Baryon contrast ratio in an isentropic cosmological quark-hadron phase transition

Details Baryon contrast ratio in an isentropic cosmological quark-hadron phase transition Baryon contrast ratio in an isentropic cosmological quark-hadron phase transition

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phlb..427..241p&link_type=abstract

Physics Letters B, Volume 427, Issue 3-4, p. 241-247.

Physics

2

Scientific paper

Assuming that the quark-hadron phase transition in the early Universe satisfies the Gibbs' construction for a first-order equilibrium phase transition with a further constraint of a continuous entropy per baryon-number ratio across the phase boundary, we show that the baryon contrast ratio R defined as a measure of the baryon-number density inhomogeneity across the phase interface, is independent of the critical temperature Tc for the phase transition. It does not depend on the QCD parameters as well. Our finding contradicts the earlier results.

Affiliated with

Also associated with

No associations

Rating

Baryon contrast ratio in an isentropic cosmological quark-hadron phase transition 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 Baryon contrast ratio in an isentropic cosmological quark-hadron phase transition, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Baryon contrast ratio in an isentropic cosmological quark-hadron phase transition will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1865737