r-process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos

doi:10.1088/1361-6471/ab0849

	r-process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos
	Horowitz, C. J.29,30,31; Arcones, A.31,32,33; Cote, B.31,34,35; Dillmann, I 31,36,37; Nazarewicz, W.34,38; Roederer, I. U.31,39; Schatz, H.31,34,40; Aprahamian, A.1,31; Atanasov, D.2; Bausweinm, A.3
刊名	JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS
	2019-08-01
卷号	46 期号:8 页码:103
关键词	nucleosynthesis rare-isotope beam facilities r-process nucleosynthesis galactic chemical evolution
ISSN号	0954-3899
DOI	10.1088/1361-6471/ab0849
通讯作者	Schatz, H.(schatz@msu.edu)
英文摘要	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.
资助项目	National Science Foundation[PHY-1102511] ; National Science Foundation[PHY-1430152] ; International Collaborations in Nuclear Theory program ; Physics Frontier Center/JINA Center for the Evolution of the Elements (JINA-CEE) - US National Science Foundation ; US Department of Energy[DOE-DE-FG02-87ER40365] ; US Department of Energy[DE-SC0018083] ; US Department of Energy[DOE-DE-NA0002847] ; US Department of Energy[DE-SC0013365] ; Helmholtz-University Young Investigator grant[VH-NG-825] ; Deutsche Forschungsgemeinschaft[SFB 1245] ; European Research Council through ERC[677912 EUROPIUM] ; Canadian NSERC Discovery Grants[SAPIN-2014-00028] ; Canadian NSERC Discovery Grants[RGPAS 462257-2014] ; IMPRS-PTFS[UNAM-DGAPA/PAPIIT IV100116] ; European Research Council under the European Unions's Seventh Framework Programme[615126] ; ERC Consolidator Grant (Hungary) funding scheme[724560] ; National Aeronautics and Space Administration (NASA)[NNX15AP39G] ; Hubble Theory Grant[HST-AR-13 261.01-A] ; NSF[AST-1514700] ; NASA through Einstein Postdoctoral Fellowship[PF4-150122] ; NASA through Einstein Postdoctoral Fellowship[NAS8-03060] ; Chinese National Key Research and Development program[MOST 2016YFA0400501] ; Chinese National Key Research and Development program[2016YFA0400504] ; National Natural Science Foundation of China[11475228] ; National Natural Science Foundation of China[11490564] ; 100 talents Program of the Chinese Academy of Sciences ; Department of Energy/National Nuclear Security Administration[DE-NA0003221] ; Department of Energy/National Nuclear Security Administration[DE-NA0003180] ; US Department of Energy through the Los Alamos National Laboratory ; National Nuclear Security Administration of US Department of Energy[DEAC52-06NA25396] ; European Research Council[ERC AdG 341157-COCO2CAS] ; Max-Planck Princeton Center for Plasma Physics (MPPC) ; US Department of Energy, Office of Nuclear Physics[DE-AC02-06CH11357] ; Academy of Finland[275389] ; Academy of Finland[284516] ; Academy of Finland[312544]
WOS关键词	NEUTRON-STAR MERGERS ; EXTREMELY METAL-POOR ; CORE-COLLAPSE SUPERNOVAE ; HIGH-DISPERSION-SPECTROGRAPH ; DIRECT MASS MEASUREMENTS ; HALF-LIFE MEASUREMENTS ; BETA COUNTING SYSTEM ; BLACK-HOLE FORMATION ; SHORT-LIVED NUCLEI ; GAMMA-RAY BURSTS
WOS研究方向	Physics
语种	英语
出版者	IOP PUBLISHING LTD
WOS记录号	WOS:000475654000001
资助机构	National Science Foundation ; International Collaborations in Nuclear Theory program ; Physics Frontier Center/JINA Center for the Evolution of the Elements (JINA-CEE) - US National Science Foundation ; US Department of Energy ; Helmholtz-University Young Investigator grant ; Deutsche Forschungsgemeinschaft ; European Research Council through ERC ; Canadian NSERC Discovery Grants ; IMPRS-PTFS ; European Research Council under the European Unions's Seventh Framework Programme ; ERC Consolidator Grant (Hungary) funding scheme ; National Aeronautics and Space Administration (NASA) ; Hubble Theory Grant ; NSF ; NASA through Einstein Postdoctoral Fellowship ; Chinese National Key Research and Development program ; National Natural Science Foundation of China ; 100 talents Program of the Chinese Academy of Sciences ; Department of Energy/National Nuclear Security Administration ; US Department of Energy through the Los Alamos National Laboratory ; National Nuclear Security Administration of US Department of Energy ; European Research Council ; Max-Planck Princeton Center for Plasma Physics (MPPC) ; US Department of Energy, Office of Nuclear Physics ; Academy of Finland
内容类型	期刊论文
源URL	[http://119.78.100.186/handle/113462/132918]
专题	中国科学院近代物理研究所
通讯作者	Schatz, H.
作者单位	1.Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA 2.Max Planck Inst Kemphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany 3.Heidelberg Inst Theoret Studies, Schloss Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany 4.Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA 5.MIT, Cambridge, MA 02139 USA 6.Univ New Hampshire, Dept Phys, Durham, NH 03824 USA 7.Univ Copenhagen, Dark Cosmol Ctr, Juliane Manes Vej 30, DK-2100 Copenhagen, Denmark 8.Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching, Germany 9.RIKEN, Astrophys Big Bang Lab, Wako, Saitama 3510198, Japan 10.Univ Jyvaskyla, POB 35, FI-40014 Jyvaskyla, Finland
推荐引用方式 GB/T 7714	Horowitz, C. J.,Arcones, A.,Cote, B.,et al. r-process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos[J]. JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS,2019,46(8):103.
APA	Horowitz, C. J..,Arcones, A..,Cote, B..,Dillmann, I.,Nazarewicz, W..,...&Wang, M..(2019).r-process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos.JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS,46(8),103.
MLA	Horowitz, C. J.,et al."r-process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos".JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS 46.8(2019):103.