PHAROS PhD Training School: Superfluidity and transport for multimessenger physics of compact stars

PHAROS PhD Training School: Superfluidity and transport for multimessenger physics of compact stars

PHAROs PhD Training School

Superfluidity and transport for multimessenger physics of compact stars, 
February 23-29, 2020
Karpacz, Poland 

School website: click here

Understanding the multimessenger physics of neutron stars requires a good knowledge not only the equation of state of their interiors but in addition an array of quantities and phenomena associated with the transport in their interiors and effects of superfluidity. These include: 

1. The oscillation spectrum of neutron stars, their damping, and emission of gravitational waves, that can be potentially observed in the near future.

2. The phenomena of glitches and their relaxations and other dynamical transient phenomena in rotational behavior of pulsars and accreting neutron stars.

3. Long-term cooling of neutron stars, the short-term thermal evolution in accreting systems, and the post-merger phase of neutron star coalescence.

4. Magnetic field evolution of isolated neutron stars and neutron star binaries, the dissipative MHD description of short-time-scale phenomena such as neutron star mergers.

These and related topics will be addressed from the perspective of understanding of transport and superfluidity in various contexts related to neutron stars. 


Lecturers:  

  • Mark Alford (Phys. Dept., Washington University St. Louis, USA)  "Dissipation and transport in neutron stars and mergers" 
  • Danai Antonopoulou (Nikolaus Copernicus Astronomical Centre, Warsaw, Poland) "Superfluid signatures in neutron star rotation"   
  • Aurel Bulgac (Phys. Dept., Washington State U., USA) "Density functional approach to superfluid systems"
  • Nicolas Chamel (Universite Libre de Bruxelles, Belgium) "Probing nuclear superfluidity with neutron stars"
  • Eckhard Krotscheck (Johannes Kepler University Linz, Austria and SUNY, Buffalo, USA)   "Many-body computations of pairing in neutron matter, EoS of nuclear matter from Correlated Basis Functions" 
  • Cristina Manuel (Instituto de Ciencias del Espacio (IEEC-CSIC) of Barcelona, Spain)  "Relativistic chiral kinetic theory, transport methods in quantum field theories"             
  • Adriana R. Raduta (Horia Hulubei National Institute, Bucharest, Romania)   "Thermal evolution of neutron stars and the role of their superfluidity"                                                                      

Organizers:

Armen Sedrakian  (Uni. Wroclaw, Poland and FIAS, Germany, Chair)
David Blaschke (Uni. Wroclaw, Poland and JINR, Russia)
Tobias Fischer (Uni. Wroclaw, Poland)
Ian Jones (Uni. Southampton, UK)
Bryn Haskell (CAMK, Poland)
Constanca Providencia (Uni. Coimbra, Portugal)