Neutron stars as laboratory for dense matter

Friday, March 2, 14:30hs - Seminar room

Speaker: Laura Tolos (ICE/UAB)

 

Abstract:

Neutron stars are an excellent laboratory for testing matter under extreme conditions. In particular, a lot of emphasis has been invested in understanding the interior of neutron stars and the equation of state of the different possible phases since its direct consequences for the mass-radius relationship of neutron stars as well as cooling processes.

I will review some results for nucleonic, kaonic and hyperonic matter together with superfluidity and their consequences for cooling processes. I will comment on possible constraints not only from neutron stars observations but also from back-to-Earth experiments, such as heavy-ion collisions. I will finally outline future prospects to be tested in neutron stars laborator

 

Utilitzem cookies pròpies i de tercers per a millorar els nostres serveis mitjançant l’anàlisi dels seus hàbits de navegació. Si continua navegant, considerem que n’accepta el seu ús. Pot canviar la configuració o obtenir més informació a la nostra "política de Cookies".

Accepto les cookies d'aquest lloc.