Proc. Neutrino Astrophysics - MPP Theory Group

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vi S.J. Hardy Quasilinear Diffusion of Neutrinos in Plasma ...................................... 75 P. Elmfors Anisotropic Neutrino Propagation in a Magnetized Plasma ......................... 79 A.N. Ioannisian, G.G. Raffelt Cherenkov Radiation by Massless Neutrinos in a Magnetic Field ................... 83 A. Kopf Photon Dispersion in a Supernova Core ............................................ 86 Gamma-Ray Bursts D.H. Hartmann, D.L. Band Gamma-Ray Burst Observations ................................................... 91 S.E. Woosley, A. MacFadyen Gamma-Ray Bursts: Models That Don’t Work and Some That Might ............... 96 M. Ruffert, H.-Th. Janka Models of Coalescing Neutron Stars with Different Masses and Impact Parameters 101 R.A. Sunyaev Physical Processes Near Black Holes .............................................. 106 High-Energy Neutrinos K. Mannheim Astrophysical Sources of High -Energy Neutrinos .................................. 109 P. Gondolo Atmospheric Muons and Neutrinos Above 1TeV .................................. 112 D. Kie̷lczewska Atmospheric Neutrinos in Super-Kamiokande ..................................... 116 Ch. Wiebusch Neutrino Astronomy with AMANDA ............................................. 121 M.E. Moorhead High Energy Neutrino Astronomy with ANTARES ................................ 127 R. Plaga Ground-Based Observation of Gamma-Rays (200GeV–100TeV) .................. 130 Cosmology C.J. Hogan Helium Absorption and Cosmic Reionization ...................................... 139 K. Jedamzik Non-Standard Big Bang Nucleosynthesis Scenarios ................................ 141 J.B. Rehm, K. Jedamzik Big Bang Nucleosynthesis With Small-Scale Matter-Antimatter Domains .......... 147
M. Bartelmann Neutrinos and Structure Formation in the Universe ............................... 149 Future Prospects P. Meunier Neutrino Experiments with Cryogenic Detectors .................................. 161 P.F. Smith OMNIS—A Galactic Supernova Observatory ...................................... 165 J. Valle Neutrinos in Astrophysics ........................................................ 170 L. Stodolsky Some Neutrino Events of the 21st Century ........................................ 178 Appendix Workshop Program and List of Participants ...................................... 183 Our Sonderforschungsbereich (SFB) “Astro-Teilchen-Physik” and its Divisions .... 193 vii
Page 1 and 2: arXiv:astro-ph/9801320v1 30 Jan 199
Page 3: Preface This was the fourth worksho
Page 8 and 9: viii
Page 11 and 12: History of Neutrino Physics: Pauli
Page 13 and 14: Brief an Oskar Klein, Stockholm, vo
Page 15 and 16: Recent observations with the Hubble
Page 17 and 18: MACHO sample of ∼100,000 light cu
Page 19: Solar Neutrinos
Page 22 and 23: 14 In the depth range where an abun
Page 24 and 25: 16 as follows: (1) All the detector
Page 26 and 27: 18 [3] J.N. Bahcall and H.A. Bethe,
Page 28 and 29: 20 the opacity has a very slowly ch
Page 30 and 31: 22 Status of the Radiochemical Gall
Page 32 and 33: 24 known true source activity. The
Page 34 and 35: 26 Solar Neutrino Observation with
Page 36 and 37: 28 Events/day/kton/bin 0.3 0.25 0.2
Page 38 and 39: 30 log(Δm 2 (eV 2 log(Δm )) 2 (eV
Page 40 and 41: 32 Table 1: Neutrino event rates in
Page 42 and 43: 34 tank and sphere high purity wate
Page 44 and 45: 36 Measurements of Low Energy Nucle
Page 46 and 47: 38 Figure 1: The S(E) factor of 3 H
Page 48 and 49: 40 Solar Neutrinos: Where We Are an
Page 50 and 51: 42 [9] B. Pontecorvo, Chalk River R
Page 52 and 53: 44 Figure 2: The difference between
Page 55 and 56: Phenomenology of Supernova Explosio
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Figure 2: Theoretical classificatio
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Supernova Rates Bruno Leibundgut Eu
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galaxies, however, and the statisti
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Figure 1: The motions of pulsars re
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Convection in Newly Born Neutron St
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a b Figure 2: Panel a shows the rec
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ference). The angular variations of
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Figure 1: Neutrino luminosity and e
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[9] G.S. Bisnovatyi-Kogan, Astron.
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and the mass-to-luminosity ratio of
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Figure 1: Time variation of superno
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Figure 3: Energy spectra of the sup
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Supernova Neutrino Opacities G.G. R
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Quasilinear Diffusion of Neutrinos
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Assuming a saturated thermal distri
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Anisotropic Neutrino Propagation in
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So far the damping rate corresponds
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Cherenkov Radiation by Massless Neu
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on ω so that they are well approxi
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2 2 / meff,e m eff 1.0 0.5 0.0 elec
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Gamma-Ray Burst Observations D.H. H
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Figure 1: The cumulative distributi
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[7] Lilly, S., in Critical Dialogue
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) Phase Transitions in Neutron Star
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after the collapse began (nb., no e
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Models of Coalescing Neutron Stars
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Figure 2: Contour plots of the mass
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From our torus models we find that
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High-Energy Neutrinos
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110 in gamma-rays. However, the acc
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112 Atmospheric Muons and Neutrinos
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114 Today, however, charm productio
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116 Atmospheric Neutrinos in Super-
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118 number of events 300 200 100 (a
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120 Acknowledgements D.K. is suppor
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122 Key signatures for νµ nucleon
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124 (a.u) 0.5 0.4 0.3 0.2 0.1 0 0 1
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126 However, in order to operate th
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128 could be gravitationally captur
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130 Ground-Based Observation of Gam
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132 Figure 2: Sensitivities in unit
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134 Crab flux Figure 4: Gamma-ray f
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136
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Helium Absorption and Cosmic Reioni
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Non-Standard Big Bang Nucleosynthes
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) Non-standard Neutrino Properties
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some heating of the plasma. In cont
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Big Bang Nucleosynthesis With Small
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Neutrinos and Structure Formation i
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Photon and Neutrino Backgrounds The
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The (photon) temperature at aeq is
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spectrum has therefore changed to 1
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Figure 4: Growth of structure in CD
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Future Prospects
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162 Figure 1: Calorimetric β − s
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164 References [1] F. Gatti: Procee
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166 The frequency of Galactic super
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168 Table 1: Comparison of proposed
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170 Neutrinos in Astrophysics José
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172 N eq 7 6.5 6 5.5 5 4.5 4 3.5 3
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174 Figure 4: SN 1987A bounds on FC
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176 [5] A. Joshipura and J. W. F. V
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178 Some Neutrino Events of the 21s
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180 2099: Relic Neutrinos And last
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182
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184 Tuesday, Oct. 21: Supernova Neu
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186 Michael Altmann Technische Univ
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188 Paolo Gondolo Max-Planck-Instit
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190 Patrizia Meunier Max-Planck-Ins
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192 Torsten Soldner Technische Univ
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194 A Experimental Particle Physics
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196 C Astrophysics and Cosmology C1
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