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Pulsar spin-down luminosity: Simulations in general relativity.

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Pulsar spin-down luminosity: Simulations in general relativity.

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dc.contributor.author Ruiz Meneses, Milton Javier
dc.contributor.author Paschalidis, Vasileios
dc.contributor.author Shapiro, Stuart L.
dc.date.accessioned 2023-06-02T06:34:09Z
dc.date.available 2023-06-02T06:34:09Z
dc.date.issued 2014
dc.identifier.citation Ruiz Meneses, Milton Javier Paschalidis, Vasileios Shapiro, Stuart L. 2014 Pulsar spin-down luminosity: Simulations in general relativity. Physical Review D 89 8 1 11
dc.identifier.uri https://hdl.handle.net/10550/87629
dc.description.abstract Adopting our new method for matching general relativistic, ideal magnetohydrodynamics to its force-free limit, we perform the first systematic simulations of force-free pulsar magnetospheres in general relativity. We endow the neutron star with a general relativistic dipole magnetic field, model the interior with ideal magnetohydrodynamics, and adopt force-free electrodynamics in the exterior. Comparing the spin-down luminosity to its corresponding Minkowski value, we find that general relativistic effects give rise to a modest enhancement: the maximum enhancement for n=1 polytropes is ∼23%. Evolving a rapidly rotating n=0.5 polytrope we find an even greater enhancement of ∼35%. Using our simulation data, we derive fitting formulas for the pulsar spin-down luminosity as a function of the neutron star compaction, angular speed, and dipole magnetic moment. We expect stiffer equations of state and more rapidly spinning neutron stars to lead to even larger enhancements in the spin-down luminosity.
dc.language.iso eng
dc.relation.ispartof Physical Review D, 2014, vol. 89, num. 8, p. 1-11
dc.subject Astronomia
dc.subject Astrofísica
dc.title Pulsar spin-down luminosity: Simulations in general relativity.
dc.type journal article
dc.date.updated 2023-06-02T06:34:10Z
dc.identifier.doi 10.1103/PhysRevD.89.084045
dc.identifier.idgrec 160069
dc.rights.accessRights open access

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