Neutrinos in Astrophysics and Cosmology - INFN Sezione di Ferrara

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Stellar Collapse and Supernova Explosion Main-sequence Main Onion sequence structure star Degenerate iron core: ρ ≈ 10 9 g cm −3 T ≈ 10 10 K MFe Fe ≈ 1.5 M sun RFe Fe ≈ 8000 km Hydrogen Burning Collapse Helium-burning Helium burning (implosion) star Helium Burning Hydrogen Burning Georg Raffelt, Max-Planck-Institut für Physik, München, Germany IDAPP 2d Meeting, 12-13 May 2006, Ferrara, Italy
Stellar Collapse and Supernova Explosion Newborn Neutron Star ~ 50 km Neutrino Cooling Proto-Neutron Proto Neutron Star ρ ≈ ρnuc nuc = 3 × 10 14 g cm −3 T ≈ 30 MeV Collapse Explosion (implosion) Georg Raffelt, Max-Planck-Institut für Physik, München, Germany IDAPP 2d Meeting, 12-13 May 2006, Ferrara, Italy
Page 1 and 2: Fermion Mass Spectrum IDAPP 2d Meet
Page 3 and 4: ⎛ ν ⎜ ⎜ ν ⎜ ⎝ ν 3 2 1
Page 5: Georg Raffelt, Max-Planck-Institut
Page 9 and 10: Neutrino Signal of Supernova 1987A
Page 11 and 12: Large Detectors for Supernova Neutr
Page 13 and 14: The Future: A Megatonne Detector? M
Page 15 and 16: IceCube as a Supernova Neutrino Det
Page 17 and 18: Level-Crossing Level Crossing Diagr
Page 19 and 20: SN statistics in external galaxies
Page 21 and 22: Experimental Limits on Relic Supern
Page 23 and 24: DSNB Measurement with Neutron Taggi
Page 25 and 26: Formation of Structure Smooth Struc
Page 27 and 28: Neutrino Free Streaming - Transfer
Page 29 and 30: Sensitivity Forecasts for Future LS
Page 31 and 32: Extending the Mass Bound to Other L
Page 33 and 34: Mass Limits on Hot Dark Matter Axio
Page 35 and 36: Dirac masses from coupling to stand
Page 37 and 38: Leptogenesis by Majorana Neutrino D
Page 39 and 40: Leptogenesis by Majorana Neutrino D
Page 41 and 42: Portion of the Hubble Ultra Deep Fi

Neutrinos in Astrophysics and Cosmology - INFN Sezione di Ferrara

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