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 …

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 …

The interpretation of pulsar rotational glitches, the sudden increase in spin frequency of
neutron stars, is a half-century-old challenge. The common view is that glitches are driven by …

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 …

The strong magnetic field of neutron stars is intimately coupled to the observed temperature
and spectral properties, as well as to the observed timing properties (distribution of spin …

Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-
spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …

Motivated by the recent detection of ultralong-period radio transients, we investigate new
models of coherent radio emission via low-altitude electron–positron pair production in …

We explore the burst energy distribution of fast radio bursts (FRBs) in the low-twist magnetar
model of Wadiasingh & Timokhin (WT19). Motivated by the power-law fluence distributions …

Current models of magnetars require extremely strong magnetic fields to explain their
observed quiescent and bursting emission, implying that the field strength within the star's …