Speaker
Akihiro Iwanaka
(RCNP, Osaka U.)
Description
We derived equations of state for neutron stars using a bottom-up holographic QCD model. Our calculations include mass-radius relationships of neutron stars and the sound velocity in high-density QCD matter. We also obtained partial restoration of chiral symmetry in finite baryon density.
Author
Akihiro Iwanaka
(RCNP, Osaka U.)
Co-authors
Atsushi Hosaka
(RCNP, JAEA)
Daisuke Fujii
(JAEA)
Motoi Tachibana
(Saga University)
Tadakatsu Sakai
(Nagoya University, KMI)