activity
20042026
most citedSearching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I

1.2k citations · 1.8k across the 34 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

30 papers · 1 filter

astro-ph.HE2026

Pulsar glitches triggered by quakes when stress reaches a threshold

Zixuan Zhou, Ruipeng Lu, Weiyang Wang +2

The starquake model of pulsar glitches is revisited in light of accumulated observational data. A statistical comparison between the time-predictable and the magnitude-predictable…

astro-ph.HE2026

Pulsar anti-glitches: starquakes driven by magnetism?

Hanyuan Long, Ruipeng Lu, Weiyang Wang +4

In the conventional starquake model of pulsar glitches, it is usually assumed that such events arise from fault slip induced by the self-gravity of compact objects. This inevitably…

astro-ph.HE2023

EOS-dependent millihertz quasi-periodic oscillation in low-mass X-ray binary

Helei Liu, Yong Gao, Zhaosheng Li +4

We studied the frequency and critical mass accretion rate of millihertz quasi-periodic oscillations (mHz QPOs) using a one-zone X-ray burst model. The surface gravity is specified…

astro-ph.HE2023★ 9 cited

Continuous gravitational waves from trapped magnetar ejecta and the connection to glitches and antiglitches

Garvin Yim, Yong Gao, Yacheng Kang +2

Gravitational waves from isolated sources have eluded detection so far. The upper limit of long-lasting continuous gravitational wave emission can now probe physically-motivated mo…

astro-ph.HE2023★ 70 cited

A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism

Weiwei Zhu, Heng Xu, Dejiang Zhou +34

The megajansky radio burst, FRB 20200428, and other bright radio bursts detected from the Galactic source SGR J1935+2154 suggest that magnetars can make fast radio bursts (FRBs), b…

astro-ph.HE2023

Revise thermal winds of remnant neutron stars in gamma-ray bursts

Shuang Du, Tingting Lin, Shujin Hou +1

It seems that the wealth of information revealed by the multi-messenger observations of the binary neutron star (NS) merger event, GW170817/GRB 170817A/kilonova AT2017gfo, places i…

astro-ph.HE2023★ 3 cited

Pulsar discovery prospect of FASTA

Mengyao Xue, Weiwei Zhu, Xiangping Wu +2

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) has discovered more than 650 new pulsars, which account for 20% of our known Galactic pulsar population. In this pa…

astro-ph.HE2023★ 9 cited

High-altitude Magnetospheric Emissions from Two Pulsars

Mao Yuan, Weiwei Zhu, Michael Kramer +21

We discover three new weak pulse components in two known pulsars, one in PSR J0304+1932 and two in PSR J1518+4904. These components are emitted about half way between the main emis…

astro-ph.HE2023★ 1.2k cited

Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I

Heng Xu, Siyuan Chen, Yanjun Guo +24

Observing and timing a group of millisecond pulsars (MSPs) with high rotational stability enables the direct detection of gravitational waves (GWs). The GW signals can be identifie…

astro-ph.HE2023★ 14 cited

Radial and Non-Radial Oscillations of Inverted Hybrid Stars

Chen Zhang, Yudong Luo, Hong-bo Li +2

We study the radial and non-radial oscillations of Cross stars (CrSs), i.e., stars with a quark matter crust and a hadronic matter core in an inverted order compared to conventiona…

astro-ph.HE2023★ 2 cited

The precursor of GRB211211A: a tide-induced giant quake?

Enping Zhou, Yong Gao, Yurui Zhou +8

The equilibrium configuration of a solid strange star in the final inspiral phase with another compact object is generally discussed, and the starquake-related issue is revisited,…

astro-ph.HE2023★ 8 cited

Free Energy of Anisotropic Strangeon Stars

Shichuan Chen, Yong Gao, Enping Zhou +1

Can pulsar-like compact objects release further huge free energy besides the kinematic energy of rotation? This is actually relevant to the equation of state of cold supra-nuclear…

astro-ph.HE2023★ 14 cited

Rescaling strange-cluster stars and its implications on gravitational-wave echoes

Chen Zhang, Yong Gao, Cheng-Jun Xia +1

Solid states of strange-cluster matter called strangeon matter can form strangeon stars that are highly compact. We show that strangeon matter and strangeon stars can be recast int…

astro-ph.HE2023★ 39 cited

The FAST Galactic Plane Pulsar Snapshot Survey: II. Discovery of 76 Galactic rotating radio transients and their enigma

D. J. Zhou, J. L. Han, Jun Xu +15

We are carrying out the GPPS survey by using the FAST, the most sensitive systematic pulsar survey in the Galactic plane. In addition to about 500 pulsars already discovered throug…

astro-ph.HE2023★ 10 cited

Broadband X-ray timing and spectral characteristics of the accretion-powered millisecond X-ray pulsar MAXI J1816195

Zhaosheng Li, Lucien Kuiper, Mingyu Ge +11

We studied the broadband X-ray timing and spectral behaviors of the newly confirmed accreting millisecond X-ray pulsar MAXI J1816195 during its 2022 outburst. We used the data f…

astro-ph.HE2023★ 12 cited

Quakes of Compact Stars

Ruipeng Lu, Han Yue, Xiaoyu Lai +3

Glitches are commonly observed for pulsars, which are explained by various mechanisms. One hypothesis attributes the glitch effect to the instantaneous moment of inertia change of…

astro-ph.HE2022★ 30 cited

Polarisation of magnetospheric curvature radiation in repeating fast radio bursts

Wei-Yang Wang, Jin-Chen Jiang, Kejia Lee +2

Fast radio busts (FRBs) can exhibit a wide variety of polarisation properties, not only between sources but also from burst to burst for a same one. In this work, we revisit the po…

astro-ph.HE2022★ 58 cited

FAST observations of an extremely active episode of FRB 20201124A: III. Polarimetry

Jin-Chen Jiang, Wei-Yang Wang, Heng Xu +26

As the third paper in the multiple-part series, we report the statistical properties of radio bursts detected from the repeating fast radio burst (FRB) source FRB 20201124A with th…

astro-ph.HE2022★ 21 cited

An X-Ray-dim "Isolated'' Neutron Star in a Binary?

Jie Lin, Chunqian Li, Weiyang Wang +13

We report the discovery of a dark companion to 2MASS J15274848+3536572 with an orbital period of 6.14 hr. Combining the radial velocity from LAMOST observations and modelling of th…

astro-ph.HE2022★ 12 cited

The radio signal of PSR B0950+08 is detected over the whole pulse phase

Zhengli Wang, Jiguang Lu, Jinchen Jiang +4

Pulsars are the "lighthouses" in the universe. Periodic pulses with the duty-cycle ~10% are detected when the radio beam of the rotating pulsar sweeps across the telescope. In this…

astro-ph.HE2022

Radio pulsations from a neutron star within the gamma-ray binary LS I +61 303

Shan-Shan Weng, Lei Qian, Bo-Jun Wang +9

LS I +61 303 is one of the rare gamma-ray binaries, emitting most of their luminosity in photons with energies beyond 100 MeV. The 26.5 d orbital period is clearly…

astro-ph.HE2021★ 2 cited

Repeating Fast Radio Burst: Coherent Circular Polarization By Bunches

Wei-Yang Wang, Jin-Chen Jiang, Jiguang Lu +5

Fast radio bursts (FRBs) are millisecond-duration signals that are highly dispersed at distant galaxies. However, the physical origin of FRBs is still unknown. Coherent curvature e…

astro-ph.HE2021★ 6 cited

Investigating magnetically-induced distortions of neutron stars through gamma-ray burst X-ray plateaus

Tingting Lin, Shuang Du, Weihua Wang +2

Magnetic field may distort neutron stars (NSs), but its effect has not been robustly tested through gravitational-wave observation yet due to the absence of a fast rotating Galacti…

astro-ph.HE2020★ 85 cited

Re-detection and a Possible Time Variation of Soft X-ray Polarisation from the Crab

Hua Feng, Hong Li, Xiangyun Long +24

The Crab nebula is so far the only celestial object with a statistically significant detection in soft x-ray polarimetry, a window that has not been explored in astronomy since the…