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 1
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location | Slides |
|---|---|---|---|---|---|---|
| Welcome | Sanjay Reddy | Institute for Nuclear Theory | In-person | C520 | PDF, PDF | |
| From Low to High Densities: an Application of Bayesian Model Mixing to the Dense Matter EOS | Christian Drischler | Institute of Nuclear and Particle Physics | In-person | C520 | ||
| First-order nucleon-to-quark phase transition: Thermodynamically-consistent constructions other than Maxwell and Gibbs | Constantinos Constantinou | INFN-TIFPA | In-person | C520 | ||
| Coffee Break | In-person | |||||
| Characterizing the nuclear models informed by PREX and CREX | Tianqi Zhao | UC Berkeley | In-person | C520 | ||
| Nuclear Matter Equation of State from In-Medium Similarity Renormalization Group | Kang Yu | Facility for Rare Isotope Beams, Michigan State University | In-person | C520 | ||
| Lunch + Unstructured Time | ||||||
| Panel: Ab-Initio Methods & Phase Transitions | Ingo Tews (Moderator) | Los Alamos National Laboratory | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location | Slides |
|---|---|---|---|---|---|---|
| Which phase transitions are possible in neutron stars? | Jan-Erik Christian | Universität Hamburg | In-person | C520 | ||
| Deconfinement transition at high isospin chemical potential | Srimoyee Sen | Iowa State University | In-person | C520 | ||
| Coffee Break | In-person | |||||
| MREX: The Mainz Radius EXperiment | Concettina Sfienti | Johannes Gutenberg University | In-person | C520 | ||
| You cannot extract neutron-skin thickness from coherent π0 photoproduction off nuclei | Pierre Capel | Johannes Gutenberg-Universität Mainz | In-person | C520 | ||
| Lunch + Unstructured Time | ||||||
| Panel: Neutron Skins | Betty Tsang (Moderator) | Michigan State University | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location | Slides | Links |
|---|---|---|---|---|---|---|---|
| Heavy-ion collision measurements in early FRIB and a look towards FRIB400 | Kyle Brown | Michigan State University | In-person | C520 | PPT | ||
| Non-monotonic specific entropy along first-order phase transition | Maneesha Sushama Pradeep | University of Maryland at College Park | In-person | C520 | |||
| Coffee Break | In-person | ||||||
| Terrestrial Messengers for Nuclear Equation of State | Betty Tsang | Michigan State University | In-person | C520 | PPT | ||
| Self-consistent T-matrix approach to strongly interacting QGP at finite baryon density | Konstantin Maslov | University of Houston | In-person | C520 | PPT | ||
| Lunch + Unstructured Time | |||||||
| Panel: Collider Experiments & QGP | Concettina Sfienti | Johannes Gutenberg University | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location | Slides |
|---|---|---|---|---|---|---|
| Correlations and Semi-Universal Analytic Inversion of the TOV Equation | Jim Lattimer | Stony Brook University | In-person | C520 | ||
| Effect of increasingly accurate mass and radius measurements on predictions for nuclear and neutron star crust properties | William Newton | Texas A&M University-Commerce | In-person | C520 | ||
| Unified equations of state for neutron stars | Nicolas Chamel | Institute of Astronomy and Astrophysics | In-person | C520 | ||
| Coffee Break | In-person | |||||
| Constraining the dense matter equation of state with new NICER mass-radius measurements and new chiral effective field theory inputs | Melissa Mendes | Institut für Kernphysik | In-person | C520 | ||
| Gravitational Wave frequencies and the nuclear EOS in Core-Collapse Supernovae | Carla Frohlich | NC State University | In-person | C520 | ||
| Lunch + Unstructured Time | ||||||
| Panel: Neutron Stars | Christian Drischler (Moderator) | Ohio University | In-person | C520 |
| Start Time | Presentation Title | Presenter | Presenter Organization | Format | Location | Slides |
|---|---|---|---|---|---|---|
| Measuring nuclear physics with Cosmic Explorer | Duncan Brown | Syracuse University | In-person | C520 | ||
| Joint Inference of cosmology and neutron star equation of state from dark binary neutron stars | Sukanta Bose | Washington State University | In-person | C520 | ||
| Inferring chiral three-nucleon forces from third-generation gravitational-wave detectors | Rahul Somasundaram | Syracuse University | In-person | C520 | ||
| Coffee Break | In-person | |||||
| Symmetry energy and its effect on structure and composition of the neutron stars: implications to model inference | Arunava Mukherjee | Saha Institute of Nuclear Physics | In-person | C520 | ||
| Simultaneously Constraining the Neutron Star Equation of State and Mass Distribution through Multimessenger Observations and Nuclear Benchmarks | Bhaskar Biswas | Hamburg Observatory | In-person | C520 | ||
| Lunch + Unstructured Time | ||||||
| Panel: Multimessenger EOS Inference with Binary Neutron Stars | Philippe Landry (Moderator) | University of Toronto | In-person | C520 |