课题基金 / 基金详情

AccelNet-WOU: International Research Network for Nuclear Astrophysics (IReNA)

AccelNet-WOU: International Research Network for Nuclear Astrophysics (IReNA)
AccelNet-WOU:国际核天体物理学研究网络 (IRENA)
批准号:
1927130
负责人:
Hendrik Schatz
金额:
$200.0万
依托单位:
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2019
资助国家:
美国
项目状态:
已结题
起止时间:
2019-10-01 至 2024-09-30

项目摘要

项目成果

Hendrik Schatz的其他基金

相似基金

相关文献

中文摘要
翻译
点击翻译按钮获取中文摘要
英文摘要
Multi-messenger astronomy, using electromagnetic radiation (radio waves, visible light, X-rays, gamma rays), neutrinos, and gravitational waves, is providing unprecedented observations of extreme astrophysical environments, such as supernovae and merging neutron stars. The diverse range of nuclear and astrophysics that needs to be synthesized to answer open questions about the universe cannot be obtained by a single country. The International Research Network for Nuclear Astrophysics (IReNA) project connects research networks and capabilities across disciplines and geographic boundaries to advance understanding of the origin of chemical elements and the nature of dense nuclear matter. This network of networks links the U.S. Joint Institute for Nuclear Astrophysics Center for the Evolution of Elements (JINA-CEE) with similar undertakings in Europe (ChETEC), Japan (UKAKUREN), Germany (EMMI and The Milky Way system), and the international NuGRID network. IReNA creates the communication channels and collaborative structures needed for rapid scientific response to new multi-messenger discoveries. Exchange programs, innovative workshops, and retreats will foster network communication and training of the next generation of scientists. Multi-messenger astronomical observation of supernovae and merging neutron stars is leading to a better understanding of and further questions on the origin of chemical elements and the physics of dense nuclear matter. For multi-messenger data to become true windows on the universe, an unprecedented amount of astrophysics and nuclear physics associated with the various messengers and their interactions must be understood. The IReNA project brings together U.S. and international networks with complementary capabilities to exchange and synthesize data, models, theory, and expertise in astrophysics and nuclear physics. The research goals are to advance our understanding of element formation in stars, stellar explosions, and neutron star mergers through new nuclear physics experiments, nuclear theory, advanced computational modeling, and new observations of the distribution of elements in stars across our Galaxy. The expanded collaborations will enable synthesis and exchange of data sets across international communities and expand capabilities far beyond what would be possible by any individual network.The Accelerating Research through International Network-to-Network Collaborations (AccelNet) program is designed to accelerate the process of scientific discovery and prepare the next generation of U.S. researchers for multiteam international collaborations. The AccelNet program supports strategic linkages among U.S. research networks and complementary networks abroad that will leverage research and educational resources to tackle grand scientific challenges that require significant coordinated international efforts.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
期刊论文(242)
专著(0)
科研奖励(0)
会议论文
The Regulated NiCu Cycles with the New 57Cu(p,gamma)58Zn Reaction Rate and Its Influence on Type I X-Ray Bursts: the GS 1826-24 Clocked Burster
新 57Cu(p,gamma)58Zn 反应速率调节的 NiCu 循环及其对 I 型 X 射线爆发的影响:GS 1826-24 时钟爆发
DOI: 10.3847/1538-4357/ac4d89
发表时间: 2022
期刊: The Astrophysical Journal
影响因子: --
作者: [Lam Yi Hua, Lu Ning, Heger Alexander, Jacobs Adam Michael, Smirnova Nadezda A., Nieto Teresa Kurtukian, Johnston Zac, Kubono Shigeru]
通讯作者: Kubono Shigeru
The Nucleosynthetic Yields of Core-collapse Supernovae: Prospects for the Next Generation of Gamma-Ray Astronomy
核心塌缩超新星的核合成产率:下一代伽马射线天文学的前景
DOI: 10.3847/1538-4357/ab64f8
发表时间: 2020
期刊: The Astrophysical Journal
影响因子: --
作者: [Andrews S]
通讯作者: Andrews S
Helium as a signature of the double detonation in Type Ia supernovae
氦作为 Ia 型超新星双重爆炸的标志
DOI: 10.1093/mnras/stad2170
发表时间: 2023
期刊: Monthly Notices of the Royal Astronomical Society
影响因子: 4.8
作者: [Collins, Christine E., Sim, Stuart A., Shingles, Luke J., Gronow, Sabrina, Röpke, Friedrich K., Pakmor, Rüdiger, Seitenzahl, Ivo R., Kromer, Markus]
通讯作者: Kromer, Markus
DOI: 10.3847/1538-4357/acd7ea
发表时间: 2023
期刊: The Astrophysical Journal
影响因子: --
作者: [Brinkman, Hannah E., Doherty, Carolyn, Pignatari, Marco, Pols, Onno, Lugaro, Maria]
通讯作者: Lugaro, Maria
101
    MRI: Development of a Separator for Capture Reactions (SECAR) Phase 2
    • 批准号:
      1624942
    • 项目类别:
      Standard Grant
    • 资助金额:
      $150.0万
    • 财政年份:
      2016
    • 负责人:
      Hendrik Schatz
    • 依托单位:
    JINA Center for the Evolution of the Elements
    • 批准号:
      1430152
    • 项目类别:
      Cooperative Agreement
    • 资助金额:
      $1140.0万
    • 财政年份:
      2014
    • 负责人:
      Hendrik Schatz
    • 依托单位:
    Development of an RF Fragment Separator at the NSCL
    • 批准号:
      0520930
    • 项目类别:
      Standard Grant
    • 资助金额:
      $25.12万
    • 财政年份:
      2005
    • 负责人:
      Hendrik Schatz
    • 依托单位:
    海外基金