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:
-
- Univ. of Oslo (Norway)
- Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab., Joint Inst. for Nuclear Astrophysics
- 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}
}
Web of Science