output
20032026
most citedThe equation of state in (2+1)-flavor QCD

1.2k citations

Showing 2021 · astro-ph.HEShow all

10 papers · 2 filters

astro-ph.HE2021★ 12 cited

GECAM detection of a bright type-I X-ray burst from 4U 0614+09: confirmation its spin frequency at 413 Hz

Y. P. Chen, J. Li, S. L. Xiong +87

One month after launching Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM), a bright thermonuclear X-ray burst from 4U~0614+09, was observed on Ja…

astro-ph.HE2021★ 10 cited

Modelling the correlated keV/TeV light curves of Be/gamma-ray binaries

A. M. Chen, J. Takata

Be/-ray binaries comprise a confirmed or presumptive pulsar orbiting a Be star and emit luminous -rays. Non-thermal emissions are thought to arise from synchrotron radiation…

astro-ph.HE2021★ 75 cited

Implications of NICER for neutron star matter: the QHC21 equation of state

Toru Kojo, Gordon Baym, Tetsuo Hatsuda

The recent NICER measurement of the radius of the neutron star PSR J0740+6620, and the inferred small variation of radii from 1.4 to 2.1, reveal key features of t…

astro-ph.HE2021★ 3 cited

A powerful e^{+-} outflow driven by a proto-strange quark star

Shao-Ze Li, Yun-Wei Yu, He Gao +2

An electron-positron layer can cover the surface of a bare strange star (SS), the electric field in which can excite the vacuum and drive a pair wind by taking away the heat of the…

astro-ph.HE2021★ 17 cited

Kilonova and Optical Afterglow from Binary Neutron Star Mergers. II. Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers

Jin-Ping Zhu, Shichao Wu, Yuan-Pei Yang +8

In the second work of this series, we explore the optimal search strategy for serendipitous and gravitational-wave-triggered target-of-opportunity (ToO) observations of kilonovae a…

astro-ph.HE2021★ 1 cited

Does a long-lived remnant neutron star exist after short gamma-ray burst GRB 160821B?

Guang-Lei Wu, Yun-Wei Yu, Jin-Ping Zhu

Mergers of double neutron stars (DNSs) could lead to the formation of a long-lived massive remnant NS, which has been previously suggested to explain the AT 2017gfo kilonova emissi…