Results 81 to 90 of about 1,325 (160)
General-relativistic pulsar magnetospheric emission [PDF]
Monthly Notices of the Royal Astronomical Society, 2018 Most current pulsar emission models assume photon production and emission within the magnetosphere. Low frequency radiation is preferentially produced in the vicinity of the polar caps whereas the high-energy tail is shifted to regions closer but still inside the light-cylinder.
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Generation of relativistic particles in pulsar magnetospheres
, 2012 The problem - fundamental for the physics of pulsars - of determining the global structure of the magnetosphere in a self-consistent way has not yet been solved satisfactorily. We report on some progress in this direction, which we have achieved by studying the trajectories of individual charged particles in the electromagnetic vacuum fields of an ...
Herold, Heinz +2 more
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Testing general relativity with black hole-pulsar binaries
Physical Review D, 2018 Binary pulsars allow us to carry out precision tests of gravity and have placed stringent bounds on a broad class of theories beyond general relativity. Current and future radio telescopes, such as FAST, SKA, and MeerKAT, may find a new astrophysical system, a pulsar orbiting around a black hole, which will provide us a new source for probing gravity ...
Seymour, Brian C., Yagi, Kent
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Pulse shapes of radio pulsars at 4.85 GHz [PDF]
, 1997 . We present pulse shapes of 87 pulsars at 4.85 GHz. Pulse widths and flux densities are measured. The frequency dependence of the prole shape and the pulse width is discussed.
A. Jessner +3 more
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Random Number Generation from Pulsars
Pulsars exhibit signals with precise inter-arrival times that are on the order of milliseconds to seconds, depending on the individual pulsar. There are subtle variations in the timing of pulsar signals. We show that these variations can serve as a natural entropy source for the creation of Random Number Generators (RNGs).
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A Cosmic Census of Radio Pulsars with the SKA [PDF]
, 2014 20 pages, 7 figures, to be published in: "Advancing Astrophysics with the Square Kilometre Array", Proceedings of Science, PoS(AASKA14)040International audienceThe Square Kilometre Array (SKA) will make ground breaking discoveries in pulsar science.
Janssen, G +74 more
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Testing General Relativity with Pulsar Timing Arrays
Proceedings of the Wisconsin Space Conference, 2012 Pulsar timing arrays are a promising tool for probing the universe through gravitational radiation. A variety of astrophysical and cosmological sources are expected to contribute to a stochastic background of gravitational waves (GWs) in the pulsar timing array (PTA) frequency band.
Sydney Chamberlin, Xavier Siemens
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High-Energy Emission from Rotation-Powered Pulsars [PDF]
, 2007 Thirty-five years after the discovery of rotation-powered pulsars, we still do not understand their pulsed emission at any wavelength. In the last few years there have been some fundamental developments in acceleration and emission models.
Harding, Alice K.
core
Rotochemical heating in millisecond pulsars [PDF]
, 2005 Rotochemical heating originates in a departure from beta equilibrium due to spin-down compression in a rotating neutron star. The main consequence is that the star eventually arrives at a quasi-equilibrium state in which the thermal photon luminosity ...
Fernández, R, Reisenegger, A
core
Cracking the Endothelial Calcium (Ca2+) Code: A Matter of Timing and Spacing. [PDF]
Int J Mol Sci, 2023 Moccia F +4 more
europepmc +1 more source