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 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 …

Providing an introduction to the theory of nonlinear Fokker-Planck equations, this book
discusses fundamental properties of transient and stationary solutions, emphasizing the …

Two recent discoveries, namely PSR J0901− 4046 and GLEAM-X J162759. 5− 523504.3
(hereafter GLEAM-X J1627), have corroborated an extant population of radio-loud periodic …

We analyze the statistics of pulse arrival times in fast radio burst(FRB) 121102 and
demonstrate that they are remarkably similar to statistics of magnetar high-energy short …

We develop a theoretical model that explains the formation of hot coronae around strongly
magnetized neutron stars—magnetars. The starquakes of a magnetar shear its external …

The extraordinary 1998 August 27 giant flare places strong constraints on the physical
properties of its source, SGR 1900+ 14. We make detailed comparisons of the published …

We report on NICER observations of the magnetar SGR 1935+ 2154, covering its 2020 burst
storm and long-term persistent emission evolution up to∼ 90 days postoutburst. During the …

The soft gamma repeater SGR 1900+ 14 became active again on 1998 June after a long
period of quiescence; it remained at a low state of activity until 1998 August, when it emitted …

The production mechanism of repeating fast radio bursts (FRBs) is still a mystery, and
correlations between burst occurrence times and energies may provide important clues to …