Nucleosynthesis in relation to cosmology

dc.contributor.authorEl-Eid, Mounib F.
dc.contributor.departmentDepartment of Physics
dc.contributor.facultyFaculty of Arts and Sciences (FAS)
dc.contributor.institutionAmerican University of Beirut
dc.date.accessioned2025-01-24T11:25:08Z
dc.date.available2025-01-24T11:25:08Z
dc.date.issued2018
dc.description.abstractWhile the primordial (or Big Bang) nucleosynthesis delivers important clues about the conditions in the high red-shift universe (termed far-field cosmology), the nucleosynthesis of the heavy elements beyond iron by the r-process or the s-process deliver information about the early phase and history of the Galaxy (termed near-field cosmology). In particular, the r-process nucleosynthesis is unique, because it is a primary process that helps to associate individual stars with the composition of the protocloud. The present contribution is intended to give a brief overview about these nucleosynthesis processes and describe their link to the early universe, stellar evolution and to the chemical evolution of the Galaxy. The focus of this present contribution is on illumination the role of nucleosynthesis in the Universe. Owing to the complexity of this subject, a general scenario is more appealing to address interested readers. © 2018 IOP Publishing Ltd.
dc.identifier.doihttps://doi.org/10.1088/1402-4896/aaac69
dc.identifier.eid2-s2.0-85044252194
dc.identifier.urihttp://hdl.handle.net/10938/26225
dc.language.isoen
dc.publisherInstitute of Physics Publishing
dc.relation.ispartofPhysica Scripta
dc.sourceScopus
dc.subjectCosmology
dc.subjectEarly universes
dc.subjectNucleosytnthesis
dc.subjectStellar evolution
dc.subjectGalaxies
dc.subjectNucleosynthesis
dc.subjectStars
dc.subjectChemical evolution
dc.subjectEarly universe
dc.subjectHeavy elements
dc.subjectNear fields
dc.subjectR-process
dc.subjectR-process nucleosynthesis
dc.subjectStellar evolutions
dc.subjectChemical elements
dc.titleNucleosynthesis in relation to cosmology
dc.typeArticle

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