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Quark matter imprint on gravitational waves from oscillating stars
Authors:Omar Benhar  Valeria Ferrari  Leonardo Gualtieri  Stefania Marassi
Affiliation:(1) Dipartimento di Fisica “G. Marconi”, Universitá degli Studi di Roma, “La Sapienza” · INFN, Sezione Roma 1, P.le A. Moro 2, 00185 Rome, Italy
Abstract:We discuss the possibility that the detection of gravitational waves emitted by compact stars may allow to constrain the MIT bag model of quark matter equation of state. Our results show that the combined knowledge of the frequency of the emitted gravitational wave and of the mass, or the radiation radius, of the source allows one to discriminate between strange stars and neutron stars and set stringent bounds on the bag constants.
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