Nuclear Equation of State: Picture from Medium Energy Heavy Ion Collisions

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dc.creatorDanielewicz, P.
dc.date2005-12-02
dc.date.accessioned2026-07-07T06:56:01Z
dc.date.available2026-07-07T06:56:01Z
dc.descriptionCharacteristics of the nuclear equation of state (EOS) and its importance, in particular for astrophysics, are discussed. Selected observables in nuclear collisions are sensitive to the EOS and can be used to constrain it. For central collisions, these include collective flow asymmetries, subthreshold kaon yields and isospin diffusion. Comparisons between the data and transport theory suggest an energy per nucleon that rises relatively slowly with density for symmetric matter and symmetry energy that rises relatively quickly around the normal nuclear density.
dc.description7 pages, 12 figures, prepared for the 50'th Symposium on Nuclear Physics, Dec 12-16, 2005, Bhabha Atomic Research Centre, Mumbai, India
dc.identifierhttps://arxiv.org/abs/nucl-th/0512009
dc.identifierhttp://arxiv.org/abs/nucl-th/0512009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/106480
dc.subjectNuclear Theory
dc.titleNuclear Equation of State: Picture from Medium Energy Heavy Ion Collisions
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