Neutron Star Radius Measurements, and Prospects for Future Constraints on the Dense Matter Equation of State

• Robert Rutledge (McGill University)

Room: 4/3-006 - TH Conference Room

Measurements of neutron star masses and radii through X-ray spectral data

• Tolga Guver (Istanbul University)

Room: 4/3-006 - TH Conference Room

Direct atmosphere model fits of X-ray bursts: New neutron star radius constraints

• Joonas Nättilä (Tuorla Observatory & Nordita)

Room: 4/3-006 - TH Conference Room

Recent developments in the physics of neutron-star crusts

• Nicolas Chamel (Université Libre de Bruxelles)

Room: 4/3-006 - TH Conference Room

Cold QCD and Compact Stars: EOS, Cooling and Axions

• Armen Sedrakian (Frankfurt University)

Room: 4/3-006 - TH Conference Room

Discussion Room: 4/3-006 - TH Conference Room

Gravitational waves from binary neutron star systems: from the equation of state to the properties of the signal using general relativistic numerical simulations

• Roberto de Pietri (Parma University)

Room: 4/3-006 - TH Conference Room

New paths to probing the nuclear equation of state via multimessenger signals from compact binary mergers involving neutron stars

• Vasileios Paschalidis

Room: 4/3-006 - TH Conference Room

A new quark-hadron hybrid EOS for core-collapse supernovae and neutron star mergers

• Matthias Hempel (Basel University)

Room: 4/3-006 - TH Conference Room

Recent developments of nuclear interactions within chiral EFT and applications to nuclear matter and nuclei

• Kai Hebeler (TU Darmstadt)

Room: 4/3-006 - TH Conference Room

Nuclear matter at zero and finite temperatures based on chiral forces

• Arianna Carbone (TU Darmstadt)

Room: 4/3-006 - TH Conference Room

Transport phenomena inside superfluid neutron stars

• Laura Tolos (University of Groningen)

Room: 4/3-006 - TH Conference Room

Discussion Room: 4/3-006 - TH Conference Room

Nuclear EoS, Hyperons and Neutron Stars

• Wolfram Weise (TU Munich)

Room: 4/3-006 - TH Conference Room

High mass neutron stars with quark cores - constraints for the EoS

• David Blaschke (University of Wroclaw)

Room: 4/3-006 - TH Conference Room

Models of Hyper and Hybrid Stars

• Stefan Schramm

Room: 4/3-006 - TH Conference Room

The physics and astrophysics of merging neutron-star binaries

• Luciano Rezzolla (Goethe University Frankfurt)

Room: 4/3-006 - TH Conference Room I will argue that if black holes represent one the most fascinating implications of Einstein's theory of gravity, neutron stars in binary system are arguably its richest laboratory, where gravity blends with astrophysics and particle physics. I will discuss the rapid recent progress made in modelling these systems and show how the inspiral and merger of a binary system of neutron stars is more than a strong source of gravitational waves. Indeed, while the gravitational signal can provide tight constraints on the equation of state for matter at nuclear densities, the formation of a black-hole--torus system can explain much of the phenomenology of short gamma-ray bursts, while the the ejection of matter during the merger can shed light on the chemical enrichment of the universe. The physics and astrophysics of merging neutron-star binaries

Probing fundamental physics with universal relations for neutron stars

• Kent Yagi (Princeton University)

Room: 4/3-006 - TH Conference Room

Discussion Room: 4/3-006 - TH Conference Room

Beyond general relativity

• Konstantinos Kokkotas

Room: 4/3-006 - TH Conference Room

Neutron stars meet AdS/CFT

• Niko Jokela

Room: 4/3-006 - TH Conference Room

Critical magnetic fields in a superconductor coupled to a superfluid

• Andreas Schmitt (University of Southampton)

Room: 4/3-006 - TH Conference Room

Quark Matter in Neutron Stars

• Eduardo Fraga (Universidade Federal do Rio de Janeiro)

Room: 4/3-006 - TH Conference Room

Global properties of rotating neutron stars with QCD equations of state

• Tyler Gorda (University of Helsinki)

Room: 4/3-006 - TH Conference Room

The Hearty Shapes of Quark Stars

• Juergen Schaffner-Bielich (Frankfurt University)

Room: 4/3-006 - TH Conference Room

Discussion Room: 4/3-006 - TH Conference Room

Unveiling the compact star interior using dynamic properties

• Kai Schwenzer (Washington University)

Room: 4/3-006 - TH Conference Room

Gravitational waves from a BSM perspective

• Alfredo Leonardo Urbano (CERN)

Room: 4/3-006 - TH Conference Room

Outlook and Future

• James Lattimer

Room: 4/3-006 - TH Conference Room

Discussion Room: 4/3-006 - TH Conference Room