Holographic model for neutron star with color superconductivity in the inner core

Not scheduled
20m
Blokhintsev hall (4th floor) (BLTP)

Blokhintsev hall (4th floor)

BLTP

Speaker

Mr Nguyen Hoang Vu (BLTP-JINR)

Description

In this project, we use the Einstein Gauss Bonnet gravity for this holographic model. The crust contains baryon phase correspond the instanton gas in AdS soliton solution and the core color supeconductivity (CSC) phase correspond to the AdS black hole. We use this model to compute the equation of state of this type of compact star

Author

Mr Nguyen Hoang Vu (BLTP-JINR)

Presentation materials

There are no materials yet.