18th Workshop on Nuclear Astrophysics, March 14 - 19, 2016

Program


Monday, March 14

Time Speaker Title
14:45 - 15:00Organizers Welcome and introductory comments
15:00 - 15:30 Raphael Hirschi, Keele Univ.
SHYNE project: 12321D for convective boundary mixing
15:30 - 16:00 Paul Woodward, University of Minnesota
3-D hydrodynamic simulations of a low-Z AGB helium shell flash with hydrogen ingestion
16:00 - 16:20 Philipp Edelmann, HITS Heidelberg
Dynamical shear instabilities in massive stars
16:20 - 16:50 COFFEE BREAK
16:50 - 17:20 Sebastian Ohlmann, HITS Heidelberg
Simulations of common envelope phases in binary stellar evolution
17:20 - 17:40 Samuel Jones, HITS Heidelberg
Evolution of stars in the Bermuda Triangle mass range (between 8 and 12 solar masses)
17:40 - 18:00 Achim Weiss, MPA
The tip of the giant branch and the importance of nuclear physics
18:00 - 18:20 Francesca Primas, ESO
Sodium abundances in GCs - constraining the nature of the polluters
18:30 DINNER


Tuesday, March 15

Time Speaker Title
9:00 - 9:30 Falk Herwig, University of Victoria, Canada
Simulations and observations of the i-process nucleosynthesis in multiple stellar sites
9:30 - 9:50 Aldo Serenelli, ICE/CSIC-IEEC, Bellaterra
Solar models and neutrinos
9:50 - 10:20 Rene Reifarth, Goethe University Frankfurt
Nuclear astrophysics in ion storage rings
10:20 - 10:50 COFFEE BREAK
10:50 - 11:10 Joachim Görres, University of Notre Dame
22Ne(alpha,n) revisited
11:10 - 11:30 Kathrin Göbel, Goethe University Frankfurt
Neutron captures beyond standard s-process temperatures
11:30 - 12:00 Thomas Rauscher, University of Basel
Theory uncertainties in modeling nucleosynthesis beyond Fe
12:00 - 12:20 Rodrigo Fernandez, UC Berkeley
Outflows from NS merger remnant disks: EM emission and nucleosynthesis
12:30 - 15:00 LUNCH BREAK
15:00 - 15:30 Meng-Ru Wu, TU Darmstadt
Nucleosynthesis in ejecta of compact binary mergers
15:30 - 16:00 Oliver Just, MPA
Can neutrinos launch jets of short GRBs
16:00 - 16:20 Alexandra Kozyreva, Keele Univ.
Fast evolving pair-instability supernovae
16:20 - 16:50 COFFEE BREAK
16:50 - 17:20 Thomas Siegert, MPE
Positron annihilation in the Milky Way
17:20 - 17:50 Shigehiro Nagataki, RIKEN Japan
Astrophysical big bangs: from SNe to SNRs
18:30 DINNER


Wednesday, March 16

Time Speaker Title
9:00 - 9:20 Bruno Leibundgut, ESO
The distance to the type IIP supernova SN2013eq
9:20 - 9:50 Yudai Suwa, MPA
From supernovae to neutron stars
9:50 - 10:20 Bernhard Müller, Queen's Univ. Belfast
A simple approach to the supernova progenitor-explosion connection
10:20 - 10:50 COFFEE BREAK
10:50 - 11:20 Thierry Foglizzo, CEA Saclay
The impact of asymmetric instabilities during the collapse of a rotating stellar core
11:20 - 11:50 Akira Harada, University of Tokyo
Systematic study of the acoustic mechanism for core-collapse supernovae
11:50 - 12:20 Remi Kazeroni, CES Saclay
The development of neutrino-driven convection in core-collapse supernovae: 2D vs 3D
12:30 LUNCH
13:30 - 18:30 FREE AFTERNOON
18:30 DINNER


Thursday, March 17

Time Speaker Title
9:00 - 9:30 Thomas Ertl, MPA
Core-collapse supernovae across the stellar mass range
9:30 - 10:00 Tobias Melson, MPA
Exploring the explosion mechanism of core-collapse supernovae in three dimensions
10:00 - 10:30 Evan O'Connor, North Caroline State Univ.
Two dimensional core-collapse supernova explosions aided by general relativity with multidimensional neutrino transport
10:30 - 11:00 COFFEE BREAK
11:00 - 11:30 Alexander Summa, MPA
Progenitor-dependent explosion dynamics in self-consistent, axisymmetric simulations of neutrino-driven core-collapse supernovae
11:30 - 12:00 Annop Wongwathanarat, RIKEN Japan
Long-time simulations of CCSNe and development of a new hydrodynamics code for astrophysical simulations
12:00 - 12:20 Dimitry Badjin, ITEP Moscow
Generation of high-energy gamma-rays in magnetar powered supernovae, their heating efficiency and observational signatures
12:30 - 15:00 LUNCH BREAK
15:00 - 15:30 Sergei Blinnikov, ITEP Moscow
Paths to superluminous supernovae
15:30 - 16:00 Mike Zingale, Stony Brook University
Models of convection in X-ray bursts and pre-SNe Ia white dwarfs
16:00 - 16:20 Semyon Glazyrin, ITEP Moscow
Spontaneous deflagration to detonation transition in supernovae Ia
16:20 - 16:50 COFFEE BREAK
16:50 - 17:20 Alan Calder, Stony Brook Univ.
Systematic effects on the brightness of Type Ia supernovae
17:20 - 17:40 Aron Michel, HITS Heidelberg
Gravitational settling of 22Ne in sub-Chandrasekhar models of Type Ia supernovae
17:40 - 18:00 Rüdiger Pakmor, HITS Heidelberg
SNe Ia from WD mergers
18:00 - 18:20 Ulrich Nöbauer, MPA
SNe Ia within dense C/O envelopes
18:30 BAVARIAN NIGHT


Friday, March 18

Time Speaker Title
9:00 - 9:30 Roland Diehl, MPE
Gamma-ray lines from SN2014J
9:30 - 9:50 Markus Kromer, Stockholm Univ.
Type Ia supernovae @ 3 micron
9:50 - 10:20 Stuart Sim, Queen's Univ. Belfast
Probing the geometry of thermonuclear supernovae with spectropolarimetry
10:20 - 10:50 COFFEE BREAK
10:50 - 11:10 Suhail Dhawan, ESO
A reddening-free estimate of the 56Ni mass of Type Ia supernovae
11:10 - 11:30 Luke Shingles, Queen's Univ. Belfast
Nebular-phase radiative transfer in Type Ia supernovae
11:30 - 11:50 Andreas Flörs, ESO
Nebular phase of SN Ia
11:50 - 12:10 Christian Vogl, MPA
Distances to type IIP supernovae by means of spectral fitting
12:10 - 12:30 Friedrich Thielemann, University of Basel
Simulating multiple X-ray bursts with the aim for superbursts
12:30 - 15:00 LUNCH BREAK
15:00 - 15:30 Victor Utrobin, ITEP Moscow
Light curve analysis of type IIP supernovae using neutrino-driven explosion simulations
15:30 - 16:00 Almudena Arcones, TU Darmstadt
Nucleosynthesis in supernovae and neutron star mergers
16:00 - 16:30 COFFEE BREAK
16:30 - 17:00 Shin-ichiro Fujimoto, Nat. Inst. Technology, Japan
Nucleosynthesis in core collapse supernovae based on 2D hydrodynamic simulations
17:00 - 17:30 Veronika Schaffenroth, Univ. Innsbruck
Observation of the runaway HD271791: nucleosynthesis in a core-collapse supernova
17:30 - 18:00 Anatoly Iyudin, Moscow State Univ.
The spatial distribution of 44Ti and other elements in Cas A and other SNRs known to be the result of a core-collapse
18:00 - 18:10 Concluding remarks
18:30 DINNER