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Zastosuj identyfikator do podlinkowania lub zacytowania tej pozycji: http://hdl.handle.net/20.500.12128/14651
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dc.contributor.authorSzadziński, Albert-
dc.contributor.authorWilczek, Andrzej-
dc.contributor.authorStephan, Elżbieta-
dc.contributor.authorWłoch, B.-
dc.contributor.authorKalantar-Nayestanakic, N.-
dc.contributor.authorKistryn, St.-
dc.contributor.authorKłos, Barbara-
dc.contributor.authorKozela, A.-
dc.contributor.authorKulessa, P.-
dc.contributor.authorŁobejko, Angelina-
dc.contributor.authorMesschendorp, J.-
dc.contributor.authorParol, W.-
dc.contributor.authorSkwira-Chalot, I.-
dc.contributor.authorZejma, J.-
dc.date.accessioned2020-06-22T06:03:37Z-
dc.date.available2020-06-22T06:03:37Z-
dc.date.issued2020-
dc.identifier.citationActa Physica Polonica B, Vol. 51, No 3 (2020), s. 763-768pl_PL
dc.identifier.issn0587-4254-
dc.identifier.urihttp://hdl.handle.net/20.500.12128/14651-
dc.description.abstractStar Anomaly is one of the most intriguing and unsolved discrepancies between theoretical calculations and experimental data observed in the domain of few-nucleon systems at low energies. Previous and upcoming measurements of the breakup reaction with the use of the BINA detector enable systematic studies of the Star configurations at intermediate energies. A dedicated simulation was developed to study feasibility of registering such events with the required accuracy and to support the future data analysis. An additional rotation angle has been introduced to parametrise the Star configurations. First results concerning the acceptance of certain segments of BINA for registering the Star configurations are presented.pl_PL
dc.language.isoenpl_PL
dc.rightsUznanie autorstwa 3.0 Polska*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/pl/*
dc.subjectStar configurationspl_PL
dc.subjectBINA detectorpl_PL
dc.titleSimulation of Star configurations in the BINA detectorpl_PL
dc.typeinfo:eu-repo/semantics/articlepl_PL
dc.identifier.doi10.5506/APhysPolB.51.763-
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Uznanie Autorstwa 3.0 Polska Creative Commons Creative Commons