Improvements on the structure of strange stars

Details Improvements on the structure of strange stars Improvements on the structure of strange stars

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.247..584b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 247, Dec. 15, 1990, p. 584-590. Research supported by C

Astronomy and Astrophysics

Astronomy

14

Neutron Stars, Quantum Chromodynamics, Stellar Models, Stellar Structure, Alpha Particles, Pulsars, Quarks, Strangeness

Scientific paper

This paper presents the structure of strange-star models, including the effects of a specific hypothetical few-quark bound state (quark-alpha). The general features of these stellar objects are discussed and analyzed in detail. It is shown that this modification to the strange-matter picture would make it possible to interpret the 'glitch' phenomenon observed in many pulsars in terms of features possessed by such objects. For low-mass stars it is found that the structure consists entirely of quark-alpha matter, forming a new branch of stable compact stars.

Affiliated with

Also associated with

No associations

Rating

Improvements on the structure of strange 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 Improvements on the structure of strange stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Improvements on the structure of strange stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1633178