New models for neutron stars

Details New models for neutron stars New models for neutron stars

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...362..251b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 362, Oct. 10, 1990, p. 251-255.

Astronomy and Astrophysics

Astronomy

50

Baryons, Black Holes (Astronomy), Field Theory (Physics), Neutron Stars, Stellar Interiors, Stellar Models, Equations Of State, Gravitational Effects, Stellar Mass

Scientific paper

A new type of neutron star model (Q stars), in which high-density, electrically neutral baryonic matter is a coherent classical solution to an effective field theory of strong forces, and is bound in the absence of gravity, is considered. This model allows massive compact objects (suggesting that Cygnus X-1 and LMC X-3 may not be black holes), and has no macroscopic minimum mass. Because laboratory experiments on ordinary nuclei do not constrain the properties of bulk baryon matter, there is a wide new range of theoretical possibilities for compact objects.

Affiliated with

Also associated with

No associations

Rating

New models for neutron stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with New models for neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New models for neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1302299