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The top documents tagged [neutrino emission]
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neutrino emission
Piero Galeotti Università di Torino and INFN GianVittorio Pallottino Università di Roma and INFN Guido Pizzella Università di Roma Tor Vergata INFN- Frascati.
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MAGNETARS AS COOLING NEUTRON STARS WITH MAGNETARS AS COOLING NEUTRON STARS WITH INTERNAL HEATING INTERNAL HEATING A.D. Kaminker, D.G. Yakovlev, A.Y. Potekhin,
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ICECUBE & Limits on neutrino emission from gamma-ray bursts IceCube collaboration Journal Club talk 4.15.2011 Alex Fry.
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Neutrino emission =0.27 MeV E=0.39,0.86 MeV =6.74 MeV ppI loss: ~2% ppII loss: 4% note: /Q= 0.27/26.73 = 1% ppIII loss: 28% Total loss: 2.3%
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Neutrinos from gamma-ray bursts, and tests of the cosmic ray paradigm GGI seminar Florence, Italy July 2, 2012 Walter Winter Universität Würzburg TexPoint.
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Neutron Stars 3: Thermal evolution Andreas Reisenegger Depto. de Astronomía y Astrofísica Pontificia Universidad Católica de Chile.
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X-Ray image of Crab Nebula Pulsar Credit: NASA/CXC/ASU/J. Hester et al.) Liliana Caballero With Pf. Horowitz Molecular Dynamics Simulations of Non-uniform.
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This dish measured 20 millirad /hour when the counter was placed directly on it. The mantle measured 9 mr/hr. The No Salt has a lower level of radioactivity.
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Neutron Stars 3: Thermal evolution Andreas Reisenegger ESO Visiting Scientist Associate Professor, Pontificia Universidad Católica de Chile.
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Gravitational waves and neutrino emission from the merger of binary neutron stars Kenta Kiuchi Collaboration with Y. Sekiguchi, K. Kyutoku, M. Shibata.
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COOLING OF NEUTRON STARS D.G. Yakovlev Ioffe Physical Technical Institute, St.-Petersburg, Russia Ladek Zdroj, February 2008, 1. Formulation of the Cooling.
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Lecture 14 Neutrino-Powered Explosions Mixing, Rotation, and Making Black Holes.
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