Superfluidity of hyperons in warm strange hadronic star matter

Abstract

In this work we evaluate the 1S0 superfluidity of hyperons in β-stable strange hadronic matter. We investigate the equation of state (EOS) of hadronic matter at finite values of baryon density and temperature in the relativistic mean field (RMF) theory. Effects of the introduced isoscalar-isovector cross-interaction term on the superfluidity are investigated systematically. In addition, the temperature effects on the superfluidity of hyperons in hadronic matter are discussed. It is found that the density region and the magnitude of the pairing gap are dependent on the cross-interaction term. The obtained maximal critical temperature of superfluid is around 109 K.

0

Turn this paper into a lesson

ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.

Discussion (0)

Sign in to join the discussion.

Loading comments…