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Documents Piero Galeotti Università di Torino and INFN GianVittorio Pallottino Università di Roma and INFN.....

Slide 1Piero Galeotti Università di Torino and INFN GianVittorio Pallottino Università di Roma and INFN Guido Pizzella Università di Roma Tor Vergata INFN- Frascati SN1987A…

Documents MAGNETARS AS COOLING NEUTRON STARS WITH MAGNETARS AS COOLING NEUTRON STARS WITH INTERNAL HEATING...

Slide 1MAGNETARS AS COOLING NEUTRON STARS WITH MAGNETARS AS COOLING NEUTRON STARS WITH INTERNAL HEATING INTERNAL HEATING A.D. Kaminker, D.G. Yakovlev, A.Y. Potekhin, N. Shibazaki*,…

Documents ICECUBE & Limits on neutrino emission from gamma-ray bursts IceCube collaboration Journal Club talk....

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Documents Neutrino emission =0.27 MeV E=0.39,0.86 MeV =6.74 MeV ppI loss: ~2% ppII loss: 4% note: /Q=...

Slide 1 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% Slide 2 2 neutrino energies…

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Documents Neutron Stars 3: Thermal evolution Andreas Reisenegger Depto. de Astronomía y Astrofísica...

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Documents This dish measured 20 millirad /hour when the counter was placed directly on it. The mantle measured...

Slide 1 Slide 2 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…

Documents Neutron Stars 3: Thermal evolution Andreas Reisenegger ESO Visiting Scientist Associate Professor,.....

Neutron Stars 3: Thermal evolution Andreas Reisenegger ESO Visiting Scientist Associate Professor, Pontificia Universidad Católica de Chile Outline Cooling processes of…

Documents Gravitational waves and neutrino emission from the merger of binary neutron stars Kenta Kiuchi...

Gravitational waves and neutrino emission from the merger of binary neutron stars Gravitational waves and neutrino emission from the merger of binary neutron stars Kenta…