Quark core formation in spinning-down pulsars

Simple item page
dc.creatorMarranghello, G. F.
dc.creatorRegimbau, T.
dc.creatorPacheco, J. A. de Freitas
dc.date2007-03-19
dc.date.accessioned2026-07-07T10:36:57Z
dc.date.available2026-07-07T10:36:57Z
dc.descriptionPulsars spin-down due to magnetic torque reducing its radius and increasing the central energy density. Some pulsar which are born with central densities close to the critical value of quark deconfinement may undergo a phase transition and structural re-arrengement. This process may excite oscillation modes and emmit gravitational waves. We determine the rate of quark core formation in neutron stars using a realistic population synthesis code.
dc.descriptionProceedings of the 2nd International Workshop on Astronomy and Relativistic Astrophysics, to appear in IJMPD
dc.identifierhttps://arxiv.org/abs/astro-ph/0703507
dc.identifierhttp://arxiv.org/abs/astro-ph/0703507
dc.identifierInt.J.Mod.Phys.D16:313-318,2007
dc.identifierdoi:10.1142/S0218271807010067
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180224
dc.subjectAstrophysics
dc.titleQuark core formation in spinning-down pulsars
dc.typetext

Files

Collections

arXiv