dc.creatorBugaev K.A.
dc.creatorVitiuk O.V.
dc.creatorGrinyuk B.E.
dc.creatorYakovenko N.S.
dc.creatorZherebtsova E.S.
dc.creatorSagun V.V.
dc.creatorSavchenko D.O.
dc.creatorBravina L.V.
dc.creatorBlaschke D.B.
dc.creatorFarrar G.R.
dc.creatorKabana S.
dc.creatorKuleshov S.V.
dc.creatorNikonov E.G.
dc.creatorTaranenko A.V.
dc.creatorZabrodin E.E.
dc.creatorZinovjev G.M.
dc.date.accessioned2021-08-03T21:57:49Z
dc.date.accessioned2024-05-02T15:05:09Z
dc.date.available2021-08-03T21:57:49Z
dc.date.available2024-05-02T15:05:09Z
dc.date.created2021-08-03T21:57:49Z
dc.date.issued2020-10
dc.identifierJournal of Physics: Conference Series, Volume 1690, Issue 116 December 2020 Article number 0121235th International Conference on Particle Physics and Astrophysics, ICPPA 2020, Moscow, Virtual, 5 October 2020 - 9 October 2020, 165881
dc.identifier17426588
dc.identifierhttp://repositorio.unab.cl/xmlui/handle/ria/19639
dc.identifier10.1088/1742-6596/1690/1/012123
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9262160
dc.description.abstractWe present a summary of the recent results obtained with the novel hadron resonance gas model with the multicomponent hard-core repulsion which is extended to describe the mixtures of hadrons and light (anti-, hyper-)nuclei. A very accurate description is obtained for the hadronic and the light nuclei data measured by STAR at the collision energy The most striking result discussed here is that for the most probable chemical freeze-out scenario for the STAR energy the found parameters allow us to reproduce the values of the experimental ratios S 3 and without fitting. © Published under licence by IOP Publishing Ltd.
dc.languagees
dc.publisherIOP Publishing Ltd
dc.subjectIonic Collisions
dc.subjectStrangeness
dc.subjectHadrons
dc.titleChemical freeze-out of light nuclei in high energy nuclear collisions and resolution of the hyper-Triton chemical freeze-out puzzle
dc.typeArtículo


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