Results 11 to 20 of about 17,260 (230)

Observations of Radio Magnetars with the Deep Space Network [PDF]

open access: yesAdvances in Astronomy, 2019
The Deep Space Network (DSN) is a worldwide array of radio telescopes which supports NASA’s interplanetary spacecraft missions. When the DSN antennas are not communicating with spacecraft, they provide a valuable resource for performing observations of ...
Aaron B. Pearlman   +2 more
doaj   +3 more sources

Multipolar Electromagnetic Emission of Newborn Magnetars [PDF]

open access: yesThe Astrophysical Journal
It is generally recognized that the electromagnetic multipolar emission from magnetars can be used to explain radiation from soft gamma repeaters or anomalous X-ray pulsars, but they have little impact on the spin-down of magnetars.
Yu Wang, Rahim Moradi, Liang Li
doaj   +2 more sources

IXPE detection of polarized X-rays from magnetars and photon mode conversion at QED vacuum resonance. [PDF]

open access: yesProc Natl Acad Sci U S A, 2023
Significance The recent detections of polarized X-rays from magnetars have opened up a new avenue to study magnetars, neutron stars endowed with superstrong magnetic fields.
Lai D.
europepmc   +3 more sources

The Stochastic Gravitational Wave Background from Magnetars [PDF]

open access: yesUniverse, 2021
Magnetars have already been a potential candidate as gravitational wave sources that could be detected by current and future terrestrial as well as ground-based gravitational wave detectors.
Sourav Roy Chowdhury, Maxim Khlopov
doaj   +2 more sources

Axion-mediated Transport of Fast Radio Bursts Originating in Inner Magnetospheres of Magnetars [PDF]

open access: yesAstrophysical Journal Letters, 2023
Among magnetar models of fast radio bursts (FRBs), there is ongoing debate about whether the site of coherent radio emission lies within or beyond the light cylinder. We propose a mechanism by which FRBs produced near the magnetar surface are transported
A. Prabhu
semanticscholar   +1 more source

Deflection of light by magnetars in the generalized Born–Infeld electrodynamics [PDF]

open access: yesThe European Physical Journal C, 2022
We study the deflection of light by a magnetic dipole field in the generalized Born–Infeld electrodynamics. Using the effective index of refraction and the trajectory equation based on geometric optics, we compute the weak bending angle of light passing ...
Jin Young Kim
semanticscholar   +1 more source

Evidence for an abundant old population of Galactic ultra long period magnetars and implications for fast radio bursts [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2022
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 sources with long periods (76 s and 1091 s respectively) whose emission can hardly be ...
P. Beniamini   +5 more
semanticscholar   +1 more source

High-energy Photon Opacity in the Twisted Magnetospheres of Magnetars [PDF]

open access: yesAstrophysical Journal, 2022
Magnetars are neutron stars characterized by strong surface magnetic fields generally exceeding the quantum critical value of 44.1 TG. High-energy photons propagating in their magnetospheres can be attenuated by QED processes like photon splitting and ...
K. Hu   +3 more
semanticscholar   +1 more source

Precession of magnetars: dynamical evolutions and modulations on polarized electromagnetic waves [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2022
Magnetars are conjectured to be highly magnetized neutron stars (NSs). Strong internal magnetic field and elasticity in the crust may deform the stars and lead to free precession.
Yong Gao   +5 more
semanticscholar   +1 more source

Magnetars and axion-like particles: probes with the hard X-ray spectrum [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2021
Quiescent hard X-ray and soft gamma-ray emission from neutron stars constitute a promising frontier to explore axion-like-particles (ALPs). ALP production in the core peaks at energies of a few keV to a few hundreds of keV; subsequently, the ALPs escape ...
J. Fortin   +4 more
semanticscholar   +1 more source

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