A living theory catalogue for fast radio bursts

E Platts, A Weltman, A Walters, SP Tendulkar… - Physics Reports, 2019 - Elsevier
At present, we have almost as many theories to explain Fast Radio Bursts as we have Fast
Radio Bursts observed. This landscape will be changing rapidly with CHIME/FRB, recently …

Magnetars

VM Kaspi, AM Beloborodov - Annual Review of Astronomy and …, 2017 - annualreviews.org
Magnetars are young and highly magnetized neutron stars that display a wide array of X-ray
activity including short bursts, large outbursts, giant flares, and quasi-periodic oscillations …

An extreme magneto-ionic environment associated with the fast radio burst source FRB 121102

D Michilli, A Seymour, JWT Hessels, LG Spitler… - Nature, 2018 - nature.com
Fast radio bursts are millisecond-duration, extragalactic radio flashes of unknown physical
origin,,. The only known repeating fast radio burst source,,—FRB 121102—has been …

Magnetars: the physics behind observations. A review

R Turolla, S Zane, AL Watts - Reports on Progress in Physics, 2015 - iopscience.iop.org
Magnetars are the strongest magnets in the present universe and the combination of
extreme magnetic field, gravity and density makes them unique laboratories to probe current …

A flaring magnetar in FRB 121102?

AM Beloborodov - The Astrophysical Journal Letters, 2017 - iopscience.iop.org
A Flaring Magnetar in FRB 121102? - IOPscience This site uses cookies. By continuing to use
this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy …

Blast waves from magnetar flares and fast radio bursts

AM Beloborodov - The Astrophysical Journal, 2020 - iopscience.iop.org
Magnetars younger than one century are expected to be hyperactive: besides winds
powered by rotation, they can generate frequent magnetic flares, which launch powerful …

A model for fast extragalactic radio bursts

Y Lyubarsky - Monthly Notices of the Royal Astronomical …, 2014 - academic.oup.com
Bursts of millisecond duration were recently discovered in the 1 GHz band. There is a strong
evidence that they come from∼ 1 Gpc distances, which implies extraordinary high …

Short-hard gamma-ray bursts

E Nakar - Physics Reports, 2007 - Elsevier
Two types of gamma-ray bursts (GRBs) are observed: short-duration hard spectrum GRBs
and long-duration soft spectrum GRBs. For many years long GRBs were the focus of intense …

The evolution and structure of pulsar wind nebulae

BM Gaensler, PO Slane - Annu. Rev. Astron. Astrophys., 2006 - annualreviews.org
Pulsars steadily dissipate their rotational energy via relativistic winds. Confinement of these
outflows generates luminous pulsar wind nebulae, seen across the electromagnetic …

Physics of strongly magnetized neutron stars

AK Harding, D Lai - Reports on Progress in Physics, 2006 - iopscience.iop.org
There has recently been growing evidence for the existence of neutron stars possessing
magnetic fields with strengths that exceed the quantum critical field strength of 4.4× 10 13 G …