Hadronic and Quark Matter – Applications in AstrophysicsNo Access

SLOWLY ROTATING PULSARS

M. D. ALLOY

Depto de Fsica, CFM, Universidade Federal de Santa Catarina, Florianpolis, SC, CP. 476, CEP 88.040 - 900, Brazil

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and

D. P. MENEZES

Depto de Fsica, CFM, Universidade Federal de Santa Catarina, Florianpolis, SC, CP. 476, CEP 88.040 - 900, Brazil

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https://doi.org/10.1142/S0218301307008501Cited by:0 (Source: Crossref)

Abstract

In the present work we investigate one possible variation on the usual static pulsars: the inclusion of rotation. We use a formalism proposed by Hartle and Thorne to calculate the properties of rotating pulsars with all possible compositions. All calculations were performed for zero temperature and also for fixed entropy equations of state.

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