Results 61 to 70 of about 525 (178)
Analytical Methods for High Energy Physics
Advances in High Energy Physics, Volume 2019, Issue 1, 2019.
Saber Zarrinkamar +2 more
wiley +1 more source
AbstractWe investigate the combined evolution of the dipolar surface magnetic field (Bs) and the spin-period (Ps) of known Magnetars and high magnetic field ( $${{\rm{B}}_s} \mathbin{\lower.3ex\hbox{$\buildrel>\over {\smash{\scriptstyle\sim}\vphantom{_x}}$}} {10^{13}}{\rm{G}}$$ ) radio pulsars.
Tanmay Tushar Chowhan +2 more
openaire +2 more sources
Two classes of X-ray/$γ$-ray sources, the Soft Gamma Repeaters and the Anomalous X-ray Pulsars have been identified with isolated, slowly spinning magnetars, neutron stars whose emission draws energy from their extremely strong magnetic field ($\sim 10^{15}-10^{16}$ G).
Dall'Osso, Simone, Stella, Luigi
openaire +2 more sources
Low-energy Radio Bursts from Magnetar XTE J1810−197: Implications for Fast Radio Bursts
Magnetars are the leading candidate sources of fast radio bursts (FRBs). However, the observational probes of the connections between magnetars and FRBs are severely limited by the paucity of detection of highly energetic radio events from magnetars—to ...
Banshi Lal +5 more
doaj +1 more source
We report on radio observations of four magnetars SGR 0501+4516, Swift 1834.9–0846, 1E 1841–045, SGR 1900+14, and a magnetar-like pulsar PSR J1846–0258 with the Five-hundred-meter Aperture Spherical radio Telescope at 1250 MHz.
Juntao Bai +9 more
doaj +1 more source
On the Nature of Magnetars [PDF]
The electromagnetic fields of magnetodipole radiation can penetrate to the conducting matter of a neutron star crust and create there electric currents and tangential magnetic fields of high magnitude. The solution obtained here has the form of surface magnetic field discontinuities propagating through the crust to the core.
openaire +1 more source
Magnetars in Binaries as the Engine of Actively Repeating Fast Radio Bursts
The association between FRB 20200428D and the Galactic magnetar SGR J1935+2154 makes magnetars the leading engine of cosmological fast radio bursts (FRBs).
Bing Zhang, Rui-Chong Hu
doaj +1 more source
The Magnetar SGR 1935+2154’s Quiet Local Environment: Clues for Its Progenitor
Magnetars are highly magnetized neutron stars whose evolution and radiation are governed by the decay and/or reconfiguration of their magnetic fields.
Wenlang He, Ping Zhou, Bingqiu Chen
doaj +1 more source
The Galactic Population of Magnetars: A Simulation-based Inference Study
Population synthesis modeling of the observed dynamical and physical properties of a population is a highly effective method for constraining the underlying birth parameters and evolutionary tracks.
M. Sautron +5 more
doaj +1 more source
Formation Channels of Magnetars
The formation channels of magnetars remain an open question. Although core-collapse supernovae of isolated massive stars are important, binary interactions—such as tidal interaction, common envelope evolution, and stellar mergers—may also play a ...
Rui-Chong Hu, Bing Zhang
doaj +1 more source

