Phys. Rev. D 44, 1321 (1991) - Rotational properties of strange-pulsar models

Rotational properties of strange-pulsar models

O. G. Benvenuto, J. E. Horvath, and H. Vucetich

Phys. Rev. D 44, 1321 – Published 15 August 1991

Abstract

We present a study of the rotational properties of strange pulsars: strange-matter stars capable of supporting glitches. It is shown that their differentiated internal structure implies a lower maximum rotational frequency than that of homogeneous strange stars. Nevertheless, they are able to fit the known pulsar properties.

Received 10 December 1990

DOI:https://doi.org/10.1103/PhysRevD.44.1321

©1991 American Physical Society

Authors & Affiliations

O. G. Benvenuto

Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque S/N, (1900) La Plata, Argentina

Instituto Astrónomico e Geofísico, Departamento de Astronomía, Universidade de São Paulo, Caixa Postal 30627, 01051 São Paulo, Brasil

Departamento de Física, Facultad de Ciencias Exactas, Universidad Nacional de La Plata, C.C. 67, (1900) La Plata, Argentina

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Issue

Vol. 44, Iss. 4 — 15 August 1991

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