Event Schedule
EOS Measurements with Next-Generation Gravitational-Wave Detectors
All time info is in Pacific Time (UTC -7); please convert accordingly. This is an in-person program.
Talks will take place in room C520.
Please note: By attending a program talk, participants agree to abide by the INT Code of Conduct.
Week 2
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location |
|---|---|---|---|---|---|
| Quantifying the likelihood of quark-matter cores in massive neutron stars | Aleksi Vuorinen | University of Helsinki | Virtual | C520 | |
| Listening to the long ringdown: a novel way to pinpoint the equation of state in neutron-star cores | Tyler Gorda | Goethe University | In-person | C520 | |
| Improving Nuclear Physics Input for next-generation gravitational-wave detectors | Ingo Tews | Los Alamos National Laboratory | In-person | C520 | |
| Coffee Break | In-person | ||||
| Universal properties of equations of state of dense nuclear matter and mass-radius curves of neutron stars | Dmitry Ofengeim | Hebrew University of Jerusalem | In-person | C520 | |
| Trace Anomaly in Dense Matter with Strong Phase Transitions | José Carlos Jiménez Apaza | Brazilian Center for Research in Physics (CBPF) | In-person | C520 | |
| Lunch + Unstructured Time | |||||
| Panel: Neutron Star Cores | Jim Lattimer (Moderator) | Stony Brook University | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location |
|---|---|---|---|---|---|
| Breaking a degeneracy between the effects of dark matter and strongly interacting matter at high densities with the next-generation gravitational-wave detectors | Violetta Sagun | University of Coimbra | In-person | C520 | |
| The impact of dark matter on BNS tidal signatures with next generation GW detectors | Hauke Koehn | Institut for Physics and Astronomy | In-person | C520 | |
| Constraining cold dense nuclear equation of state using gravitational wave and electromagnetic observations of coalescence of neutron star binaries | Shaon Ghosh | Montclair State University | Virtual | C520 | |
| Coffee Break | In-person | ||||
| Characterizing Neutron Stars With Cosmic Explorer and Einstein Telescope: Prospects and Challenges | Bangalore S. Sathyaprakash | Penn State University | Virtual | C520 | |
| Constraining the microscopic dynamics of nuclear matter with multimessenger astrophysical Data | Omar Benhar | INFN | In-person | C520 | |
| Lunch + Unstructured Time | |||||
| Panel: Dark Matter in Neutron Stars | Tianqi Zhao (Moderator) | UC Berkeley | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location |
|---|---|---|---|---|---|
| Bayesian inference of dense matter EOS: non-relativistic vs relativistic mean field models at zero and finite temperatures | Mikhail Beznogov | National Institute for R&D in Physics and Nuclear Engineering (IFIN-HH) | In-person | C520 | |
| Thermal Effects in Binary Neutron Star Mergers | Jacob Fields | The Pennsylvania State University | In-person | C520 | |
| Weak Interactions in Neutron Star Mergers | Alex Haber | Washington University in St Louis | In-person | C520 | |
| Coffee Break | In-person | ||||
| Bulk viscosity in neutron star merger remnants from neutron decays to dark baryons | Steven Harris | Indiana University | In-person | C520 | |
| Dissipative effects in matter and metric perturbations: a formal analysis | David Diaz-Guerra | University of Salamanca | Virtual | C520 | |
| Lunch + Unstructured Time | |||||
| Panel: Finite-Temperature & Out-of-Equilibrium Effects in Neutron Star Mergers | Constantinos Constantinou (Moderator) | INFN-TIFPA | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location |
|---|---|---|---|---|---|
| Challenges of measuring the Neutron Star Equation of State using GW observations | Hung Tan | Syracuse University | In-person | C520 | |
| Signature of hadron-quark crossover in binary neutron star mergers | Yuki Fujimoto | Institute for Nuclear Theory | In-person | C520 | |
| Coffee Break | In-person | ||||
| Detecting hypermassive neutron stars with short gamma-ray bursts | Cecilia Chirenti | University of Maryland | In-person | C520 | |
| Estimating the neutron-star radius and constraining the mass-radius relation with short gamma-ray bursts | Victor Guedes | University of Virginia | In-person | C520 | |
| Lunch + Unstructured Time | |||||
| Panel: Proto-Neutron Stars & Postmerger Remnants | Sukanta Bose (Moderator) | Washington State University | In-person | C520 |
| Start Time | Presentation Title | Format | Location |
|---|---|---|---|
| Contributed Talks | In-person | C520 | |
| Coffee Break | In-person | ||
| Contributed Talks | In-person | C520 | |
| Lunch | |||
| Open Discussion: EOS measurements in the era of next-generationa gravitational-wave detectors | In-person | C520 | |
| Closing Remarks | In-person | C520 | |
| Unstructured Time | In-person | C520 |