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Related papers: Fast radio bursts as cosmic lightning

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The existence of fast radio bursts (FRBs), a new type of extragalatic transients, has been established recently and quite a few models have been proposed. In this work we discuss the possible connection between the FRB sources and…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Xiang Li , Bei Zhou , Hao-Ning He , Yi-Zhong Fan , Da-Ming Wei

When fast radio burst (FRB) waves propagate through the local (< 1 pc) environment of the FRB source, electrons in the plasma undergo large-amplitude oscillations. The finite-amplitude effects cause the effective plasma frequency and…

High Energy Astrophysical Phenomena · Physics 2020-08-10 Wenbin Lu , E. Sterl Phinney

Fast radio bursts (FRBs) are brief, luminous pulses with unknown physical origin. The repetition pattern of FRBs contains essential information about their physical nature and emission mechanisms. Using the two largest samples of FRB…

High Energy Astrophysical Phenomena · Physics 2023-06-14 F. Y. Wang , Q. Wu , Z. G. Dai

Fast radio bursts (FRBs) are millisecond-duration events thought to originate beyond the Milky Way galaxy. Uncertainty surrounding the burst sources, and their propagation through intervening plasma, has limited their use as cosmological…

A bright radio burst was newly discovered in SGR 1935+2154, which exhibit some FRB-like temporal- and frequency-properties, suggesting a neutron star (NS)/magnetar magnetospheric origin of FRBs. We propose an explanation of the temporal-…

High Energy Astrophysical Phenomena · Physics 2020-08-26 Wei-Yang Wang , Renxin Xu , Xuelei Chen

We analyze the sources of free electrons that produce the large dispersion measures, DM $\approx 300-1600$ (in units cm$^{-3}$ pc), observed toward fast radio bursts (FRBs). Individual galaxies typically produce DM $\sim 25-60$ cm$^{-3}$ pc…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-10 J. Michael Shull , Charles W. Danforth

Fast radio bursts (FRBs) are millisecond radio pulses with extremely high bright temperature. Their physical origin is still a mystery. The discovery of FRB 20020428 supports the idea that at least a portion of FRBs is generated by…

High Energy Astrophysical Phenomena · Physics 2025-07-23 H. T. Lan , S. X. Yi , F. Y. Wang

The recent discovery of a Mega-Jansky radio burst occurring simultaneously with short X-ray bursts from the Galactic magnetar (strongly magnetized neutron star (NS)) SGR 1935+2154 is a smoking gun for the hypothesis that some cosmological…

High Energy Astrophysical Phenomena · Physics 2020-12-02 Kunihito Ioka

Most Fast Radio Burst (FRB) models are built from comparatively common astronomical objects: neutron stars, black holes and supernova remnants. Yet FRB sources are rare, and most of these objects, found in the Galaxy, do not make FRB.…

High Energy Astrophysical Phenomena · Physics 2021-08-20 J. I. Katz

Fast radio bursts (FRBs) have excessive dispersion measures (DMs) and an all-sky distribution, which point toward an extragalactic or even a cosmological origin. We develop a method to extract the mean host galaxy DM ($\left\langle{\rm…

High Energy Astrophysical Phenomena · Physics 2017-04-26 Yuan-Pei Yang , Rui Luo , Zhuo Li , Bing Zhang

A variety of current models for gamma-ray bursts (GRBs) suggest a common engine - a black hole of several solar masses accreting matter from a disk at a rate 0.01 to 10 solar masses per second. Using a numerical model for relativistic disk…

Astrophysics · Physics 2011-07-18 Robert Popham , S. E. Woosley , Chris Fryer

Recent observations suggest that in black hole X-ray binaries jet/outflow formation is related to the hot plasma in the vicinity of the black hole, either in the form of an advection-dominated accretion flow at low accretion rates or in a…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Qingwen Wu , Xinwu Cao , Luis C. Ho , Ding-Xiong Wang

Fast radio bursts appear to exhibit large dispersion measures, typically exceeding any expected galactic interstellar contribution, especially along the moderate to high-galactic-latitude directions in which such events have been most often…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Brian Dennison

Fast Radio Bursts (FRBs) are bright, extragalactic radio pulses whose origins are still unknown. Until recently, most FRBs have been detected at frequencies greater than 1 GHz with a few exceptions at 800 MHz. The recent discoveries of FRBs…

High Energy Astrophysical Phenomena · Physics 2020-03-11 K. M. Rajwade , M. B. Mickaliger , B. W. Stappers , C. G. Bassa , R. P. Breton , A. Karastergiou , E. F. Keane

Highly beamed, short-duration electromagnetic bursts could be produced by superconducting cosmic string (SCS) loops oscillating in cosmic magnetic fields. We demonstrated that the basic characteristics of SCS bursts such as the…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Yun-Wei Yu , Kwong-Sang Cheng , Gary Shiu , Henry Tye

Fast radio bursts (FRBs) are extragalactic radio transients with extremely high brightness temperature, which strongly suggests the presence of coherent emission mechanisms. In this study, we introduce a novel radiation mechanism for FRBs…

High Energy Astrophysical Phenomena · Physics 2023-09-13 Ze-Nan Liu , Jin-Jun Geng , Yuan-Pei Yang , Wei-Yang Wang , Zi-Gao Dai

Currently, fast radio bursts (FRBs) have become a very active field in astronomy and cosmology. However, the origin of FRBs is still unknown to date. The studies on the intrinsic FRB distributions might help us to reveal the possible…

High Energy Astrophysical Phenomena · Physics 2022-01-21 Da-Chun Qiang , Shu-Ling Li , Hao Wei

The recently discovered fast radio bursts (FRBs), presumably of extra-galactic origin, have the potential to become a powerful probe of the intergalactic medium (IGM). We point out a few such potential applications. We provide expressions…

High Energy Astrophysical Phenomena · Physics 2015-12-29 Z. Zheng , E. O. Ofek , S. R. Kulkarni , J. D. Neill , M. Juric

The radiation physics of repeating fast radio bursts (FRBs) remains enigmatic. Motivated by the observed narrow-banded emission spectrum and ambiguous fringe pattern of the spectral peak frequency ($\nu_{\rm pk}$) distribution of some…

High Energy Astrophysical Phenomena · Physics 2025-02-18 Xiao Li , Fen Lyu , Hai Ming Zhang , Can-Min Deng , En-Wei Liang

We consider radio emission from a newborn black hole (BH), which is accompanied by a mini-disk with a mass of $\lesssim M_\odot$. Such a disk can be formed from an outer edge of the progenitor's envelope, especially for metal-poor massive…

High Energy Astrophysical Phenomena · Physics 2018-06-26 Kazumi Kashiyama , Kenta Hotokezaka , Kohta Murase
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