Nuclear Structure and Nuclear Astrophysics
Nuclear Structure and Nuclear Astrophysics
批准号:
1713857
负责人:
Michael Wiescher
金额:
$616.0万
依托单位:
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2017
资助国家:
美国
项目状态:
已结题
起止时间:
2017-08-15 至 2021-07-31
中文摘要
该奖项延续了圣母大学核结构物理和核天体物理领域八名教员及其学生的研究项目。该计划的重点是直接测量核反应和衰变过程,这些过程决定了恒星的生命和宇宙中元素的起源。这个程序解决了关键的核过程,定义了恒星演化和爆炸过程的时间尺度。另一个组成部分是研究超新星爆炸前恒星生命最后几天的低能聚变反应。该计划还探讨了核结构效应和弱相互作用过程,这些过程正在指导大规模核合成过程。这项研究主要是通过使用圣母大学核科学实验室(NSL)的加速器来完成的,这些加速器是通过一系列实验技术来探测恒星反应的独特设计。实验结果扩展了我们对原子核作为多体量子系统的基本结构的认识;它们还为天体物理学界提供了关于元素起源和宇宙从大爆炸到现在的化学演化的新见解。NSL拥有在大学环境中进行此类研究的独特设备。该奖项将支持大量研究生(约30人)和本科生(约20人)在实验和理论技术方面的培训,为加入国家的核劳动力做好准备。实验方案是基于在NSL使用两个加速器。来自单端5U Pelletron的强稳定离子束用于低能捕获和聚变反应的直接研究。在圣乔治反冲分离器的逆运动学技术中,重离子束被用来研究这种反应。该分离器是独一无二的,可作为FRIB SECAR分离器设计的蓝图。FN串联加速器是一种多用途仪器。它在TwinSol设施中作为产生放射性光束的驱动器运行,TwinSol设施是美国第一个产生低能放射性光束的仪器。这些光束可以直接进行反应测量,并捕获在大型国家设施中无法达到的水平的轻放射性粒子。FN还服务于NSL的加速器质谱(AMS)项目,测试地质和宇宙样品的长寿命放射性。大量的核结构实验是基于这台机器的操作,使用各种粒子和伽马能谱技术。该计划的一小部分依赖于使用其他国家和国际设施来利用NSL无法获得的更高能量束。
英文摘要
This award continues the research program of eight faculty members and their students in Nuclear Structure Physics and Nuclear Astrophysics at the University of Notre Dame. The program focuses on direct measurements of nuclear reaction and decay processes that determine the life of stars and the origin of the elements in the universe. This program addresses key nuclear processes that define the timescales of stellar evolution and explosion processes. Another component is the study of low energy fusion reactions during the last days of a stellar life prior to supernova explosion. The program also explores the nuclear structure effects and weak interaction processes that are guiding large scale nucleosynthesis processes. The research is performed primarily by using the accelerators of the Nuclear Science Laboratory (NSL) at the University of Notre Dame, which are uniquely designed to probe stellar reactions through a number of experimental techniques. The experimental results expand our knowledge of the fundamental structure of the nucleus as a multi-body quantum system; they also provide new insight for the astrophysics community on the origin of the elements and the chemical evolution of the cosmos from the Big Bang to the present. The NSL is uniquely equipped for performing this kind of research in a university environment. The award will support the training of a large number of graduate (approximately 30) and undergraduate students (approximately 20) in experimental and theoretical techniques to be ready to join the nuclear workforce of the nation. The experimental program is based on the use of two accelerators at the NSL. Intense stable ion beams from the single ended 5U Pelletron are used for the direct study of low-energy capture and fusion reactions. Heavy ion beams are used to investigate such reactions in inverse kinematic technique using the St. GEORGE recoil separator. This separator is unique and serves as blueprint for the design of the SECAR separator at FRIB. The FN tandem accelerator is used as a multi-purpose instrument. It is operated as a driver for the production of radioactive beams at the TwinSol facility, the nationss first instrument for producing low energy radioactive beams. These beams allow direct reaction measurements with and the trapping of light radioactive particles at levels not possible at large national facilities. The FN also serves the accelerator mass spectrometry (AMS) program at the NSL, testing geological and cosmological samples for long-lived radioactivities. A large number of nuclear structure experiments is based on the operation of this machine using a variety of particle and gamma spectroscopy techniques. A smaller fraction of the program relies on the use of other national and international facilities to take advantage of higher energy beams not available at the NSL.
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DOI:
10.1140/epjp/i2018-12295-3
发表时间:
2018-10
期刊:
The European Physical Journal Plus
影响因子:
--
作者:
[R. Reifarth;P. Erbacher;S. Fiebiger;K. Göbel;T. Heftrich;M. Heil;F. Käppeler;N. Klapper;D. Kurtulgil;C. Langer;C. Lederer-Woods;A. Mengoni;B. Thomas;S. Schmidt;M. Weigand;M. Wiescher]
通讯作者:
R. Reifarth;P. Erbacher;S. Fiebiger;K. Göbel;T. Heftrich;M. Heil;F. Käppeler;N. Klapper;D. Kurtulgil;C. Langer;C. Lederer-Woods;A. Mengoni;B. Thomas;S. Schmidt;M. Weigand;M. Wiescher
DOI:
10.1103/physrevc.101.064309
发表时间:
2020-03
期刊:
Physical Review C
影响因子:
3.1
作者:
[D. Puentes;G. Bollen;M. Brodeur;M. Eibach;K. Gulyuz;A. Hamaker;C. Izzo;S. Lenzi;M. Maccormick;M. Redshaw;R. Ringle;R. Sandler;S. Schwarz;P. Schury;N. Smirnova;J. Surbrook;A. Valverde;A. Villari;I. Yandow]
通讯作者:
D. Puentes;G. Bollen;M. Brodeur;M. Eibach;K. Gulyuz;A. Hamaker;C. Izzo;S. Lenzi;M. Maccormick;M. Redshaw;R. Ringle;R. Sandler;S. Schwarz;P. Schury;N. Smirnova;J. Surbrook;A. Valverde;A. Villari;I. Yandow
Stopped, bunched beams for the TwinSol facility
TwinSol 设施的停止束束
DOI:
10.1007/s10751-019-1591-x
发表时间:
2019
期刊:
Hyperfine Interactions
影响因子:
--
作者:
[Valverde, A. A., Brodeur, M., Burdette, D. P., Clark, J. A., Klimes, J. W., Lascar, D., O’Malley, P. D., Ringle, R., Savard, G., Varentsov, V.]
通讯作者:
Varentsov, V.
First off-line tests and performance of the Notre Dame multi-reflection time-of-flight mass spectrometer
巴黎圣母院多重反射飞行时间质谱仪的首次离线测试和性能
DOI:
10.1016/j.nimb.2019.04.018
发表时间:
2020
期刊:
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
影响因子:
--
作者:
[Kelly, J.M., Brodeur, M., Liu, B., Campagna, Q., Gonzales, C., Maier, J.]
通讯作者:
Maier, J.
Using 19F(3He,t)19Ne*(γ) to study astrophysically important levels near the 18F+p threshold
使用 19F(3He,t)19Ne*(γ) 研究 18F p 阈值附近的天体物理重要水平
DOI:
10.1063/1.5127732
发表时间:
2019
期刊:
AIP Conference Proceedings
影响因子:
--
作者:
[Hall, M. R., Bardayan, D. W., Ahn, S., Allen, J. M., Anderson, J. T., Ayangeakaa, A. D., Baugher, T., Blackmon, J. C., Blankstein, D., Burcher, S.]
通讯作者:
Burcher, S.
共 69 条
Underground Low-Background Nuclear Astrophysics Studies
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批准号:1913746
-
项目类别:Continuing Grant
-
资助金额:$75.0万
-
财政年份:2019
-
负责人:Michael Wiescher
-
依托单位:
Nuclear Structure and Nuclear Astrophysics
-
批准号:1419765
-
项目类别:Continuing Grant
-
资助金额:$650.0万
-
财政年份:2014
-
负责人:Michael Wiescher
-
依托单位:
DIANA, an Underground Accelerator Facility for Nuclear Astrophysics
-
批准号:1242506
-
项目类别:Standard Grant
-
资助金额:$160.05万
-
财政年份:2012
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负责人:Michael Wiescher
-
依托单位:
Nuclear Structure and Nuclear Astrophysics
-
批准号:1068192
-
项目类别:Continuing Grant
-
资助金额:$591.6万
-
财政年份:2011
-
负责人:Michael Wiescher
-
依托单位:
DIANA, A Novel Nuclear Accelerator Lab Underground
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批准号:0918728
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项目类别:Cooperative Agreement
-
资助金额:$230.0万
-
财政年份:2009
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负责人:Michael Wiescher
-
依托单位:
PFC: Joint Institute for Nuclear Astrophysics, JINA
-
批准号:0822648
-
项目类别:Cooperative Agreement
-
资助金额:$1045.0万
-
财政年份:2008
-
负责人:Michael Wiescher
-
依托单位:
MRI: Acquisition of an Accelerator for Stellar Nucleosynthesis Measurements
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批准号:0820883
-
项目类别:Standard Grant
-
资助金额:$246.44万
-
财政年份:2008
-
负责人:Michael Wiescher
-
依托单位:
Nuclear Structure and Nuclear Astrophysics
-
批准号:0758100
-
项目类别:Continuing Grant
-
资助金额:$450.0万
-
财政年份:2008
-
负责人:Michael Wiescher
-
依托单位:
Nuclear Structure and Nuclear Astrophysics
-
批准号:0457120
-
项目类别:Continuing Grant
-
资助金额:$0.0万
-
财政年份:2005
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负责人:Michael Wiescher
-
依托单位:
Joint Institute for Nuclear Astrophysics - JINA
-
批准号:0216783
-
项目类别:Cooperative Agreement
-
资助金额:$0.0万
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财政年份:2003
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负责人:Michael Wiescher
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依托单位:
Collaborative Research of the Joint Institute for Nuclear Astrophysics
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批准号:0072711
-
项目类别:Standard Grant
-
资助金额:$18.0万
-
财政年份:2001
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负责人:Michael Wiescher
-
依托单位:
Low Energy Nuclear Reactions in Late Stellar Evolution
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批准号:0099403
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项目类别:Standard Grant
-
资助金额:$15.0万
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财政年份:2001
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负责人:Michael Wiescher
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依托单位:
U.S.-Germany Cooperative Research: Alpha-Induced Reactions in Red Giants
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批准号:9815296
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项目类别:Standard Grant
-
资助金额:$1.84万
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财政年份:1999
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负责人:Michael Wiescher
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依托单位:
Study Of Low Energy Nuclear Reactions In Late Stellar Evolution
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批准号:9803757
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项目类别:Continuing Grant
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资助金额:$28.71万
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财政年份:1998
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负责人:Michael Wiescher
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依托单位:
Fourth International Symposium on Nuclei in the Cosmos
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批准号:9601426
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项目类别:Standard Grant
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资助金额:$0.4万
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财政年份:1996
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负责人:Michael Wiescher
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依托单位:
海外基金