Hamburg Neutrinos from Supernova Explosions ... - DESY Library

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Impressum Proceedings of the Hamburg Neutrinos from Supernova Explosion (HAνSE 2011) July 19-23, 2011, Hamburg, Germany Conference homepage http://hanse2011.desy.de/ Slides at http://hanse2011.desy.de/e119287/ Online proceedings at http://www-library.desy.de/preparch/desy/proc/proc11-03.html The copyright is governed by the Creative Commons agreement, which allows for free use and distribution of the articles for non-commercial activity, as long as the title, the authors’ names and the place of the original are referenced. Editors: Alessandro Mirizzi, Pasquale Dario Serpico, Günter Sigl December 2011 DESY-PROC-2011-03 ISBN 978-3-935702-53-9 ISSN 1435-8077 Published by Verlag Deutsches Elektronen-Synchrotron Printed by Kopierzentrale Deutsches Elektronen-Synchrotron Notkestraße 85 22607 Hamburg Germany ii
Organizing Committee Sovan Chakraborty, Alessandro Mirizzi (Chairman), Günter Sigl, Ricard Tomàs Bayo II Institut für Theoretische Physik Universität Hamburg Luruper Chaussee 149 D-22761 Hamburg Caren Hagner I Institut für ExperimentalPhysik Universität Hamburg Luruper Chaussee 149 D-22761 Hamburg Pasquale Dario Serpico Laboratoire de Physique Theorique Univ. de Savoie, CNRS B.P.110 F-74941 Annecy-Le-Vieux Conference Secretary and Local Organization Wiebke Kircheisen and Marco Baumgartl II Institut für Theoretische Physik Universität Hamburg Luruper Chaussee 149 D-22761 Hamburg iii
Page 1: Proceedings of the Hamburg Neutrino
Page 5: Acknowledgements The organizers wou
Page 8 and 9: Turbulence and Supernova Neutrinos
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 53 and 54:
LONG-TERM EVOLUTION OF MASSIVE STAR
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LONG-TERM EVOLUTION OF MASSIVE STAR
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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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