arXiv · 1604.01799
Fast Radio Bursts---A Brief Review: Some Questions, Fewer Answers
Abstract
Fast Radio Bursts are millisecond bursts of radio radiation at frequencies of about 1 GHz, recently discovered in pulsar surveys. They have not yet been definitively identified with any other astronomical object or phenomenon. The bursts are strongly dispersed, indicating passage through a high column density of low density plasma. The most economical interpretation is that this is the interglactic medium, indicating that FRB are at "cosmological" distances with redshifts in the range 0.3--1.3. Their inferred brightness temperatures are as high as $10^{37\,\circ}$K, implying coherent emission by "bunched" charges, as in radio pulsars. I review the astronomical sites, objects and emission processes that have been proposed as the origin of FRB, with particular attention to Soft Gamma Repeaters and giant pulsar pulses.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
J. I. Katz. 2016-05-09. Fast Radio Bursts---A Brief Review: Some Questions, Fewer Answers. https://doi.org/10.1142/s0217732316300135
Cite the original work for its findings. Save a collection to share your selection of sources.