activity
20132022
most citedPhysical Environment of Accreting Neutron Stars

5 citations · 11 across the 7 of their papers we have counts for

collaborators

7 papers

gr-qc2022

Gravitational Casimir Effect in Inspiralling Neutron Star Binary

Jing Wang

Currently, the discussions and investigations for the vacuum energy is drawing great both theoretical and experimental attention. The vacuum states of variety of fields, subject to…

gr-qc2021

Inspiraling Corrugation-Induced Quantum Effects on Neutron Star Binary Plane

Jing Wang

We use the path-integral formula and investigate some dynamical quantum effects induced by the inspiraling lateral corrugation of orbital plane in gravitationally bound neutron sta…

astro-ph.HE2019★ 5 cited

Physical Environment of Accreting Neutron Stars

Jing Wang

Neutron stars (NSs) powered by accretion, which are known as accretion-powered NSs, always locate in binary systems and manifest themselves as X-ray sources. Physical process durin…

astro-ph.HE2019★ 3 cited

Massive scalar counterpart of gravitational waves in scalarized neutron star binaries

Jing Wang

In analogy with spontaneous magnetization of ferromagnets below the Curie temperature, a neutron star (NS), with a compactness above a certain critical value, may undergo spontaneo…

astro-ph.HE2016★ 1 cited

Graviton mass generation in in-spiraling DNS

Jing Wang

We point out that a spontaneous scalarized inspiring double neutron star (DNS) system can provide us a natural laboratory to investigate the generation mechanism of masses for grav…

astro-ph.HE2016★ 2 cited

Gravitational Higgs mechanism in inspiraling scalarized NS-WD binary

Jing Wang

We investigate the gravitational Higgs mechanism in the inspiraling scalarized neutron star - white dwarf (NS-WD) binaries, whose dynamics are described by the scalar-tensor theory…

astro-ph.HE2013

Neutron star high mass binaries as the origin of SGR/AXP

Jing Wang, Hsiang-Kuang Chang

A close high-mass binary system consisting of a neutron star (NS) and a massive OB supergiant companion is expected to lead to a TZO structure, which consists of a NS core and a st…