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Studying Lambda interactions in nuclear matter with the 208Pb(e,e'K+)208 Lambda-tl reaction
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SYSNO ASEP 0509987 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Studying Lambda interactions in nuclear matter with the 208Pb(e,e'K+)208 Lambda-tl reaction Author(s) Garibaldi, F. (IT)
Benhar, O. (IT)
Bydžovský, Petr (UJF-V) RID, ORCID, SAI
Covrig, S. (US)
Gogami, T. (JP)
Markowitz, P. (US)
Millener, D.J. (US)
Nakamura, S. N. (JP)
Reinhold, J. (US)
Tang, L. (US)
Urciuoli, G. M. (IT)
Vidana, I. (IT)Number of authors 12 Article number 040003 Source Title AIP Conference Proceedings, 2130. - Melville : American Institute of Physics Inc., 2019 - ISSN 0094-243X - ISBN 978-0-7354-1872-1 Number of pages 9 s. Publication form Print - P Action 13th International Conference on Hypernuclear and Strange Particle Physics Event date 24.06.2018 - 29.06.2018 VEvent location Portsmouth Country US - United States Event type WRD Language eng - English Country US - United States Keywords hypernuclei ; neutron stars ; hyperons Subject RIV BE - Theoretical Physics OECD category Atomic, molecular and chemical physics (physics of atoms and molecules including collision, interaction with radiation, magnetic resonances, Mössbauer effect) Institutional support UJF-V - RVO:61389005 UT WOS 000557835700032 EID SCOPUS 85070286219 DOI 10.1063/1.5118400 Annotation The hyperon puzzle, the observation that the two-solar-mass neutron stars existence is hardly explained by all models predicting the appearance of hyperons in the neutron star core is currently one of the unsolved key issues in the physics of compact stars. An experimental study of the reaction (e,e′K) on 40Ca 48Ca nuclei to study the isospin dependence of hyperon dynamics has been proposed, by the Jefferson lab hypernuclear collaboration, and approved by the Jefferson Lab (JLab) PAC. This paper describes a proposal to make a complementary study by extending it to 208Pb, whose properties largely reflects those of the uniform nuclear matter present in the interior of the neutron stars making it the ideal one for this task. Workplace Nuclear Physics Institute Contact Markéta Sommerová, sommerova@ujf.cas.cz, Tel.: 266 173 228 Year of Publishing 2020
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