Hamburg Neutrinos from Supernova Explosions ... - DESY Library

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Turbulence and Supernova Neutrinos 84 James P. Kneller Collective neutrino oscillations in supernovae: Matter suppression during the accretion phase 90 Alessandro Mirizzi, Sovan Chakraborty, Ninetta Saviano Flavor Stability Analysis of Supernova Neutrino Fluxes Compared with Simulations 94 Srdjan Sarikas, Georg Raffelt 3 III Session: Phenomenology and Detection Strategies 99 Signatures of supernova neutrino oscillations 101 Amol Dighe Low-energy Neutrino-Nucleus Cross Sections 113 Natalie Jachowicz Supernova neutrino signal in IceCube 123 Gösta Kroll for the Icecube Collaboration Supernova Neutrinos in Liquid Scintillator Detectors by means of neutrino-proton elastic scattering 128 Aldo Ianni Supernova neutrinos in LVD 132 Walter Fulgione for the LVD Collaboration Supernova Neutrino Signal at HALO: Learning about the Primary Neutrino Fluxes 137 Daavid Väänänen, Cristina Volpe Supernova Neutrino Detection via Coherent Scattering 141 Georgios Tsiledakis, E. Bougamont, P. Colas, A. Dastgheibi-Fard, J. Derre, I. Giomataris, G. Gerbier, M. Gros, P. Magnier, X. F. Navick, P. Salin, I. Savvidis, J. D. Vergados 4 Summary Talk 145 Neutrino Forecast: Mostly Sunny, with a Good Chance of Supernovas 147 Mark Vagins viii
Chapter 1 Astrophysical Aspects Convenors: Chris Cardall Gail McLaughlin HAνSE 2011 1
Page 1 and 2: Proceedings of the Hamburg Neutrino
Page 3 and 4: Organizing Committee Sovan Chakrabo
Page 5: Acknowledgements The organizers wou
Page 11 and 12: Neutrinos and Supernovae Stephen W
Page 13 and 14: NEUTRINOS AND SUPERNOVAE some form
Page 15 and 16: NEUTRINOS AND SUPERNOVAE shock beco
Page 17 and 18: NEUTRINOS AND SUPERNOVAE spectral P
Page 19 and 20: NEUTRINOS AND SUPERNOVAE 6 Conclusi
Page 21 and 22: NEUTRINOS AND SUPERNOVAE [45] S. W.
Page 23 and 24: CORE-COLLAPSE SUPERNOVAE: EXPLOSION
Page 31 and 32: NEW ASPECTS AND BOUNDARY CONDITIONS
Page 45 and 46: LONG-TERM EVOLUTION OF MASSIVE STAR
Page 57 and 58: NEUTRINO-DRIVEN WINDS AND NUCLEOSYN
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NEUTRINO-DRIVEN WINDS AND NUCLEOSYN
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EQUATION OF STATE FOR SUPERNOVA Tab
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EQUATION OF STATE FOR SUPERNOVA res
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Supernova as Particle-Physics Labor
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SUPERNOVA AS PARTICLE-PHYSICS LABOR
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SUPERNOVA AS PARTICLE-PHYSICS LABOR
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Supernova neutrino flavor evolution
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SUPERNOVA NEUTRINO FLAVOR EVOLUTION
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Supernova bound on keV-mass sterile
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SUPERNOVA BOUND ON KEV-MASS STERILE
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Supernovae and sterile neutrinos Ir
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SUPERNOVAE AND STERILE NEUTRINOS Fi
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SUPERNOVAE AND STERILE NEUTRINOS Fl
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TURBULENCE AND SUPERNOVA NEUTRINOS
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COLLECTIVE NEUTRINO OSCILLATIONS IN
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COLLECTIVE NEUTRINO OSCILLATIONS IN
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FLAVOR STABILITY ANALYSIS OF SUPERN
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FLAVOR STABILITY ANALYSIS OF SUPERN
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Signatures of supernova neutrino os
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SIGNATURES OF SUPERNOVA NEUTRINO OS
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Low-energy Neutrino-Nucleus Cross S
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LOW-ENERGY NEUTRINO-NUCLEUS CROSS S
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Supernova neutrino signal in IceCub
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SUPERNOVA NEUTRINO SIGNAL IN ICECUB
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SUPERNOVA NEUTRINO SIGNAL IN ICECUB
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SUPERNOVA NEUTRINOS IN LIQUID SCINT
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SUPERNOVA NEUTRINOS IN LIQUID SCINT
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SUPERNOVA NEUTRINOS IN LVD on-line
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SUPERNOVA NEUTRINOS IN LVD Table 1:
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Supernova Neutrino Signal at HALO:
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SUPERNOVA NEUTRINO SIGNAL AT HALO:
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Supernova Neutrino Detection via Co
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SUPERNOVA NEUTRINO DETECTION VIA CO
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Chapter 4 Summary Talk HAνSE 2011
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“HANSE”, a quite resonant word
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most likely energy range, as well a
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Note that without neutron tagging,
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the exploding star was big and rath
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MARK VAGINS Figure 13: The selectiv
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other, unrelated topics like proton
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List of Participants Arcones, Almud
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HAνSE 2011 163
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HAνSE 2011 165
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