Dark Matter and Neutrino Physics with Cryogenic Detectors

使用低温探​​测器的暗物质和中微子物理

基本信息

项目摘要

Multiple astronomical observations have established that about 85% of the matter in the universe is not made of known particles. Deciphering the nature of this so-called Dark Matter is of fundamental importance to cosmology, astrophysics, and high-energy particle physics. A leading hypothesis is that it is comprised of Weakly Interacting Massive Particles, or WIMPs, that were produced moments after the Big Bang. If WIMPs are the dark matter, then their presence in our galaxy may be detectable via scattering from atomic nuclei in detectors located deep underground to help reject backgrounds due to cosmic rays.The Cryogenic Dark Matter Search (CDMS) Collaboration has pioneered the use of low temperature phonon-mediated detectors to detect the rare scattering of WIMPs on nuclei and distinguish them from backgrounds. This work will have a broad impact which extends beyond the dark matter search. The technical developments will further advance phonon-mediated detectors, which have already found many applications in science and technology.This award will provide funds for three activities:-- The SuperCDMS Soudan experiment is currently taking data which will have world-leading sensitivity to dark matter for masses below 5 gigaelectronvolt (GeV). The experiment will continue taking data next year, and the full set of different analyses of the data will take place over the next two years. MIT has taken a leadership role in the low-threshold analysis, and will continue to do so. -- Play a central role in the design, prototyping, testing, and commissioning of the next-generation experiment. -- Develop and prototype new low-threshold, low-background detectors with enough sensitivity to cover all the available dark matter parameter space for masses between 1-10 GeV down to the irreducible background from solar neutrinos.This award will contribute to the training of undergraduate and graduate students and postdoctoral researchers, continuing the group's strong involvement in mentoring undergraduates from underrepresented groups by participating in the MIT Summer Research Program.
多次天文观察结果表明,宇宙中约有85%的物质不是由已知粒子制成的。破译这种所谓的暗物质的性质对于宇宙学,天体物理学和高能粒子物理学至关重要。一个主要的假设是,它由弱相互作用的巨大颗粒或wimps组成,这些颗粒或wimps是在大爆炸后瞬间产生的。 If WIMPs are the dark matter, then their presence in our galaxy may be detectable via scattering from atomic nuclei in detectors located deep underground to help reject backgrounds due to cosmic rays.The Cryogenic Dark Matter Search (CDMS) Collaboration has pioneered the use of low temperature phonon-mediated detectors to detect the rare scattering of WIMPs on nuclei and distinguish them from backgrounds.这项工作将产生广泛的影响,超出了暗物质搜索。技术发展将进一步推进声子介导的检测器,这些探测器已经在科学和技术中找到了许多应用。该奖项将为三项活动提供资金: - SuperCDMS Soudan实验目前正在获取数据,这些数据将对低于5 gigaelectronvolt(GEV)(GEV)的群众具有世界领先的敏感性。该实验将在明年继续获取数据,并且将在未来两年内进行全套数据分析。麻省理工学院在低阈值分析中扮演了领导角色,并将继续这样做。 - 在下一代实验的设计,原型制作,测试和调试中发挥核心作用。 -- Develop and prototype new low-threshold, low-background detectors with enough sensitivity to cover all the available dark matter parameter space for masses between 1-10 GeV down to the irreducible background from solar neutrinos.This award will contribute to the training of undergraduate and graduate students and postdoctoral researchers, continuing the group's strong involvement in mentoring undergraduates from underrepresented groups by participating in the麻省理工学院夏季研究计划。

项目成果

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Enectali Figueroa-Feliciano其他文献

Enectali Figueroa-Feliciano的其他文献

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{{ truncateString('Enectali Figueroa-Feliciano', 18)}}的其他基金

Q-Array Deployment and Science Analysis for the Ricochet Experiment
跳弹实验的 Q 阵列部署和科学分析
  • 批准号:
    2209585
  • 财政年份:
    2022
  • 资助金额:
    $ 33.75万
  • 项目类别:
    Standard Grant
Collaborative Research: The SuperCDMS at SNOLAB Science Program
合作研究:SNOLAB 科学计划的 SuperCDMS
  • 批准号:
    2111324
  • 财政年份:
    2021
  • 资助金额:
    $ 33.75万
  • 项目类别:
    Continuing Grant
Low-Threshold Modular Detectors for Coherent Elastic Neutrino-Nucleus Scattering
用于相干弹性中微子核散射的低阈值模块化探测器
  • 批准号:
    2013203
  • 财政年份:
    2020
  • 资助金额:
    $ 33.75万
  • 项目类别:
    Continuing Grant
Collaborative Research: The SuperCDMS SNOLAB Experiment
合作研究:SuperCDMS SNOLAB 实验
  • 批准号:
    1809730
  • 财政年份:
    2018
  • 资助金额:
    $ 33.75万
  • 项目类别:
    Continuing Grant
SuperCDMS SNOLAB: Calibration, Commissioning, and Beyond
SuperCDMS SNOLAB:校准、调试及其他
  • 批准号:
    1708153
  • 财政年份:
    2017
  • 资助金额:
    $ 33.75万
  • 项目类别:
    Standard Grant
Dark Matter and Neutrino Physics with Cryogenic Detectors
使用低温探​​测器的暗物质和中微子物理
  • 批准号:
    1550658
  • 财政年份:
    2015
  • 资助金额:
    $ 33.75万
  • 项目类别:
    Continuing Grant
CAREER: Increasing the Dark Matter Science Reach of the SuperCDMS Experiment
事业:扩大 SuperCDMS 实验的暗物质科学范围
  • 批准号:
    0847342
  • 财政年份:
    2009
  • 资助金额:
    $ 33.75万
  • 项目类别:
    Continuing Grant

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Probing matter-antimatter asymmetry with the muon electric dipole moment
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    U1435211
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    2014
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Dark matter searches and neutrino measurements with the DarkSide-20k experiment
使用 DarkSide-20k 实验进行暗物质搜索和中微子测量
  • 批准号:
    2904779
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    2023
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    $ 33.75万
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    Studentship
Unified Solutions of Neutrino Mass, Dark Matter and Experimental Anomalies by Scalar Extension
中微子质量、暗物质和实验异常的标量扩展统一解
  • 批准号:
    22KF0238
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    2023
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    $ 33.75万
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    Grant-in-Aid for JSPS Fellows
Explorations in Dark Matter and Neutrino Physics
暗物质和中微子物理探索
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    2310224
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Direct Dark Matter Searches and Neutrino Detection with the LZ Dark Mattr Experiment
通过 LZ 暗物质实验进行直接暗物质搜索和中微子探测
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    2782587
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Measuring Dark Matter, Neutral Hydrogen and Neutrino Mass with Next Generation Weak Lensing and Radio Data
使用下一代弱透镜和无线电数据测量暗物质、中性氢和中微子质量
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