Properties of the high density strongly interacting matter and neutron stars

Nyomtatóbarát változatNyomtatóbarát változat
PhD típus: 
Fizikai Tudományok Doktori Iskola
Év: 
2022/2023/1
Témavezető: 
Név: 
Wolf György
Email cím: 
wolf.gyorgy@wigner.hu
Kutatóintézet/Tanszék: 
Wigner RCP/Theory Department
Beosztás: 
Head of the Theoretical Physics Department, Scientific advisor
Tudományos fokozat: 
Doctor of the Academy
Konzulens: 
Név: 
Komor Márton
Email cím: 
kormosmarton@gmail.com
Intézet: 
Institute of Physics
Beosztás: 
Research associate professor
Tudományos fokozat: 
PhD
Leírás: 

With the increasing number of precise observation of neutron stars and their collisions their understanding requires accurate determination of the equation of state of the high density strongly interacting matter. Furthermore, to understand the cooling and the rotational modes of neutron stars, we should calculate the transport properties of its matter at different densities. We would like to use effective field theory using loop expansion and/or functional renormalization group method to determine them.

During the PhD the candidate should derive the equation of state of the strongly interacting matter and determine the structure of neutron stars, and determine the viscosities and/or heat capacities its matter.

Elvárások: 

field theory, computational knowledge

Munkahely neve: 
Wigner RCP
Munkahely címe: 
1121 Konkoly-Thege 29-33