Publication:
Improved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State

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cris.virtual.departmentDepartamento de Física
cris.virtual.departmentCentro Científico Tecnológico de Valparaíso CCTVAL USM
cris.virtual.departmentDepartamento de Física
cris.virtual.departmentDepartamento de Física
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datacite.subject.fosoecd::Natural sciences
dc.contributor.authorRowley, J.
dc.contributor.authorCompton, N.
dc.contributor.authorDjalali, C.
dc.contributor.authorHicks, K.
dc.contributor.authorPrice, J.
dc.contributor.authorZachariou, N.
dc.contributor.authorAdhikari, K. P.
dc.contributor.authorArmstrong, W. R.
dc.contributor.authorAtac, H.
dc.contributor.authorBaashen, L.
dc.contributor.authorBarion, L.
dc.contributor.authorBashkanov, M.
dc.contributor.authorBattaglieri, M.
dc.contributor.authorBedlinskiy, I.
dc.contributor.authorBenmokhtar, F.
dc.contributor.authorBianconi, A.
dc.contributor.authorBiondo, L.
dc.contributor.authorBiselli, A. S.
dc.contributor.authorBondi, M.
dc.contributor.authorBossù, F.
dc.date.accessioned2024-12-26T18:25:00Z
dc.date.available2024-12-26T18:25:00Z
dc.date.issued2021-12-31
dc.description.abstractStrange matter is believed to exist in the cores of neutron stars based on simple kinematics. If this is true, then hyperon-nucleon interactions will play a significant part in the neutron star equation of state. Yet, compared to other elastic scattering processes, there is very little data on Λ-N scattering. This experiment utilized the CEBAF Large Acceptance Spectrometer (CLAS) detector to study the Λp → Λp elastic scattering cross section in the incident Λ momentum range 0.9–2.0 GeV=c. These are the first data on this reaction since the 1970s. The new cross sections have significantly better accuracy and precision than the existing world data, and the techniques developed here can also be used in future experiments.
dc.identifier10.1103/PhysRevLett.127.272303
dc.identifier.doi10.1103/PhysRevLett.127.272303
dc.identifier.issn00319007
dc.identifier.scopus2-s2.0-85122493659
dc.identifier.urihttps://cris.usm.cl/handle/123456789/1966
dc.language.isoen
dc.relation.ispartofPhysical Review Letters
dc.relation.ispartofseriesPhysical Review Letters
dc.rightstrue
dc.rightsAttribution 4.0 International*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.subjectn/a
dc.titleImproved Λp Elastic Scattering Cross Sections between 0.9 and 2.0 GeV/c as a Main Ingredient of the Neutron Star Equation of State
dc.typeResource Types::text::journal::journal article::review article
dspace.entity.typePublication
oaire.citation.issue27
oaire.citation.volume127
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person.affiliation.nameOhio University
person.affiliation.nameOhio University
person.affiliation.nameOhio University
person.affiliation.nameOhio University
person.affiliation.nameCalifornia State University, Dominguez Hills
person.affiliation.nameUniversity of York
person.affiliation.nameOld Dominion University
person.affiliation.nameArgonne National Laboratory
person.affiliation.nameTemple University
person.affiliation.nameFlorida International University
person.affiliation.nameIstituto Nazionale di Fisica Nucleare, Sezione di Ferrara
person.affiliation.nameUniversity of York
person.affiliation.nameIstituto Nazionale di Fisica Nucleare, Sezione di Genova
person.affiliation.nameNational Research Centre "Kurchatov Institute"
person.affiliation.nameDuquesne University
person.affiliation.nameIstituto Nazionale di Fisica Nucleare, Sezione di Pavia
person.affiliation.nameIstituto Nazionale di Fisica Nucleare, Sezione di Catania
person.affiliation.nameFairfield University
person.affiliation.nameIstituto Nazionale di Fisica Nucleare, Sezione di Genova
person.affiliation.nameUniversité Paris-Saclay
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