Event Schedule

IReNA-INT Joint Workshop on Thermal and Magnetic Evolution of Neutron Stars

Week 1

Monday, December 9, 2024

Start Time Presentation Title Presenter Presenter Organization Format Location Slides
New views on thermonuclear bursts Duncan Galloway Monash University In-person C421 PDF
TBA Hendrik Schatz Michigan State University In-person C421
Break
Spectral Features Observed during Thermonuclear X-ray Bursts from 4U 1820-30 Gaurava Kumar Jaisawal Technical University of Denmark In-person C421
Thermal evolution of accreting neutron stars at high accretion rates Martín Javier Nava Callejas Universidad Nacional Autónoma de México In-person C421 PDF
Constraining Accreted Neutron Star Crust Shallow Heating with the Inferred Depth of Carbon Ignition in X-ray Superbursts Zachary Meisel Air Force Institute of Technology In-person C421 PDF
Lunch
Discussion and short talks In-person C423

Tuesday, December 10, 2024

Start Time Presentation Title Presenter Presenter Organization Format Location Slides
Leak in or leak out in accreting neutron stars ? Dany Page Universidad Nacional Autónoma de México In-person C421
Neutron Star Cooling and the Composition of Dense Matter Andrew Steiner University of Tennessee, Knoxville and Oak Ridge National Laboratory In-person C421
Break
Layers of electron captures in the crust of accreting neutron stars Lami Suleiman California State University, Fullerton Virtual C421 PDF
Short-range correlations and Urca process in neutron stars Armen Sedrakian Frankfurt Institute for Advanced Studies and University of Wrocław In-person C421 PDF
Cooling of rapidly rotating neutron stars in 2D Mikhail Beznogov National Institute for Physics and Nuclear Engineering In-person C421 PDF
Lunch
Cooling, masses and emulators Sudhanva Lalit Michigan State University In-person C423 PDF
Relevance of the Kohn-Luttinger effect for superfluidity in neutron stars Mia Kumamoto University of Washington, Institute for Nuclear Theory Virtual C423 PDF

Wednesday, December 11, 2024

Start Time Presentation Title Presenter Presenter Organization Format Location Slides
Recent developments in the modelling of neutron-star crusts Nicolas Chamel Université Libre de Bruxelles In-person C421 PDF
Shallow heating of accreting neutron stars Edward Brown Michigan State University In-person C421
Break
Thermal evolution of KS 1731-260 Rahul Jain Lawrence Livermore National Laboratory In-person C421
Constraining twin stars with cold neutron star cooling data Melissa Mendes Technische Universität Darmstadt Virtual C421 PDF
Providing crustal parameters for the NS cooling simulations Nikolai Shchechilin Université Libre de Bruxelles In-person C421 PDF
Lunch
Superfluid fraction in the inner crust Michael Urban IJCLab, Université Paris-Saclay In-person C423 PDF
Crust breaking and the limiting rotation rate of neutron stars Chuck Horowitz Indiana University Virtual C423 PDF

Thursday, December 12, 2024

Start Time Presentation Title Presenter Presenter Organization Format Location Slides
Origin and Dynamics of Magnetar Magnetic Fields: Insights from 3D Magneto-Thermal Simulations Clara Dehman University of Alicante In-person C421 PDF
Effects of superfluidity-superconductivity and Landau quantization on neutron star magneto-thermal evolution Peter Rau Columbia University In-person C421 PDF
Break
A new 3D code for MAgneto-Thermal evolution in Isolated Neutron Stars (MATINS): thermal evolution and light curves Stefano Ascenzi Gran Sasso Science Institute In-person C421 PDF
Modelling Magnetar Outbursts as Short-Term Crustal Cooling Events Davide De Grandis Institute of Space Sciences In-person C421 PDF
Operator representation of magnetic field evolution in neutron star cores Dmitry Ofengeim Hebrew University of Jerusalem In-person C421 PDF
Lunch
Thermal evolution of neutron stars and alternative theories of gravity Martín Javier Nava Callejas Universidad Nacional Autónoma de México In-person C423 PDF

Friday, December 13, 2024

Start Time Presentation Title Presenter Format Location
Panel 1: Neutron star surface phenomena Multiple In-person C421
Break
Panel 2: Crust phenomena Multiple In-person C421
Lunch
Panel 3: Core phenomena Multiple In-person C423