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The s Process and Beyond.

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Title: The s Process and Beyond.
Authors: Lugaro, Maria1,2,3,4 (AUTHOR) maria.lugaro@csfk.org, Pignatari, Marco1,2,5,6 (AUTHOR), Reifarth, René7,8 (AUTHOR), Wiescher, Michael6,8 (AUTHOR)
Source: Annual Review of Nuclear & Particle Science. 2023, Vol. 73, p315-340. 22p.
Abstract: Neutron captures produce the vast majority of abundances of elements heavier than iron in the Universe. Beyond the classical slow (s) and rapid (r) processes, there is observational evidence for neutron-capture processes that operate at neutron densities in between, at different distances from the valley of β stability. Here, we review the main properties of the s process within the general context of neutron-capture processes and the nuclear physics input required to investigate it. We describe massive stars and asymptotic giant branch stars as the s-process astrophysical sites and discuss the related physical uncertainties. We also present current observational evidence for the s process and beyond, which ranges from stellar spectroscopic observations to laboratory analysis of meteorites. [ABSTRACT FROM AUTHOR]
Copyright of Annual Review of Nuclear & Particle Science is the property of Annual Reviews Inc. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
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Header DbId: egs
DbLabel: Engineering Source
An: 172334057
AccessLevel: 6
PubType: Academic Journal
PubTypeId: academicJournal
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  Data: The s Process and Beyond.
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  Data: <searchLink fieldCode="AR" term="%22Lugaro%2C+Maria%22">Lugaro, Maria</searchLink><relatesTo>1,2,3,4</relatesTo> (AUTHOR)<i> maria.lugaro@csfk.org</i><br /><searchLink fieldCode="AR" term="%22Pignatari%2C+Marco%22">Pignatari, Marco</searchLink><relatesTo>1,2,5,6</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Reifarth%2C+René%22">Reifarth, René</searchLink><relatesTo>7,8</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Wiescher%2C+Michael%22">Wiescher, Michael</searchLink><relatesTo>6,8</relatesTo> (AUTHOR)
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  Data: <searchLink fieldCode="JN" term="%22Annual+Review+of+Nuclear+%26+Particle+Science%22">Annual Review of Nuclear & Particle Science</searchLink>. 2023, Vol. 73, p315-340. 22p.
– Name: Abstract
  Label: Abstract
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  Data: Neutron captures produce the vast majority of abundances of elements heavier than iron in the Universe. Beyond the classical slow (s) and rapid (r) processes, there is observational evidence for neutron-capture processes that operate at neutron densities in between, at different distances from the valley of β stability. Here, we review the main properties of the s process within the general context of neutron-capture processes and the nuclear physics input required to investigate it. We describe massive stars and asymptotic giant branch stars as the s-process astrophysical sites and discuss the related physical uncertainties. We also present current observational evidence for the s process and beyond, which ranges from stellar spectroscopic observations to laboratory analysis of meteorites. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of Annual Review of Nuclear & Particle Science is the property of Annual Reviews Inc. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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RecordInfo BibRecord:
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    Identifiers:
      – Type: doi
        Value: 10.1146/annurev-nucl-102422-080857
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      – Code: eng
        Text: English
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        PageCount: 22
        StartPage: 315
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      – TitleFull: The s Process and Beyond.
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            NameFull: Lugaro, Maria
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            NameFull: Pignatari, Marco
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            NameFull: Reifarth, René
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            NameFull: Wiescher, Michael
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            – D: 01
              M: 09
              Text: 2023
              Type: published
              Y: 2023
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              Value: 73
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            – TitleFull: Annual Review of Nuclear & Particle Science
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