activity
19952023
most citedX-Ray Flares from Postmerger Millisecond Pulsars

371 citations · 9.8k across the 240 of their papers we have counts for

collaborators
Showing 2011Show all

6 papers · 1 filter

astro-ph.CO2011★ 29 cited

Weak gravitational lensing effects on cosmological parameters and dark energy from gamma-ray bursts

F. Y. Wang, Z. G. Dai

Gamma-ray bursts (GRBs) are attractive objects for constraining the nature of dark energy in a way complementary to other cosmological probes, especially at high redshifts. However…

astro-ph.HE2011★ 34 cited

Nearby low-luminosity GRBs as the sources of ultra-high energy cosmic rays revisited

Ruo-Yu Liu, Xiang-Yu Wang, Zi-Gao Dai

Low-luminosity gamma-ray bursts (GRBs) with luminosity . 10^49erg/s probably consititute a distinct population from the classic high-luminosity GRBs. They are the most luminous obj…

astro-ph.HE2011★ 66 cited

Probing the tidal disruption flares of massive black holes with high-energy neutrinos

Xiang-Yu Wang, Ruo-Yu Liu, Zi-Gao Dai +1

The recently discovered high-energy transient Swift J164449.3+573451 (Sw J1644+57) is thought to arise from the tidal disruption of a passing star by a dormant massive black hole.…

astro-ph.HE2011★ 83 cited

The updated luminosity correlations of gamma-ray bursts and cosmological implications

F. Y. Wang, Shi Qi, Z. G. Dai

Several interesting luminosity correlations among gamma-ray burst (GRB) variables have been recently discussed extensively. In this paper, we derive the six luminosity correlations…

astro-ph.HE2011

Implications of Understanding Short Gamma-Ray Bursts Detected by {\it Swift}

Lang Shao, Zi-Gao Dai, Yi-Zhong Fan +3

In an effort to understand the puzzle of classifying gamma-ray bursts (GRBs), we perform a systematic study of {\it Swift} GRBs and investigate several short GRB issues. Though sho…

astro-ph.HE2011★ 47 cited

An Evolving Stellar Initial Mass Function and the Gamma-Ray Burst Redshift Distribution

F. Y. Wang, Z. G. Dai

Recent studies suggest that Swift gamma-ray bursts (GRBs) may not trace an ordinary star formation history. Here we show that the GRB rate turns out to be consistent with the star…