour oscillations of supernova neutrinos. We spell out explicitly how these non-universal neutrino-neutrino interactions enter the flavour oscillation equations.…”
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291“…We analyze the possibility of superluminal neutrino propagation delta v = (v - c)/c > 0 as indicated by OPERA data, in view of previous phenomenological constraints from supernova SN1987a and gravitational Cerenkov radiation. …”
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292por Botella, Ines Gil“…This multipurpose detector opens up unique opportunities to look for phenomena beyond the Standard Model through the study of atmospheric, solar and supernova neutrinos, nucleon decay searches and neutrinos from the CERN to Gran Sasso beam. …”
Publicado 2003
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293“…This mechanism may also be relevant for Gamma Ray Bursts and, in the absence of magnetic field, supernova explosions.…”
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294“…We study the impact of neutrino magnetic moments on astrophysical neutrinos, in particular supernova neutrinos and ultra-high energy neutrinos from extragalactic sources. …”
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295por Yang, Bin, Jin, Zhi-Ping, Li, Xiang, Covino, Stefano, Zheng, Xian-Zhong, Hotokezaka, Kenta, Fan, Yi-Zhong, Piran, Tsvi, Wei, Da-Ming“…Long-duration (>2 s) γ-ray bursts that are believed to originate from the death of massive stars are expected to be accompanied by supernovae. GRB 060614, that lasted 102 s, lacks a supernova-like emission down to very stringent limits and its physical origin is still debated. …”
Publicado 2015
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296“…The concepts of Early Vascular Aging (EVA) and Supernormal Vascular Aging (SUPERNOVA) help to better understand on which determinants of arterial stiffness it is possible to act, in order to limit target organ damage and cardiovascular complications. …”
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297por Kopal, Zdenek“…Cataclysmic variables refer to an object in one of three classes: dwarf nova, nova, or supernova. These topics are followed by discussions on the eclipse phenomena and the eclipses i…”
Publicado 1963
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298por Raffelt, Georg G“…These fluxes can be used for direct measurements (e.g. solar or supernova neutrinos) or the back-reaction on the star can be used to derive limits on new particles. …”
Publicado 2002
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299por Ellis, John R., Harries, Nicholas, Meregaglia, Anselmo, Rubbia, Andre, Sakharov, Alexander“…We consider the limits that may be set on a linear or quadratic violation of Lorentz invariance in the propagation of energetic neutrinos, v/c=[1 +- (E/M_\nuQG1)] or [1 +- (E/M_\nu QG2}^2], using data from supernova explosions and the OPERA long-baseline neutrino experiment. …”
Publicado 2008
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300“…Presents the story of radio astronomy, of how radio waves are generated by stars, supernova, quasars, colliding galaxies, and by the very beginnings of the universe itself. …”
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