On the structure of strange stars and bagged QCD parameters

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

22

Peculiar Stars, Stellar Evolution, Stellar Structure, Baryons, Equations Of State, Red Shift, Stellar Magnetic Fields, Stellar Models

Scientific paper

The structure of stellar objects made up of strange matter, suspected to be the actual ground state of cold, dense baryonic matter, has been studied. The equation of state containing three strong interaction parameters B, alpha(c) and m(s) has been varied throughout the strange matter stability window in order to get a wide picture of these hypothetical objects. It is found that this type of model can account for the presently known observational features of compact objects, and conversely, that no restriction on the space of parameters (compatible with strange matter stability) is imposed by observational facts; unless some configurations having both e(-) and e(+) in their structure happen to be unstable. The issues of the most likely parameter set in the light of present QCD understanding and the birth scenarios of strange stars are also briefly discussed.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

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

Rate now

     

Profile ID: LFWR-SCP-O-1617017

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.