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The Equation of State for Cold and Dense Strongly Interacting Matter

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arxiv nucl-th/0301062 v2 pith:GVEIHBRI submitted 2003-01-21 nucl-th astro-phhep-ph

E.S. Fraga , Y. Hatta , R.D. Pisarski , J. Schaffner-Bielich This is my paper · ORCID
classification nucl-thastro-phhep-ph
keywords chiralcolddensedensitiesequationinteractingmatterresults
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We discuss recent results for the equation of state for cold and dense strongly interacting matter. We consider the extreme cases of very high densities, where weak-coupling approaches may in principle give reasonable results, and very low densities, where we use the framework of heavy-baryon chiral perturbation theory. We also speculate on the nature of the chiral transition and present possible astrophysical implications.

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