Event Schedule
Nuclear Physics in Mergers - Going Beyond the Equation of State
All time info is in Pacific Time (UTC -7); please convert accordingly.
Please check the schedule regularly, as it is subject to change.
This workshop takes place between weeks 1 and 2 of the separate 25-2b program.
Note: By attending a workshop talk, participants agree to abide by the INT Code of Conduct
Week 1
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location | Slides |
|---|---|---|---|---|---|---|
| Welcome to the workshop! | The Organizers | In-person | C520 | |||
| Dense matter inference: promises and challenges with next-generation observations | Jocelyn Read | California State University Fullerton | Virtual | C520 | ||
| COFFEE | ||||||
| Connecting observations of the cold EoS to dynamical astrophysics | Isaac Legred | University of Illinois Urbana-Champaign | In-person | C520 | ||
| The crack, the whisk and the spark: Neutron star mergers beyond the dense matter equation state | Elias Most | Caltech | In-person | C520 | ||
| LUNCH BREAK | ||||||
| Turbulence modeling - A game we have no choice but to play ... | Nils Andersson | University of Southampton UK | In-person | C520 | ||
| Inferring the nuclear equation of state from binary merger simulations | Kenta Kiuchi | Max Planck Institute for Gravitational Physics | In-person | C520 | ||
| COFFEE | ||||||
| Discussion | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location | Slides |
|---|---|---|---|---|---|---|
| Transport in Neutron Star Mergers | Alexander Haber | University of Southampton UK | In-person | C520 | ||
| Bulk Viscosity of Two-Flavor Color Superconducting Quark Matter in Neutron Star Mergers | Arus Harutyunyan | Byurakan Astrophysical Observatory, Yerevan State University | Virtual | C520 | ||
| COFFEE | ||||||
| Towards a self-consistent description of 𝜐 interactions in mergers: challenges and achievements | Zidu Lin | University of Tennessee Knoxville | In-person | C520 | ||
| Bulk Viscous Dissipation in Neutron Star Megers: Effect of Magnetic field | Pranjal Tambe | Inter-University Centre for Astronomy and Astrophysics | In-person | C520 | ||
| LUNCH BREAK | ||||||
| Dependence of the bulk viscosity of neutron star matter on the nuclear symmetry energy | Yumu Yang | University of Illinois Urbana-Champaign | In-person | C520 | ||
| Neutrino dynamics in neutron star mergers | Liam Brodie | Washington University in St. Louis | In-person | C520 | ||
| COFFEE | ||||||
| Discussion | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location | Slides |
|---|---|---|---|---|---|---|
| How do we connect the dense matter EOS to heavy-ion data? | Jaki Noronha-Hostler | University of Illinois Urbana Champaign | In-person | C520 | ||
| COFFEE | ||||||
| Heavy-Ion Collisions and the QCD Phase Diagram | Jamie Karthein | Massachusetts Institute of Technology | Virtual | C520 | ||
| T-matrix approach to quark-gluon plasma at finite baryon density | Konstantin Maslov | University of Houston | In-person | C520 | ||
| LUNCH BREAK | ||||||
| UHECRs from Binary Neutron Star mergers | Glennys Farrar | New York University | In-person | C520 | ||
| Geometric radius measurement during mergers: leveraging low-density nuclear physics through dynamical resonance to constrain the core | David Tsang | University of Bath | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location | Slides |
|---|---|---|---|---|---|---|
| Enhancements to Neutrino Opacities in Hot Magnetized Matter | Mia Kumamoto | Ohio University / N3AS | In-person | C520 | ||
| The neutron lifetime anomaly, dark baryons, and their impact on neutron star mergers | Steven Harris | Iowa State University | In-person | C520 | ||
| COFFEE | ||||||
| Multi-Messenger Probes of Dark Matter With Neutron Stars and Binary Neutron Star Mergers | Violetta Sagun | University of Southampton UK | In-person | C520 | ||
| LUNCH BREAK | ||||||
| Pi in the Sky: Neutron stars with exceptionally light QCD axions | Masha Baryakhtar | University of Washington | In-person | C520 | ||
| Probing QCD axions with neutron stars: cooling and oscillations | Antonio Gómez-Bañón | Universidad de Alicante | In-person | C520 | ||
| COFFEE | ||||||
| Discussion | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location | Slides |
|---|---|---|---|---|---|---|
| Searching for quark matter in neutron stars: challenges and prospects | Sophia Han | T.D. Lee Institute / SJTU | In-person | C520 | ||
| COFFEE | ||||||
| Correlations between the Neutron Star Mass–Radius Relation and the Equation of State | Boyang Sun | Stony Brook University | In-person | C520 | ||
| EoS with Quarkyonic Matter | Marlene Nahrgang | Subatech | In-person | C520 |