Venue
The workshop was held at Ringberg Castle, 50 km south of Munich. It offers full-board accommodation and an inspiring atmosphere for intense communication, particularly fruitful for workshops.
Show on a map Castle's websiteThe systematic observational hunt for electromagnetic transients has revealed a growing diversity of supernova types and explosion-related phenomena. Progenitor searches have succeeded in identifying an increasing number of supernova progenitors and progenitor candidates, beginning to bridge the gap between massive star evolution and final stellar deaths as single stars and in binaries. Multi-wavelength studies of supernova remnants have collected an amazing wealth of precious data about the hydrodynamic and nucleosynthetic fingerprints left by the blast wave of the explosion. The computational modeling of supernovae and of the latest stages of progenitor evolution has become feasible in three spatial dimensions, and our theoretical picture of the neutrino-driven mechanism and of its consequences is on the way to mature.
While the progress in each area is remarkable, the accelerating inflow of observational data has posed more new riddles not only for the rare outliers of the stellar death events, than it was able to solve. Tying the many loose ends together will require the close(r) interaction of modelers and observers of progenitor stars, supernovae, and supernova remnants. Only then it will be possible to draw the right conclusions and to find answers for some of the most nagging astrophysical questions, for example:
This workshop was intended to foster the interaction of the mentioned communities and follows up a similar, productive meeting at Chicheley Hall in June 2016.
The workshop was held at Ringberg Castle, 50 km south of Munich. It offers full-board accommodation and an inspiring atmosphere for intense communication, particularly fruitful for workshops.
Show on a map Castle's websiteThis workshop was sponsored by the European Research Council under Advanced Grant AdG No. 341157-COCO2CASA.
Website ERC Project COCO2CASALast updated: 2017-07-25
Monday, July 24 | ||
12:30 - 14:00 | Lunch | |
14:00 - 14:10 | Hans-Thomas Janka (MPA) | Welcome Address |
14:10 - 14:35 | Justyn Maund (University of Sheffield) | Resolved stellar populations as probes of the progenitors of supernovae |
14:35 - 15:00 | Schuyler Van Dyk (Caltech/IPAC) | The Direct Identification of Core-Collapse SN Progenitors |
15:00 - 15:25 | Emma Beasor (Liverpool John Moores University) | The evolution of RSG to SN |
15:25 - 15:50 | Jorick Vink (Armagh Observatory and Planetarium) | SN Progenitor identification from mass loss |
15:50 - 16:20 | Coffee break | |
16:20 - 16:45 | Matteo Cantiello (Center for Computational Astrophysics, Flatiron Institute) | Local and Global Radiation Hydrodynamics Simulations of Massive Star Envelopes |
16:45 - 17:10 | Alexander Heger (Monash Centre for Astrophysics) | The seeds of supermassive black holes |
17:10 - 17:35 | Philipp Podsiadlowski (University of Oxford) | Neutron-Star and Black-Hole Kicks |
17:35 - 18:00 | Ryosuke Hirai (Waseda University) | The binary companion to the progenitor of iPTF13bvn |
18:00 - 18:25 | Manos Zapartas (University of Amsterdam) | Predicting the Presence of Companions for Stripped-Envelope Core-Collapse Supernovae: The Case of the Broad-Lined Type IC SN 2002AP |
18:30 | Dinner | |
Tuesday, July 25 | ||
09:00 - 09:25 | Paul Crowther (University of Sheffield) | On the spatial distribution of massive stars in star-forming galaxies and inferences for progenitors of ccSNe |
09:25 - 09:50 | Fabian Schneider (University of Oxford) | Influence of binary mass-transfer on pre-supernova stellar structures |
09:50 - 10:15 | Ben Davies (Liverpool John Moores University) | The Red Supergiant Problem, and a reappraisal of the masses of II-P progenitors |
10:15 - 10:40 | Jacob Jencson (California Institute of Technology) | Hunting for the missing supernovae with SPIRITS |
10:40 - 11:10 | Coffee break | |
11:10 - 11:35 | Ken'ichi Nomoto (Kavli IPMU, University of Tokyo) | Electron capture supernovae from super AGB stars |
11:35 - 12:00 | Christopher Kochanek (Ohio State University) | The LBT Survey for Failed Supernovae and its First Candidate |
12:00 - 12:25 | Ko Nakamura (Fukuoka University) | Systematic features of core-collapse supernova based on multi-D simulations |
12:30 - 14:30 | Lunch | |
14:30 - 14:55 | Robert Bollig (MPA) | Muon Creation in Supernova Matter Facilitates Neutrino-driven Explosions |
14:55 - 15:20 | Jerome Guilet (CEA Saclay) | How to form a millisecond magnetar? Magnetic field amplification in a protoneutron star |
15:20 - 15:45 | Martin Obergaulinger (University of Valencia) | Core collapse with rotation and magnetic fields: explosions, black holes, magnetars |
15:45 - 16:10 | Thierry Foglizzo (CEA Saclay) | The impact of modest stellar rotation on the asymmetric explosion of massive stars |
16:10 - 16:40 | Coffee break | |
16:40 - 17:05 | Tomoya Takiwaki (National Astronomical Observatory of Japan) | Rotation aided neutrino driven-explosions |
17:05 - 17:30 | Remi Kazeroni (MPA) | The development of neutrino-driven convection in core-collapse supernovae: 2D vs 3D |
17:30 - 17:55 | Quintin Mabanta (Florida State University) | Effects of Turbulence on the Critical Conditions of Explosion |
17:55 - 18:20 | Jeremiah Murphy (Florida State University) | A Unifying Explosion Condition for Core-collapse Supernova |
18:30 | Dinner | |
Wednesday, July 26 | ||
09:00 - 09:25 | Kei Kotake (Fukuoka University) | Correlation and Directionality of Multimessenger Signals in 3D Core-Collapse Supernova Models |
09:25 - 09:50 | Haakon Andresen (MPA) | How does moderate progenitor rotation affect the gravitational wave signal from core-collapse supernovae? |
09:50 - 10:15 | Kosuke Sumiyoshi (Numazu College of Technology) | 2D/3D Core-collapse supernovae explored by 6D Boltzmann neutrino transport |
10:15 - 10:40 | Oliver Just (RIKEN) | Supernova simulations with the ALCAR code |
10:40 - 11:10 | Coffee break | |
11:10 - 11:35 | Akira Harada (University of Tokyo) | The Rotating Core-Collapse Supernova Simulation with Full Boltzmann Neutrino Transport |
11:35 - 12:00 | Bernhard Müller (Queen's University Belfast / Monash University) | Core-Collapse Supernova Simulations from 3D Progenitor Models |
12:00 - 12:25 | William Raphael Hix (Oak Ridge National Laboratory) | Lessons on the Nucleosynthesis from Multi-dimensional Supernova models |
12:30 - 14:00 | Lunch | |
14:00 - 14:25 | Dan Patnaude (Smithsonian Astrophysical Observatory) | Connecting Supernova Remnants to Their Explosions and Progenitors |
14:25 - 14:50 | Ping Zhou (University of Amsterdam) | Spatially resolved study of supernova remnant W49B: on its supernova properties and explosion mechanism |
14:50 - 15:15 | Iair Arcavi (University of California, Santa Barbara) | The Impossible Supernova |
15:15 - 15:40 | Elena Sorokina (Lomonosov Moscow State University) | Bumpy Light Curves of Supernovae as Indicators of the Interaction with CSM |
15:40 - 16:05 | Coffee break | |
16:05 - 16:30 | Sergei I. Blinnikov (ITEP, Moscow) | Central Engines and Environment of Superluminous Supernovae |
16:30 - 16:55 | Shing-Chi Leung (Kavli IPMU, University of Tokyo) | Effects of rotation and metallicity on the pre-collapse evolution of Pulsation Pair-Instability Supernovae |
16:55 - 17:20 | Alexey Tolstov (Kavli IPMU, University of Tokyo) | Superluminous supernova models: from X-ray to near-infrared photometry |
17:20 - 17:45 | Josefin Larsson (KTH Royal Institute of Technology, Stockholm) | Blackbody components in the early afterglows of gamma-ray bursts: new insight into the progenitors |
17:45 | Castle tour | |
18:30 | Dinner | |
Thursday, July 27 | ||
09:00 - 09:25 | Annop Wongwathanarat (RIKEN) | Long-time three-dimensional core-collapse supernova simulations |
09:25 - 09:50 | Claudia Travaglio (INAF - Astrophysical Observatory Turin) | Multi-d core collapse supernovae nucleosynthesis to forge connections to the chemical enrichment of the cosmos |
09:50 - 10:15 | Jason Spyromilio (ESO) | Supernova 1987A at 30 |
10:15 - 10:40 | Victor Utrobin (ITEP, Moscow) | Mixing constraints on the progenitor of supernova 1987A |
10:40 - 11:10 | Coffee break | |
11:10 - 11:35 | Claes Fransson (Stockholm University, Oskar Klein Centre) | The ejecta and circumstellar interaction of SN 1987A |
11:35 - 12:00 | Athira Menon (Monash University) | Binary mergers and blue supergiants: progenitors of SN 1987A and other peculiar Type-II supernovae |
12:00 - 12:25 | Lars Bildsten (KITP, University of California, Santa Barbara) | Core Collapse Supernovae Light Curves that Incorporate Rayleigh-Taylor Mixing with MESA |
12:30 - 14:30 | Lunch | |
14:30 - 14:55 | Roland Diehl (MPE) | Gamma ray lines from young SNR |
14:55 - 15:20 | Christoph Weinberger (MPE) | Kinematic constraints of SNe by Ti-44 gamma ray measurements |
15:20 - 15:45 | Anatoly Iyudin (Lomonosov Moscow State University) | What are chances for Cas A being produced by the binary system? |
15:45 - 16:15 | Coffee break | |
16:15 - 18:30 | Honoring session for Ewald Müller's retirement | |
16:15 - 16:55 | Friedrich Thielemann (University of Basel) | Supernovae, Magnetic Fields and a few Basel Attempts to Copy Ewald Müller's Activities |
16:55 - 17:10 | Jose Maria Ibanez (University of Valencia) | The Garching-Valencia collaboration: a personal touch |
17:10 - 17:50 | Miguel-Angel Aloy (University of Valencia) | Are relativistic jets the birth cryings of supernova remnants? |
17:50 - 18:30 | Harald Dimmelmeier | Ewald meets Einstein: A story of general relativistic core collapse, happy PhD research years and a few lessons for life |
18:30 | Dinner (Bavarian Night) | |
Friday, July 28 | ||
09:00 - 09:25 | Michael Gabler (MPA) | From a Supernova towards its remnant with 3D simulations |
09:25 - 09:50 | Gilles Ferrand (RIKEN) | 3D simulations of young supernova remnants |
09:50 - 10:15 | Salvatore Orlando (INAF - Osservatorio Astronomico di Palermo) | Connecting Supernova Remnants to their progenitor SN explosions: the Cassiopeia A laboratory |
10:15 - 10:40 | Satoru Katsuda (Chuo University) | Explosion asymmetries anti-correlating with neutron-star kicks in young supernova remnants |
10:40 - 11:10 | Coffee break | |
11:10 - 11:35 | Maria Arias de Saavedra Benitez (University of Amsterdam) | Cassiopeia A at LOFAR frequencies |
11:35 - 12:00 | Frederic Vogt (ESO) | The multi-faceted MUSE view of 1E 0102.2-7219 |
12:00 - 12:25 | Wolfgang Kerzendorf (ESO) | The surviving companion of Cassiopeia A |
12:30 - 14:30 | Lunch | |
14:30 - 18:30 | Free afternoon (self-organized excursion) | |
18:30 | Dinner |