| Name | Institute
| Title of talk |
|---|
| | | |
| Arcones, Almudena | GSI, Darmstadt, D |
Core-collapse supernovae, neutrino-driven wind and nucleosynthesis |
| | | |
| Bisnovatyi-Kogan, G.S. | IKI, Moscow, RUS |
Activity of the non-equilibrium layer in the neutron star crust |
| | | |
| Blinnikov, Sergei | ITEP, Moscow, RUS |
New applications of SN II to cosmology |
| | | |
| Ciaraldi-Schoolmann, Franco | MPA |
Turbulence in delayed detonation models in Type I a Supernovae
simulations |
| | | |
| Diehl, Roland | MPE |
Gamma ray spectroscopy and nucleosynthesis (to be refined) |
| | | |
| Edelmann, Philipp | MPA | Thermonuclear
reaction fronts in white dwarfs |
| | | |
| Fernandez, Rodrigo | IAS, Princeton, USA |
Progress on the SASI |
| | | |
| Fink, Michael | MPA | Detonation in WD stars |
| | | |
| Fransson, Claes | Oskar Klein Centre, Stockholm, S
| Modeling and observations of the ejecta and ring of
SN 1987A at very late stages |
| | | |
| Frischknecht, Urs | Univ. Basel, CH |
Light element destruction and s process in massive stars with
rotation |
| | | |
| Fryxell, Bruce | Univ. of Michigan, USA |
Supernova Rayleigh-Taylor Instabilities |
| | | |
| Görres, Joachim | Univ. of Notre Dame, USA |
Neutron sources for the s-process |
| | | |
| Hachinger, Stephan | MPA |
How much helium is hidden in SNe Ic? |
| | | |
| Hartmann, Dieter | Clemson University, USA |
Cosmic chemical evolution: What to expect from GRB observations |
| | | |
| Hempel, Matthias | Univ. Heidelberg, D |
Statistical model for a complete supernovae equation of state |
| | | |
| Herzog, Matthias | MPA |
Burning of a neutron star to a strange star |
| | | |
| Hillebrandt, Wolfgang | MPA |
Type Ia Supernovae: the beauties and the beasts |
| | | |
| Hix, William Raphael | Oak Ridge Natl. Lab., USA |
CHIMERA models for core-collapse supernovae |
| | | |
| Isern, Jordi | IEEC, Catalunya, E |
Axions and the cooling of white dwarfs |
| | | |
| Ishimaru, Yuhri | Int. Christian Univ., Japan |
Galactic chemical evolution and origin of r-process elements |
| | | |
| Iyudin, Anatoli | Moscow State Univ., RUS |
Observational evidence of a hypernova in our Galaxy |
| | | |
| Janka, H.-Thomas | MPA |
t.b.d. |
| | | |
| Käppeli, Roger | Univ. Basel, CH |
No talk |
| | | |
| Kotake, Kei | NAOJ, Tokyo, Japan |
2D and 3D modeling of core-collapse supernova explosion |
| | | |
| Kratz, Karl-Ludwig | MPI f. Chemie, Mainz, D |
Co-production of p-, s- and r-process isotopes in the HEW scenario |
| | | |
| Kromer, Markus | MPA |
Radiative transfer in SNe Ia - Predicting observables for explosion
models |
| | | |
| Leibundgut, Bruno | ESO |
t.b.d. |
| | | |
| Liebendörfer, Matthias | Univ. Basel, CH |
t.b.d. |
| | | |
| Marta, Michele | FZD, Dresden, D |
Experimental study of 14N (p, gamma) O15 reaction |
| | | |
| Martínez Pinedo, Gabriel | GSI, Darmstadt, D |
Nuclear physics and r-process nucleosynthesis |
| | | |
| Miczek, Fabian | MPA |
Stability of shear flows in stellar interiors |
| | | |
| Mocak, Miroslav | IAA, Bruxelles, B |
Hydrodynamic simulations of core convection in stars |
| | | |
| Müller, Bernhard | MPA | A new
multi-dimensional GR neutrino hydrodynamics code for CCSNe
|
| | | |
| Müller, Ewald | MPA |
3D simulations of mixing in supernova envelopes |
| | | |
| Murphy, Jeremiah | Univ. of Washington, USA |
(1) Conditions for successful CCSN explosions (2) A model for GW
emission from CCSN explosions |
| | | |
| Nadyozhin, Dmitrij | ITEP, Moscow, RUS |
Non-equilibrium neutronization and the electron neutrino flash for
gravitational collapse of stellar core (with A.V. Yudin) |
| | | |
| Nishimura, Nobuya | NAOJ, Tokyo, Japan |
R-process nucleosynthesis in magnetically dominated core collapse
supernovae |
| | | |
| Obergaulinger, Martin | MPA |
Hydromagnetic instabilities in SNe |
| | | |
| Pakmor, Rüdiger | MPA | Double white dwarfs
mergers as progenitors of SNe Ia |
| | | |
| Perego, Albino | Univ. Basel, CH |
Neutrino physics and neutrino transport in core collapse supernova |
| | | |
| Röpke, Friedrich | MPA | SN Ia models |
| | | |
| Ruiter, Ashley | MPA | Progenitors of SNe Ia and
Accretion Induced Collapse |
| | | |
| Sagert, Irina | Goethe Univ., Frankfurt, D |
Equation of state for explosive astrophysical systems, including a
quark matter phase transition: Compatibility with heavy ion and pulsar
data is considered. |
| | | |
| Sauer, Daniel | Stockholm Univ., S |
Alternatively powered supernovae |
| | | |
| Schaffner-Bielich, Jürgen | Univ.
Heidelberg, D | No talk |
| | | |
| Schmidt, Wolfram | Univ. Göttingen, D |
Intermittency and DDTs in SNe Ia |
| | | |
| Seitenzahl, Ivo | MPA |
Internal conversion electrons and SN light curves |
| | | |
| Shen, Ken | UCSB, USA |
Helium shell detonations from AM CV_N systems: New results on SNE IA |
| | | |
| Sim, Stuart | MPA |
Testing Type Ia Supernova explosion models: SN 2003 GS as a test case |
| | | |
| Thielemann, Friedel | Univ. Basel, CH |
Explosive nucleosynthesis in core collapse supernovae: The Fe-group
and beyond |
| | | |
| Travaglio, Claudia | Astron. Obs. Turin, Italy |
p-process nucleosnthesis in SN Ia |
| | | |
| Utrobin, Victor | ITEP Moscow, RUS |
Progenitors of type IIp supernovae |
| | | |
| Wanajo, Shinya | Excellence Cluster Universe TUM/MPA |
The r-process in black hole winds |
| | | |
| Weiss, Achim | MPA | No talk |
| | | |