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On the Circular Polarisation of Repeating Fast Radio Bursts
Shi Dai, Jiguang Lu, Chen Wang +9
Fast spinning (e.g., sub-second) neutron star with ultra-strong magnetic fields (or so-called magnetar) is one of the promising origins of repeating fast radio bursts (FRBs). Here…
Kilonova Emission From Black Hole-Neutron Star Mergers. II. Luminosity Function and Implications for Target-of-opportunity Observations of Gravitational-wave Triggers and Blind Searches
Jin-Ping Zhu, Shichao Wu, Yuan-Pei Yang +8
We present detailed simulations of black hole-neutron star (BH-NS) mergers kilonova and gamma-ray burst (GRB) afterglow and kilonova luminosity function, and discuss the detectabil…
Repeating Fast Radio Bursts from Pulsar-Asteroid Belt Collisions: Frequency Drifting and Polarization
Ze-Nan Liu, Wei-Yang Wang, Yuan-Pei Yang +1
Fast radio bursts (FRBs) are a new kind of extragalactic radio transients. Some of them show repeating behaviors. Recent observations indicate that a few repeating FRBs (e.g., FRB…
Pair separation in parallel electric field in magnetar magnetosphere and narrow spectra of fast radio bursts
Yuan-Pei Yang, Jin-Ping Zhu, Bing Zhang +1
When the magnetosphere of a magnetar is perturbed by crustal deformation, an electric field parallel to the magnetic field line would appear via Alvfén waves in the c…
Persistent Radio Emission from Synchrotron Heating by a Repeating Fast Radio Burst Source in a Nebula
Qiao-Chu Li, Yuan-Pei Yang, Zi-Gao Dai
The first repeating fast radio burst (FRB), FRB 121102, was found to be associated with a spatially coincident, persistent nonthermal radio source, but the origin of the persistent…
Is GRB 110715A the progenitor of FRB 171209?
Xiang-Gao Wang, Long Li, Yuan-Pei Yang +5
The physical origin of fast radio bursts (FRBs) is unknown. Young magnetars born from gamma-ray bursts (GRBs) have been suggested to be a possible central engine of FRBs. We test s…
Cosmology-insensitive estimate of IGM baryon mass fraction from five localized fast radio bursts
Zhengxiang Li, He Gao, Jun-Jie Wei +3
Five fast radio bursts (FRBs), including three apparently non-repeating ones FRB 180924, FRB 181112, and FRB 190523, and two repeaters, FRB 121102 and FRB 180916.J0158+65, have alr…
Kilonova Emission From Black Hole-Neutron Star Mergers. I. Viewing-Angle-Dependent Lightcurves
Jin-Ping Zhu, Yuan-Pei Yang, Liang-Duan Liu +5
In this paper, we present a numerical method to study the predicted lightcurves as a function of viewing angle. We extrapolate the fitting formulae for the mass and velocity of tid…
Fast radio bursts from activities of neutron stars newborn in BNS mergers: offset, birth rate and observational properties
F. Y. Wang, Y. Y. Wang, Yuan-Pei Yang +3
Young neutron stars (NSs) born in core-collapse explosions are promising candidates for the central engines of fast radio bursts (FRBs), since the first localized repeating burst F…
The effects of plasma lensing on the inferred dispersion measures of Fast Radio Bursts
Xinzhong Er, Yuanpei Yang, Adam Rogers
Radio signals are delayed when propagating through plasma. This type of delay is frequency-dependent and is usually used for estimating the projected number density of electrons al…
Are persistent emission luminosity and rotation measure of fast radio bursts related?
Yuan-Pei Yang, Qiao-Chu Li, Bing Zhang
The physical origin of fast radio bursts (FRBs) is still unknown. Multiwavelength and polarization observations of an FRB source would be helpful to diagnose its progenitor and env…
Fast radio bursts as strong waves interacting with ambient medium
Yuan-Pei Yang, Bing Zhang
Fast radio bursts (FRBs) are mysterious radio transients whose physical origin is still unknown. Within a few astronomical units near an FRB source, the electric field of the elect…