Fast radio bursts

TL;DR: Fast radio bursts (FRBs) as discussed by the authors are a class of radio sources that appear similar to the individual pulses from pulsars, but their large dispersive delays suggest that they originate from far outside the Milky Way and hence are many orders-of-magnitude more luminous.

TL;DR: Fast radio bursts (FRBs) as mentioned in this paper are the most common source of radio bursts and have a longer life cycle than the individual pulses from a pulsar and hence are many orders of magnitude more luminous than individual pulsars.

TL;DR: In this article, the authors provide a currently up-to-date catalogue of the numerous and varied theories proposed for Fast Radio Bursts so far and launch an online evolving repository for the use and benefit of the community to dynamically update our theoretical knowledge and discuss constraints and uses of Fast Radio Burst.

TL;DR: In this article, the authors provide a currently up-to-date catalogue of the numerous and varied theories proposed for Fast Radio Bursts so far and launch an online evolving repository for the use and benefit of the community to dynamically update our theoretical knowledge and discuss constraints and uses of Fast Radio Burst.

TL;DR: In this article, a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors.

TL;DR: In this article, it is argued that a convective dynamo can also generate a very strong dipole field after the merger of a neutron star binary, but only if the merged star survives for as long as about 10-100 ms.