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October 14, 2024 to November 15, 2024
YITP
Asia/Tokyo timezone

The Effect of Isovector Scalar Meson on Neutron Star Matter Based on a Parity Doublet Model

Nov 7, 2024, 5:30 PM
30m
Panasonic Auditorium, Yukawa Hall (YITP)

Panasonic Auditorium, Yukawa Hall

YITP

4th week (Nuclear matter under extreme conditions) 1-day workshop (4th week)

Speaker

Yuk Kei Kong (Nagoya University)

Description

We study the effect of the isovector-scalar meson a0(980) on the properties of nuclear matter and the neutron star (NS) matter by constructing a parity doublet model with including the a0 meson based on the chiral SU(2)L×SU(2)R symmetry.
We also include the ω-ρ mixing contribution to adjust the slope parameter at the saturation.
We find that, when the chiral invariant mass of nucleon m0 is smaller than about 800\,MeV, the existence of a0(980) enlarges the symmetry energy by strengthening the repulsive ρ meson coupling. On the other hand, for large m0 where the Yukawa coupling of a0(980) to nucleon is small, the symmetry energy is reduced by the effect of ω-ρ mixing.
We then construct the equation of state (EoS) of a neutron star matter to obtain the mass-radius relation of NS.
We find that, in most choices of m0, the existence of a0(980) stiffens the EoS and makes the radius of NS larger.
We then constrain the chiral invariant mass of nucleon from the observational data of NS, and find that 580 MeVm0860 MeV for L0=57.7 MeV.

Primary author

Yuk Kei Kong (Nagoya University)

Co-authors

Prof. Masayasu Harada (Nagoya University) Dr Takuya Minamikawa (Nagoya University)

Presentation materials