activity
20092023
most citedConstraints on interquark interaction parameters with GW170817 in a binary strange star scenario

146 citations · 1.8k across the 51 of their papers we have counts for

collaborators
Showing 2018Show all

5 papers · 1 filter

nucl-th2018★ 20 cited

Quark mean-field model for nuclear matter with or without bag

Zhen-Yu Zhu, Ang Li, Jin-Niu Hu +1

We propose the new quark mean-field bag (QMFB) model by incorporating the bag confinement mechanism in the original quark mean-field model. Nuclear matter and neutron star properti…

nucl-th2018★ 16 cited

Nucleon radius effects on neutron stars in quark mean field model

Zhen-Yu Zhu, Ang Li

We study the effects of free space nucleon radius on nuclear matter and neutron stars within the framework of quark mean field model. The nucleon radius is treated self-consistentl…

astro-ph.HE2018★ 97 cited

The allowed parameter space of a long-lived neutron star as the merger remnant of GW170817

Shunke Ai, He Gao, Zi-Gao Dai +3

Limited by the sensitivities of the current gravitational wave (GW) detectors, the central remnant of the binary neutron star (NS) merger associated with GW170817 remains an open q…

nucl-th2018★ 99 cited

Neutron star equation of state from the quark level in the light of GW170817

Zhen-Yu Zhu, En-Ping Zhou, Ang Li

Matter state inside neutron stars is an exciting problem in astrophysics, nuclear physics and particle physics. The equation of state (EOS) of neutron stars plays a crucial role in…

astro-ph.HE2018★ 1 cited

Pulsar glitch and nuclear EoS: Applicability of superfluid model

A. Li, R. Wang

In this contribution, we have made use of the contemporary equation of states (EOSs) for the complete neutron star structure, and confronted them with one particular glitch constra…