Hadronic matter and rapidly rotating compact stars

Details Hadronic matter and rapidly rotating compact stars Hadronic matter and rapidly rotating compact stars

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994stin...9514442w&link_type=abstract

Presented at the International Conference on Nuclear Structure in the Late Nineties, Hanoi, Viet Nam, 14-18 Mar. 1994

Physics

Hadrons, Matter (Physics), Neutron Stars, Stellar Rotation, Baryons, Equations Of State, Pions, Quarks, Relativity

Scientific paper

In part one of this paper the authors review the present status of neutron star matter calculations, and introduce a representative collection of realistic nuclear equations of state which are derived for different assumptions about the physical behavior of dense matter (baryon populations, pion condensation, possible transition of baryon matter to quark matter). Part two deals with the theoretical determination of the minimum possible rotational periods of neutron stars, performed in the framework of general relativity, whose knowledge serves to distinguish between pulsars that can be understood as rotating neutron stars and those that cannot. Likely candidates for the latter are hypothetical strange stars. Their properties are discussed in the third part of this contribution.

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