Speaker
Ms
Udita Shukla
(University of Wroclaw)
Description
Gravitational waves offer exciting opportunities to study bulk properties of dense matter and challenge theoretical models of dense equations of state (EoS). NJL-type models widely employed in the COMPOSE database for studying neutron stars have the known problem that the speed of sound fails to approach the conformal limit. We investigate how a dynamical chiral quark model, which implements non-local interactions among quarks resolves the issue. Additionally, the influence of diquark on the QCD phase diagram is also investigated.
Author
Ms
Udita Shukla
(University of Wroclaw)
Co-author
Prof.
Pok Man Lo
(University of Wroclaw)
