Results 11 to 20 of about 354 (138)

Pulsar magnetospheres in general relativity [PDF]

open access: yesPhysical Review D, 2018
The main contribution to the pulsar power can be calculated by assuming a rotating magnetically-dominated magnetosphere described by the force-free approximation. Although this simple model has been used thoroughly to study pulsar magnetospheres in the flat spacetime regime, only few works have considered the relativistic corrections introduced by the ...
Carrasco, Federico León   +2 more
openaire   +3 more sources

Generative pulsar timing analysis [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
A new Bayesian method for the analysis of folded pulsar timing data is presented that allows for the simultaneous evaluation of evolution in the pulse profile in either frequency or time, along with the timing model and additional stochastic processes such as red spin noise, or dispersion measure variations. We model the pulse profiles using `shapelets'
Lentati, L, Alexander, P., Hobson, M. P.
openaire   +2 more sources

Pulsar magnetospheres: a general relativistic treatment [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2005
42 pages, 3 figures, Mon. Not. R. Astron.
Kim, Hongsu   +3 more
openaire   +2 more sources

Testing General Relativity with Pulsar Timing [PDF]

open access: yesLiving Reviews in Relativity, 2003
60 pages, accepted for publication in Living Reviews in Relativity (see http://relativity.livingreviews.org).
openaire   +5 more sources

GENERIC GRAVITY TESTS WITH THE DOUBLE PULSAR [PDF]

open access: yesThe Twelfth Marcel Grossmann Meeting, 2012
3 pages, no figures, Proceedings of the 12th Marcel Grossmann Meeting on General Relativity (MG 12), Paris, France, 12-18 Jul ...
Wex, N., Kramer, M.
openaire   +2 more sources

General-relativistic pulsar magnetospheric emission [PDF]

open access: yesMonthly 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.
openaire   +3 more sources

Cherenkov‐Curvature Radiation and Pulsar Radio Emission Generation [PDF]

open access: yesThe Astrophysical Journal, 1999
Electromagnetic processes associated with a charged particle moving in a strong circular magnetic field is considered in cylindrical coordinates. We investigate the relation between the vacuum curvature emission and Cherenkov emission and argue, that for the superluminal motion of a particle in the inhomogeneous magnetic field in a dielectric, the ...
Lyutikov, Maxim   +2 more
openaire   +3 more sources

BlackHoleCam — Testing general relativity with pulsars orbiting Sagittarius A

open access: yesThe Fifteenth Marcel Grossmann Meeting, 2022
BlackHoleCam is a project funded by a European Research Council Synergy Grant to build a complete astrophysical description of nearby supermassive black holes by using a combination of radio imaging, pulsar observations, stellar astrometry and general relativistic magneto-hydrodynamic models.
Eatough, R.P.   +10 more
openaire   +3 more sources

General relativistic effects on pulsar radiation

open access: yes, 2021
20 pages, 6 ...
Kim, Dong-Hoon, Trippe, Sascha
openaire   +2 more sources

Pulsar spin-down luminosity: Simulations in general relativity [PDF]

open access: yesPhysical Review D, 2014
11 pages, 5 figures.
Ruiz Meneses, Milton Javier   +2 more
openaire   +3 more sources

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