Event Schedule
The r-process and the nuclear EOS after LIGO-Virgo's third observing run
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All workshop talks will take place in C520. All time info. is in Pacific Daylight Time (UTC -7); please convert accordingly. Please note: By attending a program talk, participants agree to abide by the INT Code of Conduct |
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Week 1
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Slides |
|---|---|---|---|---|---|
| Director's Welcome | Sanjay Reddy | Institute for Nuclear Theory | In-person | ||
| EOS from combined theory, experiment, and observations | Jeremy Holt | Texas A&M | Virtual | ||
| Neutron star mergers with the Lagrangian Numerical Relativity code SPHINCS_BSSN. | Stephan Rosswog | Stockholm University | Virtual | ||
| Numerical relativity simulations and gravitational wave modeling | Sebastiano Bernuzzi | Jena FSU | Virtual | ||
| BREAK | |||||
| Constraints on the EOS and nuclear symmetry energy from experiments and observations. | James Lattimer | Stony Brook University | In-person | ||
| LUNCH | |||||
| Neutrino processes in hot and dense matter | Sanjay Reddy | Institute for Nuclear Theory | In-person | ||
| Bulk viscosity in neutron star mergers | Elias Most | Princeton University | Virtual | ||
| New techniques in numerical relativity | Zachariah Etienne | University of Idaho | Virtual | ||
| BREAK | |||||
| Uncertainty Quantification and the Equation of State of Hot and Dense Matter | Andrew Steiner | UT Knoxville, Oak Ridge National Laboratory | In-person |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Slides |
|---|---|---|---|---|---|
| Nonparametric astrophysical inference of the nuclear equation of state and connections to nuclear experiment and theory | Reed Essick | Perimeter Institute for Theoretical Physics | In-person | ||
| Confronting neutron star equation of state to present observational data | Jerome Margueron | Institut de physique des 2 infinis de Lyon | Virtual | ||
| New EOS developments for neutron star matter and for finite temperature | Achim Schwenk | TU Darmstadt | Virtual | ||
| BREAK | |||||
| Post-merger GW emission in BNS mergers and empirical relations for GW asteroseismology | Nikolaos Stergioulas | Aristotle University of Thessaloniki | Virtual | ||
| The relevance of muons production and neutrino trapping in Binary Neutron Star mergers | Eleonora Loffredo | Gran Sasso Science Institute | In-person | ||
| BREAK | |||||
| Gravitational wave signals from quark matter with realistic phase transition | Yuki Fujimoto | Institute for Nuclear Theory | In-person | ||
| Gravitational-wave signatures of high-density matter and the maximum mass of neutron stars | Phillipe Landry | Canadian Institute for Theoretical Astrophysics | In-person | ||
| Multimessenger parameter and population inference | Richard O'Shaughnessy | Rochester Institute of Technology | Virtual | ||
| BREAK | |||||
| DISCUSSION (featuring short talk from Shunke Ai, UNLV) |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Slides |
|---|---|---|---|---|---|
| Neutrinos and nucleosynthesis in neutron star mergers | Gail McLaughlin | North Carolina State University | Virtual | ||
| Numerical simulation for binary neutron star merger, properties of the ejecta, nucleosynthesis | Sho Fujibayashi | Max Planck Institute for Gravitational Physics | Virtual | ||
| Neutrino absorption and neutrino fast flavor oscillations in neutrino-cooled black-hole accretion disks formed as remnants of NS-NS and NS-BH mergers | Oliver Just | GSI Heavy Ion Research Centre | Virtual | ||
| BREAK | |||||
| Finite-temperature effects in neutron star mergers | Carolyn Raithel | Institute for Advanced Study | In-person | ||
| LUNCH | |||||
| The latest developments of nuclear theory related to the r-process | Matthew Mumpower | Los Alamos National Laboratory | Virtual | ||
| Magnetic fields in GRMHD simulations of BNS mergers | Pedro Espino | University of California Berkeley | In-person | ||
| Neutrino fast flavour conversion in Neutron Star post merger disks | Xinyu Li | Perimeter Institute for Theoretical Physics | Virtual | ||
| BREAK | |||||
| Nuclear Equation of State from Astro and Terrestrial Measurements | Betty Tsang | Michigan State University | In-person |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Slides |
|---|---|---|---|---|---|
| R-process nucleosynthesis in neutron-star mergers and other explosive events | Daniel Siegel | Perimeter Institute for Theoretical Physics | In-person | ||
| Long term 3-dimensional magnetohydrodynamic simulations of outflows from black hole accretion disks formed in neutron star mergers | Steven Fahlman | University of Alberta | In-person | ||
| Impact of asymmetric fermionic and bosonic dark matter on neutron star properties | Violetta Sagun | University of Coimbra | Virtual | ||
| BREAK | |||||
| Neutrino driven winds from proto neutron stars | Dhruv Desai | Columbia University | In-person | ||
| Neutrino-Cooled Accretion Disks using HARM3D+NUC | Ariadna Murguia Berthier | Northwestern University | Virtual | ||
| LUNCH | |||||
| Resolving the fastest ejecta from binary neutron star mergers: Implications for electromagnetic counterparts | Coleman Dean | University of Alberta | In-person | ||
| Electromagnetic observations of neutron star mergers to constrain the nuclear equation of state | Ryan Foley | University of California Santa Cruz | Virtual | ||
| BREAK | |||||
| Neutrino flavor conversion impact on r-process nucleosynthesis from mergers | Meng-Ru Wu | Academia Sinica | Virtual | ||
| Signatures of primordial black hole and neutron star interactions | Volodymyr Takhistov | Kavli IPMU, University of Tokyo | Virtual |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Slides |
|---|---|---|---|---|---|
| The galactic chemical evolution of the Magellanic Clouds Reveal the r-process Enrichment Timescale | Kevin Schlaufman | Johns Hopkins University | In-person | ||
| Kilonova r-process models: nuclear physics and atomic opacities. | Gabriel Martinez-Pinedo | GSI Darmstadt, TU Darmstadt | Virtual | ||
| Kilonovae from radiative transfer simulations of neutron star mergers | Mattia Bulla | Stockholm University | Virtual | ||
| BREAK | |||||
| The inferred r-process abundance pattern from the GW170817 kilonova | John Ruan | Bishop's University | In-person | ||
| LUNCH | |||||
| Optical and infrared constraints on the ejecta mass and abundances in kilonovae | Charlie Kilpatrick | Northwestern University | In-person | ||
| Observational constraints on r-process production from collapsars | Shreya Anand | California Institute of Technology | In-person | ||
| BREAK | |||||
| What we learned about the amount of r-process elements produced from binary mergers from LIGO-Virgo's observations | Hsin-Yu Chen | Massachusetts Institute of Technology | In-person | ||
| r-process in GW objects, collapsars and neutron star mergers, and Galactic chemical evolution | Toshitaka Kajino | Beihang University, NAOJ, University of Tokyo | Virtual | ||
| CLOSING |