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Title: Experimentally Constrained (\(n,\gamma \)) Reaction Rates Relevant to r- and i-Process Nucleosynthesis

Abstract

The element distribution that we observe in the Universe today, tells a fascinating story of nucleosynthesis events that have taken place throughout the 13.7-billion-years-long history starting with the Big Bang. It is known for a long time that radiative neutron-capture reactions play a major role in synthesizing elements heavier than iron. However, many questions remain when it comes to our understanding of neutron-capture processes in extreme stellar environments. In particular, the intermediate and rapid neutron-capture processes are very challenging to describe, as there exist little or no data on the much-needed neutron-capture rates. In this work we discuss possibilities to obtain indirect, experimental constrains on these rates by means of the Oslo and the β-Oslo methods.

Authors:
 [1];  [1];  [2];  [3]
  1. Univ. of Oslo (Norway)
  2. Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab., Joint Inst. for Nuclear Astrophysics
  3. Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab.
Publication Date:
Research Org.:
Michigan State Univ., East Lansing, MI (United States)
Sponsoring Org.:
USDOE National Nuclear Security Administration (NNSA); National Science Foundation (NSF); European Cooperation in Science and Technology
OSTI Identifier:
1657658
Grant/Contract Number:  
NA0003221; 637686; OISE-1927130; PHY 1102511; PHY 1430152; PHY 1350234
Resource Type:
Accepted Manuscript
Journal Name:
Acta Physica Polonica. Series B
Additional Journal Information:
Journal Volume: 51; Journal Issue: 3; Conference: XXXVI Mazurian Lakes Conference on Physics, Piaski (Poland), 1-7 Sep 2019; Journal ID: ISSN 0587-4254
Publisher:
Jagiellonian University
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; 73 NUCLEAR PHYSICS AND RADIATION PHYSICS

Citation Formats

Guttormsen, M., Larsen, A. C., Spyrou, A., and Liddick, S. N. Experimentally Constrained (\(n,\gamma \)) Reaction Rates Relevant to r- and i-Process Nucleosynthesis. United States: N. p., 2020. Web. doi:10.5506/aphyspolb.51.667.
Guttormsen, M., Larsen, A. C., Spyrou, A., & Liddick, S. N. Experimentally Constrained (\(n,\gamma \)) Reaction Rates Relevant to r- and i-Process Nucleosynthesis. United States. https://doi.org/10.5506/aphyspolb.51.667
Guttormsen, M., Larsen, A. C., Spyrou, A., and Liddick, S. N. Wed . "Experimentally Constrained (\(n,\gamma \)) Reaction Rates Relevant to r- and i-Process Nucleosynthesis". United States. https://doi.org/10.5506/aphyspolb.51.667. https://www.osti.gov/servlets/purl/1657658.
@article{osti_1657658,
title = {Experimentally Constrained (\(n,\gamma \)) Reaction Rates Relevant to r- and i-Process Nucleosynthesis},
author = {Guttormsen, M. and Larsen, A. C. and Spyrou, A. and Liddick, S. N.},
abstractNote = {The element distribution that we observe in the Universe today, tells a fascinating story of nucleosynthesis events that have taken place throughout the 13.7-billion-years-long history starting with the Big Bang. It is known for a long time that radiative neutron-capture reactions play a major role in synthesizing elements heavier than iron. However, many questions remain when it comes to our understanding of neutron-capture processes in extreme stellar environments. In particular, the intermediate and rapid neutron-capture processes are very challenging to describe, as there exist little or no data on the much-needed neutron-capture rates. In this work we discuss possibilities to obtain indirect, experimental constrains on these rates by means of the Oslo and the β-Oslo methods.},
doi = {10.5506/aphyspolb.51.667},
journal = {Acta Physica Polonica. Series B},
number = 3,
volume = 51,
place = {United States},
year = {Wed Jan 01 00:00:00 EST 2020},
month = {Wed Jan 01 00:00:00 EST 2020}
}

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