{"@context":"http://schema.org","@id":"https://doi.org/10.17182/hepdata.98927.v1/t5","@reverse":{"isBasedOn":[{"@type":"ScholarlyArticle","identifier":{"@type":"PropertyValue","propertyID":"URL","value":"https://inspirehep.net/literature/696676"}},{"@id":"https://doi.org/10.1103/PhysRevC.74.064906","@type":"JournalArticle"}]},"@type":"Dataset","additionalType":"Dataset","author":{"@type":"Organization","name":"STAR Collaboration"},"creator":{"@type":"Organization","name":"STAR Collaboration"},"datePublished":"2021","description":"$(p-\\Lambda) \\oplus (\\bar{p}-\\bar{\\Lambda})$ and $(\\bar{p}-\\Lambda) \\oplus (p-\\bar{\\Lambda})$ combined correlation functions. Correlation functions are corrected for purity and momentum resolution. Curves...","distribution":[{"@type":"DataDownload","contentUrl":"https://www.hepdata.net/download/table/806992/root","description":"ROOT file","encodingFormat":"https://root.cern"},{"@type":"DataDownload","contentUrl":"https://www.hepdata.net/download/table/806992/yaml","description":"YAML file","encodingFormat":"https://yaml.org"},{"@type":"DataDownload","contentUrl":"https://www.hepdata.net/download/table/806992/csv","description":"CSV file","encodingFormat":"text/csv"},{"@type":"DataDownload","contentUrl":"https://www.hepdata.net/download/table/806992/yoda","description":"YODA file","encodingFormat":"https://yoda.hepforge.org"}],"identifier":[{"@type":"PropertyValue","propertyID":"HEPDataRecord","value":"https://www.hepdata.net/record/ins696676?version=1"},{"@type":"PropertyValue","propertyID":"HEPDataRecordAlt","value":"https://www.hepdata.net/record/98927"}],"inLanguage":"en","includedInDataCatalog":{"@id":"https://doi.org/10.17182/hepdata.98927.v1","@type":"DataCatalog","url":"https://www.hepdata.net/record/ins696676?version=1"},"isPartOf":{"@id":"https://doi.org/10.17182/hepdata.98927.v1","@type":"Dataset","description":"We report on $p-\\Lambda$, $p-\\bar{\\Lambda}$, $\\bar{p}-\\Lambda$, and $\\bar{p}-\\bar{\\Lambda}$ correlation functions constructed in central $Au-Au$ collisions at $\\sqrt{s_{NN}}=200$ GeV by the STAR experiment at RHIC. The proton and lambda source size is inferred from the $p-\\Lambda$ and $\\bar{p}-\\bar{\\Lambda}$ correlation functions. It is found to be smaller than the pion source size also measured by the STAR experiment at smaller transverse masses, in agreement with a scenario of a strong universal collective flow. The $p-\\bar{\\Lambda}$ and $\\bar{p}-\\Lambda$ correlation functions, which are measured for the first time, exhibit a large anticorrelation. Annihilation channels and/or a negative real part of the spin-averaged scattering length must be included in the final-state interactions calculation to reproduce the measured correlation function.","name":"Proton Lambda correlations in central Au + Au collisions at s(NN)**(1/2) = 200-GeV.","url":"https://www.hepdata.net/record/ins696676?version=1"},"keywords":"Au Au --> L0(bar L0) p(bar p) X, Kstar, 200, correlations, RHIC, STAR","name":"Table 5","provider":{"@type":"Organization","name":"HEPData"},"publisher":{"@type":"Organization","name":"HEPData"},"url":"https://www.hepdata.net/record/100422","version":1}