Event Schedule

Neutron Rich Matter on Heaven and Earth

Please note: By attending a program talk, participants agree to abide by the INT Code of Conduct.

Week 1

Monday, June 26, 2023

Start Time Presentation Title Presenter Presenter Organization Location Slides
Introduction Sanjay Reddy, Director Institute for Nuclear Theory
Equation of state of dense matter Nicholas Chamel Institute of Astronomy and Astrophysics C520 PDF
Break
How to leverage observables sensitive to crust physics … William Newton Texas A&M University-Commerce C520 PDF
Break
Constraining the low-density neutron star equation of state from heavy-ion collisions Helena Pais University of Salamanca C520 PDF
Break
Equations of state for hot neutron stars Adriana R. Raduta IFIN-HH C520 PDF
Lunch
Constraints on heavy-element production from LIGO-Virgo-KAGRA observations Hsin-Yu Chen The University of Texas at Austin C520 PDF
Break
Fast neutrino cooling in the accreting neutron star MXB 1659-29 Farrukh Fattoyev Manhattan College C520 PDF
Break
Dorado simulations Bas Dorsman University of Amsterdam C520 PDF
Probing exotic matter in neutron star cores with g-mode oscillations Sophia Han T.D. Lee Institute/SJTU C520 PDF

Tuesday, June 27, 2023

Start Time Presentation Title Presenter Presenter Organization Location Slides
The PREX and CREX experiments and the equation of state Charles Horowitz Indiana University C520 PDF
Break
Neutron skins and neutron stars, nuclear equation of state Brendan Reed Indiana University C520 PDF
Break
Constraining nuclear models with recent data on neutron radii of 208Pb and 48Ca Tianqi Zhao Ohio University C520 PDF
Break C520
Bayesian Refinement of RMF Models Marc Salinas Florida State University C520 PDF
Lunch
Inferring phase transitions from nonparametric equations of state Isaac Legred Caltech C520 PDF
Break
WaveformUncertainty Jocelyn Read California State University Fullerton C520 PDF
Break
Constraining the neutron star equation of state from gravitational wave detections Rahul Somasundaram LANL and Syracuse University C520 PDF
Discussion/Gravitational-Waves tutorials C520

Wednesday, June 28, 2023

Start Time Presentation Title Presenter Presenter Organization Format Location Slides Links
First-order hadron-to-quark phase transitions in neutron stars Constantinos Constantinou INFN-TIFPA Virtual C520 PDF
Break
Dark matter Admixed Neutron Stars Shafayat Shawqi University of Alberta C520 PDF
Break
Trace anomaly as a measure of conformality related to the EoS Yuki Fujimoto Institute for Nuclear Theory C520 PDF
Break
Multimessenger Resonant Shattering Flares … David Tsang University of Bath C520 PDF
Lunch
Introduction to Pulse Profile Modeling Bas Dorsman University of Amsterdam C520 PDF
Break
Challenges in NICER Pulse Profile Modeling analyses Serena Vinciguerra Anton Pannekoek Institute (University of Amsterdam) C520 PDF
Break
NICER analysis of PSR J0437-4715 using X-PSI Devarshi Choudhury Anton Pannekoek Institute for Astronomy C520 PDF
Discussion/Pulse-Profile tutorials C520

Thursday, June 29, 2023

Start Time Presentation Title Presenter Presenter Organization Location Slides
Kilohertz QPOs in short gamma-ray bursts: A hypermassive neutron star origin? Elias Most Princeton University C520 PDF
Break
How do the assumptions on the neutron star atmosphere affect the neutron star parameter constraints with NICER Tuomo Salmi University of Amsterdam C520 PDF
Break
Pulse Profile Modeling of Thermonuclear Burst Oscillations Sources Yves Kini API C520 PDF
Break
TBA C520
Lunch
Effect of rotation on neutron star mass and radius determination Sharon Morsink University of Alberta C520 PDF
Break
Constraining fundamental physics parameters with Mass radius measurements of NS Chun Huang Washington University in St. Louis C520 PDF
Break
TBA C520
Caltech seminar C520

Friday, June 30, 2023

Start Time Presentation Title Presenter Presenter Organization Format Location Slides
Neutron skin of 208Pb from ultra-relativistic heavy-ion collisions Giuliano Giacalone Universität Heidelberg Virtual C520 PDF
Break
Ab-initio calculations of proton scattering in the context of neutron skin Alexis Mercenne Louisiana State University C520 PDF
Break
Neutron star equation of state inference with Machine Learning Jessica Irwin University of Glasgow C520 PDF
Break
Bayesian Model Mixing analysis of the empirical saturation point Christian Drischler Institute of Nuclear and Particle Physics C520 PDF
Lunch
Future Instruments and Experiments. Additional: INT-XG Anna Watts, Jocelyn Read, Jorge Piekarewicz C520 PDF, PDF, PDF