Hamburg Neutrinos from Supernova Explosions ... - DESY Library

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Contents 1 I Session: Astrophysical Aspects 1 Neutrinos and Supernovae 3 Stephen W. Bruenn, Eric J. Lentz, Eric J. Lingerfelt, Anthony Mezzacappa, Raphael W. Hix, John N. Blondin, O. E. Bronson Messer, Pedro Marronetti Core-Collapse Supernovae: Explosion Dynamics, Neutrinos and Gravitational Waves 14 Bernhard Müller, Hans-Thomas Janka, Andreas Marek, Florian Hanke, Annop Wongwathanarat, Ewald Müller New Aspects and Boundary Conditions of Core-Collapse Supernova Theory 22 Christian Ott, Evan P. O’Connor, Basudeb Dasgupta Long-term evolution of massive star explosions 36 Tobias Fischer, Matthias Liebendörfer, Friedrich K. Thielemann, Gabriel Martínez-Pinedo, Benedikt Ziebarth, Karlheinz Langanke Neutrino-driven winds and nucleosynthesis of heavy elements 48 Almudena Arcones Equation of State for Supernova 52 Gang Shen 2 II Session: Particle Physics Aspects 57 Supernova as Particle-Physics Laboratory 59 Georg Raffelt Supernova neutrino flavor evolution of high densities 65 A. Baha Balantekin Supernova bound on keV-mass sterile neutrinos 75 Shun Zhou Supernovae and sterile neutrinos 79 Irene Tamborra HAνSE 2011 vii
Page 1 and 2: Proceedings of the Hamburg Neutrino
Page 3 and 4: Organizing Committee Sovan Chakrabo
Page 5: Acknowledgements The organizers wou
Page 9: Chapter 1 Astrophysical Aspects Con
Page 12 and 13: ely on the correlations between the
Page 14 and 15: and deposits energy in the surround
Page 16 and 17: STEPHEN W. BRUENN, ERIC J. LENTZ, E
Page 22 and 23: Core-Collapse Supernovae: Explosion
Page 24 and 25: BERNHARD MÜLLER, HANS-THOMAS JANKA
Page 26 and 27: E2 GW amplitude A [cm] 20 50 0 -50
Page 28 and 29: 2D to 3D. First predictions based o
Page 30 and 31: New Aspects and Boundary Conditions
Page 32 and 33: CHRISTIAN OTT, EVAN P. O’CONNOR,
Page 40 and 41: 4 Summary and Outlook In this contr
Page 44 and 45: Long-term evolution of massive star
Page 46 and 47: TOBIAS FISCHER, MATTHIAS LIEBENDÖR
Page 48 and 49: during the initial shock expansion
Page 50 and 51: Luminosity [erg/s] Mean Energy [MeV
Page 52 and 53: Spectra [a. u.] Spectra [a. u.] 0.0
Page 54 and 55: Acknowledgement The work was suppor
Page 56 and 57:
Neutrino-driven winds and nucleosyn
Page 58 and 59:
3 Lighter heavy elements in neutrin
Page 60 and 61:
Equation of State for Supernova Gan
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Model ρ0 (fm −3 ) ε0 (MeV) K0 (
Page 65:
Chapter 2 Particle Physics Aspects
Page 68 and 69:
to the eV range [17]. It is more in
Page 70 and 71:
4 Flavor and lepton number violatio
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[38] P. Fayet, D. Hooper and G. Sig
Page 74 and 75:
approach is helpful in exploring th
Page 76 and 77:
Defining z(p, t) = ψx(p, t) ψe(p,
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equation � p −jp wp−ξ most g
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so that we obtain a diagonal Hamilt
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[16] H. Duan, G. M. Fuller and Y. Z
Page 84 and 85:
Moreover, the WDM sterile neutrinos
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larger than that of ordinary neutri
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t 0.5 Rν 25 Lνe 9.5 Lνe 10.06 L
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Flux (a.u.) Flux (a.u.) Flux (a.u.)
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Turbulence and Supernova Neutrinos
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f(P 11 ) f(P 22 ) f(P 33 ) 4 2 0 4
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f(P 11 ), f(P 12 ), f(P( 13 ) 1000
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Collective neutrino oscillations in
Page 100 and 101:
ALESSANDRO MIRIZZI, SOVAN CHAKRABOR
Page 102 and 103:
Flavor Stability Analysis of Supern
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3 Results We aim at comparing the l
Page 107:
Chapter 3 Phenomenology and Detecti
Page 110 and 111:
addition, the νe and νµ spectra
Page 112 and 113:
the numerical investigation of the
Page 114 and 115:
The resonant energies increase with
Page 116 and 117:
Cherenkov, IceCube), the latter met
Page 118 and 119:
the shock propagation and (iii) the
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[41] H. Duan, G. M. Fuller and Y. Z
Page 122 and 123:
predictions, with their related unc
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dσ/dω (10 -42 cm 2 MeV -1 ) 100 1
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dσ/dω (10 -42 cm 2 MeV -1 ) 10 1
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0.5 0.45 0.4 0.35 0.3 0.25 0.2 0.15
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[10] B.E. Bodmann et al., Phys. Let
Page 132 and 133:
analyzing a rolling time window. Si
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DOM Hits (50ms binning) 100 95 90 8
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Supernova Neutrinos in Liquid Scint
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2 Neutrino-proton elastic scatterin
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SN neutrinos in LVD Walter Fulgione
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Duty Cycle (%) 100 80 60 40 20 0 19
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References [1] LVD Collaboration, I
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2 Neutrino flavor evolution: the fo
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4 Conclusions We have presented new
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2 Detector description and performa
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Figure 3: (color online) The rise t
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Neutrino Forecast: Mostly Sunny, wi
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NEUTRINO FORECAST: MOSTLY SUNNY, WI
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Page 161 and 162:
Page 163 and 164:
Page 165 and 166:
Page 167:
List of Authors Arcones, Almudena,
Page 170 and 171:
Sigl, Günter (Hamburg University)
Page 172 and 173:
164 HAνSE 2011
Page 174:
166 HAνSE 2011
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