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CAREER: WoU-MMA: PeVatrons and Beyond: Tackling the Century-old Problem with the New Messengers

CAREER: WoU-MMA: PeVatrons and Beyond: Tackling the Century-old Problem with the New Messengers
职业生涯:WoU-MMA:PeVatrons 及其他:用新使者解决百年问题
批准号:
2238916
负责人:
Ke Fang
金额:
$79.54万
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2023
资助国家:
美国
项目状态:
未结题
起止时间:
2023-09-01 至 2028-08-31

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中文摘要
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英文摘要
Cosmic rays are charged particles composed of protons, helium, and heavier elements that travel at nearly the speed of light. They may carry energy above 1 Peta-electronvolt (PeV), well beyond the reach of man-made accelerators. A cosmic-ray source capable of accelerating protons up to the PeV energy is called a “PeVatron”. The nature of PeVatrons is among the most fundamental questions in Particle Astrophysics. This program aims to advance our understanding of PeVatrons through observational and theoretical studies. The research will be connected to educational outreach through activities including: (1) hosting a series of inter-disciplinary discussion events that serve as a bridge in connecting research areas in the physics, astronomy, and statistics programs at the PI’s institution; (2) engaging high school students in Madison, WI and nearby regions in hands-on classes that show how scientists use modern techniques to solve complicated physics problems; and (3) conducting outreach and mentoring activities to involve students from groups that have been traditionally underrepresented in science. The team will analyze data from the IceCube Neutrino Observatory (IceCube) and the High-Altitude Water Cherenkov Gamma-ray Observatory (HAWC) using an efficient joint-analysis framework and new source-finding algorithms. They will also research the theory of cosmic ray sources by numerically simulating particle transport and interaction in cosmic environments.The award is aligned with the NSF Big Idea of Windows on the Universe: the Era of Multi-messenger Astrophysics as it coordinates the use of multi-messengers observations utilizing high energy gamma rays from HAWC with high energy neutrinos from IceCube and will improve theoretical modeling to better interpret the data.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.
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WoU-MMA: Galactic Gamma-Ray Astrophysics with HAWC (UW-Madison Group Grant)
  • 批准号:
    2110821
  • 项目类别:
    Standard Grant
  • 资助金额:
    $47.06万
  • 财政年份:
    2021
  • 负责人:
    Ke Fang
  • 依托单位:
海外基金