r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos
Abstract
This is an exciting time for the study of r-process nucleosynthesis. Recently, a neutron star merger GW170817 was observed in extraordinary detail with gravitational waves and electromagnetic radiation from radio to gamma rays. The very red color of the associated kilonova suggests that neutron star mergers are an important r-process site. Astrophysical simulations of neutron star mergers and core collapse supernovae are making rapid progress. Detection of both electron neutrinos and antineutrinos from the next galactic supernova will constrain the composition of neutrino-driven winds and provide unique nucleosynthesis information. Finally, FRIB and other rare-isotope beam facilities will soon have dramatic new capabilities to synthesize many neutron-rich nuclei that are involved in the r-process. The new capabilities can significantly improve our understanding of the r-process and likely resolve one of the main outstanding problems in classical nuclear astrophysics. However, to make best use of the new experimental capabilities and to fully interpret the results, a great deal of infrastructure is needed in many related areas of astronomy, astrophysics, and nuclear theory. We place these experiments in context by discussing astrophysical simulations and observations of r-process sites, observations of stellar abundances, galactic chemical evolution, and nuclear theory for the structure and reactionsmore »
- Authors:
-
more »
- Indiana Univ., Bloomington, IN (United States)
- Technical Univ. of Darmstadt (Germany)
- Hungarian Academy of Sciences (MTA), Budapest (Hungary)
- TRIUMF, Vancouver, BC (Canada)
- Michigan State Univ., East Lansing, MI (United States)
- Univ. of Michigan, Ann Arbor, MI (United States)
- Univ. of Notre Dame, IN (United States)
- European Organization for Nuclear Research (CERN), Geneva (Switzerland)
- Heidelberg Inst. for Theoretical Studies (HITS gGmbH) (Germany)
- Argonne National Lab. (ANL), Argonne, IL (United States)
- Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
- Univ. of New Hampshire, Durham, NH (United States)
- Univ. of Copenhagen (Denmark)
- RIKEN, Wako (Japan)
- Univ. of Jyvaskyla (Finland)
- North Carolina State Univ., Raleigh, NC (United States)
- Vanderbilt Univ., Nashville, TN (United States)
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Univ. of Veracruz, Xalapa, Veracruz (Mexico)
- Columbia Univ., New York, NY (United States)
- Univ. of Notre Dame, IN (United States); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Central Michigan Univ., Mount Pleasant, MI (United States)
- Goethe Univ., Frankfurt (Germany)
- Univ. of Massachusetts, Lowell, MA (United States)
- Chinese Academy of Sciences (CAS), Lanzhou, Gansu (China)
- Publication Date:
- Research Org.:
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States); Argonne National Lab. (ANL), Argonne, IL (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA), Office of Defense Nuclear Nonproliferation; USDOE Office of Science (SC), Nuclear Physics (NP)
- OSTI Identifier:
- 1525822
- Alternate Identifier(s):
- OSTI ID: 1574224
- Report Number(s):
- LA-UR-18-22069
Journal ID: ISSN 0954-3899
- Grant/Contract Number:
- 89233218CNA000001; SC0013365; NA0002847; SC0018083; FG02-87ER40365; AC02-06CH11357
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Physics. G, Nuclear and Particle Physics
- Additional Journal Information:
- Journal Volume: 46; Journal Issue: 8; Journal ID: ISSN 0954-3899
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; galactic chemical evolution; nucleosynthesis; r-process nucleosynthesis; rare-isotope beam facilities
Citation Formats
Horowitz, Charles J., Arcones, Almudena, Cote, Benoit, Dillmann, Iris, Nazarewicz, Witold, Roederer, Ian, Schatz, Hendrik, Aprahamian, Ani, Atanasov, Dinko, Bauswein, Andreas, Beers, T. C., Bliss, Julia, Brodeur, Maxime, Clark, Jason, Frebel, Anna, Foucart, Francois, Hansen, Camilla, Just, Oliver, Kankainen, Anu, McLaughlin, Gail, Kelly, James, Liddick, Sean, Lee, Duane, Lippuner, Jonas, Martin, Dirk, Mendoza-Temis, Joel, Metzger, Brian T., Mumpower, Matthew, Perdikakis, Georgios, Pereira, Jorge, O'Shea, Brian, Reifarth, Rene, Rogers, Andy, Siegel, Daniel, Spyrou, Artemis, Surman, Rebecca, Tang, Xiao-Dong, Uesaka, Tomohiro, and Wang, Meng. r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos. United States: N. p., 2019.
Web. doi:10.1088/1361-6471/ab0849.
Horowitz, Charles J., Arcones, Almudena, Cote, Benoit, Dillmann, Iris, Nazarewicz, Witold, Roederer, Ian, Schatz, Hendrik, Aprahamian, Ani, Atanasov, Dinko, Bauswein, Andreas, Beers, T. C., Bliss, Julia, Brodeur, Maxime, Clark, Jason, Frebel, Anna, Foucart, Francois, Hansen, Camilla, Just, Oliver, Kankainen, Anu, McLaughlin, Gail, Kelly, James, Liddick, Sean, Lee, Duane, Lippuner, Jonas, Martin, Dirk, Mendoza-Temis, Joel, Metzger, Brian T., Mumpower, Matthew, Perdikakis, Georgios, Pereira, Jorge, O'Shea, Brian, Reifarth, Rene, Rogers, Andy, Siegel, Daniel, Spyrou, Artemis, Surman, Rebecca, Tang, Xiao-Dong, Uesaka, Tomohiro, & Wang, Meng. r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos. United States. https://doi.org/10.1088/1361-6471/ab0849
Horowitz, Charles J., Arcones, Almudena, Cote, Benoit, Dillmann, Iris, Nazarewicz, Witold, Roederer, Ian, Schatz, Hendrik, Aprahamian, Ani, Atanasov, Dinko, Bauswein, Andreas, Beers, T. C., Bliss, Julia, Brodeur, Maxime, Clark, Jason, Frebel, Anna, Foucart, Francois, Hansen, Camilla, Just, Oliver, Kankainen, Anu, McLaughlin, Gail, Kelly, James, Liddick, Sean, Lee, Duane, Lippuner, Jonas, Martin, Dirk, Mendoza-Temis, Joel, Metzger, Brian T., Mumpower, Matthew, Perdikakis, Georgios, Pereira, Jorge, O'Shea, Brian, Reifarth, Rene, Rogers, Andy, Siegel, Daniel, Spyrou, Artemis, Surman, Rebecca, Tang, Xiao-Dong, Uesaka, Tomohiro, and Wang, Meng. Fri .
"r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos". United States. https://doi.org/10.1088/1361-6471/ab0849. https://www.osti.gov/servlets/purl/1525822.
@article{osti_1525822,
title = {r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos},
author = {Horowitz, Charles J. and Arcones, Almudena and Cote, Benoit and Dillmann, Iris and Nazarewicz, Witold and Roederer, Ian and Schatz, Hendrik and Aprahamian, Ani and Atanasov, Dinko and Bauswein, Andreas and Beers, T. C. and Bliss, Julia and Brodeur, Maxime and Clark, Jason and Frebel, Anna and Foucart, Francois and Hansen, Camilla and Just, Oliver and Kankainen, Anu and McLaughlin, Gail and Kelly, James and Liddick, Sean and Lee, Duane and Lippuner, Jonas and Martin, Dirk and Mendoza-Temis, Joel and Metzger, Brian T. and Mumpower, Matthew and Perdikakis, Georgios and Pereira, Jorge and O'Shea, Brian and Reifarth, Rene and Rogers, Andy and Siegel, Daniel and Spyrou, Artemis and Surman, Rebecca and Tang, Xiao-Dong and Uesaka, Tomohiro and Wang, Meng},
abstractNote = {This is an exciting time for the study of r-process nucleosynthesis. Recently, a neutron star merger GW170817 was observed in extraordinary detail with gravitational waves and electromagnetic radiation from radio to gamma rays. The very red color of the associated kilonova suggests that neutron star mergers are an important r-process site. Astrophysical simulations of neutron star mergers and core collapse supernovae are making rapid progress. Detection of both electron neutrinos and antineutrinos from the next galactic supernova will constrain the composition of neutrino-driven winds and provide unique nucleosynthesis information. Finally, FRIB and other rare-isotope beam facilities will soon have dramatic new capabilities to synthesize many neutron-rich nuclei that are involved in the r-process. The new capabilities can significantly improve our understanding of the r-process and likely resolve one of the main outstanding problems in classical nuclear astrophysics. However, to make best use of the new experimental capabilities and to fully interpret the results, a great deal of infrastructure is needed in many related areas of astronomy, astrophysics, and nuclear theory. We place these experiments in context by discussing astrophysical simulations and observations of r-process sites, observations of stellar abundances, galactic chemical evolution, and nuclear theory for the structure and reactions of very neutron-rich nuclei. This review paper was initiated at a three-week International Collaborations in Nuclear Theory program in June 2016, where we explored promising r-process experiments and discussed their likely impact, and their astronomical, astrophysical, and nuclear theory context.},
doi = {10.1088/1361-6471/ab0849},
journal = {Journal of Physics. G, Nuclear and Particle Physics},
number = 8,
volume = 46,
place = {United States},
year = {2019},
month = {7}
}
Web of Science
Figures / Tables:

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Preparing isomerically pure beams of short-lived nuclei at JYFLTRAP
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Trap-assisted separation of nuclear states for gamma-ray spectroscopy: the example of 100 Nb
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Systematics of Isotope Production with Radioactive Beams
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