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The physics of strongly interacting matter: neutron stars, cold atomic gases and related systems

22–26 Apr 2024
ECT*
Europe/Rome timezone

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The workshop will bring together experts from nuclear physics, astrophysics, and cold atomic gases to develop an improved understanding of the physics of strongly interacting matter, with a particular focus on neutron stars. The workshop will focus on the following main goals:

* To survey observational data on neutron star masses, radii, tidal deformability and moment of inertia, and to understand all aspects in the modeling processes needed to extract these.
 
* To improve our understanding of matter with low proton concentrations encountered in neutron stars at around nuclear density.
 
* To determine whether or not phases with non-spherical nuclei (pasta phases) are stable.
 
* To understand the dynamics of pasta phases in neutron stars and supersolid phases in cold Fermi gases.
 
* To better pin down the equation of state at supranuclear densities.
 
* To understand the physical origin of the maximum in the sound velocity at high densities deduced from observations of neutron stars.
 
* To explore constraints on the properties of dense matter from nuclear experiments in the laboratory.
 
* To explore possible cold gas experiments that could illuminate unresolved issues
 

INVITED SPEAKERS

Andreas Bauswein, GSI Darmstadt
Silas Beane, University of Washington

Nicolas Chamel, Brussels U

Maria Colonna, Catania

Christoph Eigen, Cambridge

Roland Farrell, University of Washington

Yuki Fujimoto, University of Washington

Maciej Galka, Heidelberg U

Sebastien Guillot, Toulouse

Charles Horowitz, Indiana U

Elinor Kath, Heidelberg U

Michael Kramer, Bonn

Elena Poli, Innsbruck
Jocelyn Read, California State U
Thomas Schaefer, NC State
Dam Son, Chicago
Sandro Stringari, U Trento
Wolfram Weise, TU Munich

Starts
Ends
Europe/Rome
ECT*
Aula Renzo Leonardi
Strada delle Tabarelle 286, I-38123 Villazzano (Trento)
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Information for participants here

 

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