| Time | Speaker | Title |
|---|
| 09:00 - 09:25 | Ashley Ruiter, MPA
|
Progenitors of SNe Ia and Accretion
Induced Collapse
|
| 09:25 - 09:50 | Ken Shen, UC Santa Barbara
|
Helium shell detonations from AM CV_N
systems: New results on SNe Ia
|
| 09:50 - 10:15 | Michael Fink, MPA
|
Detonation in WD stars
|
| 10:15 - 10:45 | COFFEE BREAK |
| 10:45 - 11:10 | Markus Kromer, MPA
|
Radiative transfer in SNe Ia -
Predicting observables for explosion models
|
| 11:10 - 11:35 | Stuart Sim, MPA
|
Detonations in Sub-Chandrasekhar Mass
White Dwarfs: a comparison with
observations
|
| 11:35 - 12:00 | Ivo Seitenzahl, MPA
|
Internal conversion electrons and
SN light curves
|
| 12:00 - 12:25 | Daniel Sauer, Stockholm Univ.
|
Alternatively powered supernovae
|
| 12:00 - 15:00 | LUNCH BREAK |
| 15:00 - 15:25 | Claes Fransson, Oskar Klein Centre, Stockholm
|
Modeling and observations of the ejecta
and ring of SN 1987A at very late stages
|
| 15:25 - 15:55 | Fabian Miczek, MPA
|
Stability of shear flows in stellar interiors
|
| 15:55 - 16:15 | Miroslav Mocak, IAA
|
Hydrodynamic simulations of core
convection in stars
|
| 16:15 - 16:45 | COFFEE BREAK |
| 16:45 - 17:10 | Jordi Isern, IEEC Barcelona
|
Axions and the cooling of white dwarfs
|
| 17:10 - 17:35 | Matthias Hempel, Univ. Heidelberg
|
Statistical model for a complete
supernovae equation of state
|
| 17:35 - 18:00 | Irina Sagert, Univ. Frankfurt
|
EOS for explosive
astrophysical systems, including a
quark matter phase transition:
Compatibility with heavy ion and
pulsar data is considered
|
| 18:30 | DINNER |
| Time | Speaker | Title |
|---|
| 09:00 - 09:25 | Jeremiah Murphy, Univ. Washington, Seattle
|
Conditions for successful CCSN explosions
|
| 09:25 - 09:50 | Rodrigo Fernandez, IAS Princeton
|
Progress on the SASI
|
| 09:50 - 10:15 | Kei Kotake, NAOJ Tokyo
|
2D and 3D modeling of core-collapse
supernova explosion
|
| 10:15 - 10:45 | COFFEE BREAK |
| 10:45 - 11:10 | Raphael Hix, ORNL
|
CHIMERA models for core-collapse supernovae
|
| 11:10 - 11:35 | Matthias Liebendörfer, Univ. Basel
|
Approximantions for 3D supernova models
|
| 11:35 - 12:00 | Bernhard Müller, MPA
|
A new multi-dimensional GR neutrino
hydrodynamics code for CCSNe
|
| 12:00 - 15:00 | LUNCH BREAK |
| 15:00 - 15:25 | Jeremiah Murphy, Univ. Washington
|
A model for GW emission from CCSN explosions
|
| 15:25 - 15:50 | Martin Obergaulinger, MPA
|
Hydromagnetic instabilities in SNe
|
| 15:50 - 16:15 | Ewald Müller, MPA
|
3D simulations of mixing in supernova envelopes
|
| 16:15 - 16:45 | COFFEE BREAK |
| 16:45 - 17:10 | Bruce Fryxell, Univ. Michigan
|
Supernova Rayleigh-Taylor Instabilities
|
| 17:10 - 17:35 | Matthias Herzog, MPA
|
Burning of a neutron star to a strange star
|
| 17:35 - 18:00 | Friedel Thielemann, Univ. Basel
|
Explosive nucleosynthesis in core
collapse supernovae: The Fe-group and beyond
|
| 18:30 | BAVARIAN NIGHT |
| Time | Speaker | Title |
|---|
| 09:00 - 09:25 | Sergei Blinnikov, ITEP Moscow
|
New applications of SN II to cosmology
|
| 09:25 - 09:50 | Michele Marta, FZ Dresden
|
Experimental study of 14N (p, gamma)
O15 reaction
|
| 09:50 - 10:15 | Gabriel Martinez-Pinedo, GSI
|
Nuclear physics and r-process nucleosynthesis
|
| 10:15 - 10:45 | COFFEE BREAK |
| 10:45 - 11:10 | Almudena Arcones, GSI
|
Core-collapse supernovae,
neutrino-driven wind and nucleosynthesis
|
| 11:10 - 11:35 | Shinya Wanajo, TUM
|
The r-process in black hole winds
|
| 11:35 - 12:00 | Yuhri Ishimaru, ICU
|
Galactic chemical evolution and origin
of r-process elements
|
| 12:00 - 12:25 | Nobuya Nishimaru, NAOJ Tokyo
|
r-process nucleosynthesis in
magnetically dominated core
collapse supernovae
|
| 12:00 - 15:00 | LUNCH BREAK |
| 15:00 - 15:25 | Claudia Travaglio, AO Turino
|
p-process nucleosnthesis in SNe Ia
|
| 15:25 - 15:50 | Joachim Görres, Univ. Indiana Notre Dame
|
Neutron sources for the s-process
|
| 15:50 - 16:15 | Urs Frischknecht, Univ. Basel
|
Light element destruction and s process
in massive stars with rotation
|
| 16:15 - 16:45 | COFFEE BREAK |
| 16:45 - 17:10 | Joachim Görres, Univ. Indiana Notre Dame
|
On the C12+C12 reaction rate
|
| 17:10 - 17:35 | Roland Diehl, MPE
|
Gamma ray spectroscopy and nucleosynthesis
|
| 17:35 - 18:00 | Dieter Hartmann, Clemson Univ.
|
Cosmic chemical evolution: What to
expect from GRB observations
|
| 18:00 - 18:15 | Organizers |
Concluding remarks
|
| 18:30 | DINNER |