Rare Event Searches at MIT
Rare Event Searches at MIT
批准号:
2110720
负责人:
Lindley Winslow
金额:
$77.1万
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2021
资助国家:
美国
项目状态:
已结题
起止时间:
2021-08-01 至 2024-07-31
中文摘要
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英文摘要
The nature of dark matter is one of the great mysteries of physics. Second only to this is the mystery of the universe’s observed matter-antimatter asymmetry. Axions and Majorana neutrinos, respectively, are as-yet undiscovered particles which may participate in providing the answers. Axions are a well-motivated dark matter candidate while Majorana neutrinos can produce the matter antimatter asymmetry of the universe through a process called leptogenesis. Rare-event searches are the only feasible techniques to explore these models. For this reason, the types of experiments are the highest priority for particle and nuclear physics, respectively. This award will support two efforts: the search for micro-eV axions with ABRACADABRA and DMRadio, and the neutrinoless double-beta decay (0νββ) search KamLAND-Zen. These efforts build on the expertise within the MIT group, and both experimental efforts use novel multidisciplinary techniques from deep learning to quantum sensing.The broader impacts are two-fold: the development of robust vibration isolation for cryogenic experiments and the training of the next generation of scientists. This award will bring together disparate communities from gravitational wave detection to 0νββ for a workshop on vibration isolation. Undergraduate research is a priority for the PI since it is critical for recruiting and retaining physics students. This award will sponsor a study of undergraduate research at MIT and the development of best practices to engage a diverse group of students in STEM fields.The string and QCD axion models motivate a search for Axion dark matter with masses below 10^−6 eV. The ABRACADABRA and Dark Matter Radio experiments have joined forces to probe this mass-range as the DMRadio experiment. This is a staged program that builds on the success of ABRA-10 cm, expands to DMRadio-50L to test the resonant readout, then moves to higher frequencies at the m^3-scale to search down to the QCD axion. Neutrinoless double beta decay is sought in the KamLAND-Zen experiment. Deep learning techniques will be used for training and benchmarking the search algorithm. The tuning of the KLZ detector is non-trivial because many of the Monte Carlo (MC) inputs have the same gross effect and the experiments are tuning on minor deviations of the light curves in various dimensions. The group is exploring generative adversarial networks (GAN) as a way to tackle this problem. The main use of GANs is the generation of artificial images. The adversarial network is good at picking up many small features to increase the accuracy of the classifier for candidate rare events.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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Measurement of cosmic-ray muon spallation products in a xenon-loaded liquid scintillator with KamLAND
使用 KamLAND 测量载氙液体闪烁体中的宇宙射线 μ 子散裂产物
DOI:
10.1103/physrevc.107.054612
发表时间:
2023
期刊:
Physical Review C
影响因子:
3.1
作者:
[Abe, S., Asami, S., Eizuka, M., Futagi, S., Gando, A., Gando, Y., Gima, T., Goto, A., Hachiya, T., Hata, K.]
通讯作者:
Hata, K.
DOI:
10.3847/1538-4357/ac32c1
发表时间:
2021-08
期刊:
The Astrophysical Journal
影响因子:
--
作者:
[S. Abe;S. Asami;A. Gando;Y. Gando;T. Gima;A. Goto;T. Hachiya;K. Hata;S. Hayashida;K. Hosokawa;K. Ichimura;S. Ieki;H. Ikeda;K. Inoue;K. Ishidoshiro;Y. Kamei;N. Kawada;T. Kinoshita;Y. Kishimoto;M. Koga;N. Maemura;T. Mitsui;H. Miyake;K. Nakamura;R. Nakamura;H. Ozaki;T. Sakai;H. Sambonsugi;I. Shimizu;J. Shirai;K. Shiraishi;A. Suzuki;Y. Suzuki;A. Takeuchi;K. Tamae;K. Ueshima;Y. Wada;H. Watanabe;Y. Yoshida;Shuhei Obara;A. Ichikawa;A. Kozkov;D. Chernyak;Y. Takemoto;S. Yoshida;S. Umehara;K. Fushimi;S. Hirata;K. Nakamura;M. Yoshida;B. Berger;B. Fujikawa;J. Learned;J. Maricic;S. Axani;Z. Fu;J. Ouellet;L. Winslow;Y. Efremenko;H. Karwowski;D. Markoff;W. Tornow;A. Li;J. Detwiler;S. Enomoto;M. Decowski;C. Grant;S. Dell’Oro;T. O’Donnell]
通讯作者:
S. Abe;S. Asami;A. Gando;Y. Gando;T. Gima;A. Goto;T. Hachiya;K. Hata;S. Hayashida;K. Hosokawa;K. Ichimura;S. Ieki;H. Ikeda;K. Inoue;K. Ishidoshiro;Y. Kamei;N. Kawada;T. Kinoshita;Y. Kishimoto;M. Koga;N. Maemura;T. Mitsui;H. Miyake;K. Nakamura;R. Nakamura;H. Ozaki;T. Sakai;H. Sambonsugi;I. Shimizu;J. Shirai;K. Shiraishi;A. Suzuki;Y. Suzuki;A. Takeuchi;K. Tamae;K. Ueshima;Y. Wada;H. Watanabe;Y. Yoshida;Shuhei Obara;A. Ichikawa;A. Kozkov;D. Chernyak;Y. Takemoto;S. Yoshida;S. Umehara;K. Fushimi;S. Hirata;K. Nakamura;M. Yoshida;B. Berger;B. Fujikawa;J. Learned;J. Maricic;S. Axani;Z. Fu;J. Ouellet;L. Winslow;Y. Efremenko;H. Karwowski;D. Markoff;W. Tornow;A. Li;J. Detwiler;S. Enomoto;M. Decowski;C. Grant;S. Dell’Oro;T. O’Donnell
DOI:
10.1103/physrevd.107.072006
发表时间:
2022-11
期刊:
Physical Review D
影响因子:
5
作者:
[K. Abe;S. Asami;M. Eizuka;S. Futagi;A. Gando;Y. Gando;T. Gima;A. Goto;T. Hachiya;K. Hata;K. Ichimura;S. Ieki;H. Ikeda;K. Inoue;K. Ishidoshiro;Y. Kamei;N. Kawada;Y. Kishimoto;M. Koga;M. Kurasawa;T. Mitsui;H. Miyake;T. Nakahata;K. Nakamura;R. Nakamura;H. Ozaki;T. Sakai;I. Shimizu;J. Shirai;K. Shiraishi;A. Suzuki;Y. Suzuki;A. Takeuchi;K. Tamae;H. Watanabe;Y. Yoshida;Shuhei Obara;A. Ichikawa;S. Yoshida;S. Umehara;K. Fushimi;K. Kotera;Y. Urano;B. Berger;B. Fujikawa;J. Learned;J. Maricic;S. Axani;Z. Fu;J. Smolsky;L. Winslow;Y. Efremenko;H. Karwowski;D. Markoff;W. Tornow;J. Detwiler;S. Enomoto;M. Decowski;C. Grant;A. Li;H. Song;S. Dell’Oro;T. O’Donnell]
通讯作者:
K. Abe;S. Asami;M. Eizuka;S. Futagi;A. Gando;Y. Gando;T. Gima;A. Goto;T. Hachiya;K. Hata;K. Ichimura;S. Ieki;H. Ikeda;K. Inoue;K. Ishidoshiro;Y. Kamei;N. Kawada;Y. Kishimoto;M. Koga;M. Kurasawa;T. Mitsui;H. Miyake;T. Nakahata;K. Nakamura;R. Nakamura;H. Ozaki;T. Sakai;I. Shimizu;J. Shirai;K. Shiraishi;A. Suzuki;Y. Suzuki;A. Takeuchi;K. Tamae;H. Watanabe;Y. Yoshida;Shuhei Obara;A. Ichikawa;S. Yoshida;S. Umehara;K. Fushimi;K. Kotera;Y. Urano;B. Berger;B. Fujikawa;J. Learned;J. Maricic;S. Axani;Z. Fu;J. Smolsky;L. Winslow;Y. Efremenko;H. Karwowski;D. Markoff;W. Tornow;J. Detwiler;S. Enomoto;M. Decowski;C. Grant;A. Li;H. Song;S. Dell’Oro;T. O’Donnell
Proposal for a definitive search for GUT-scale QCD axions
关于明确搜索 GUT 规模 QCD 轴子的提案
DOI:
10.1103/physrevd.106.112003
发表时间:
2022
期刊:
Physical Review D
影响因子:
5
作者:
[Brouwer, L., Chaudhuri, S., Cho, H.-M., Corbin, J., Dawson, C. S., Droster, A., Foster, J. W., Fry, J. T., Graham, P. W., Henning, R.]
通讯作者:
Henning, R.
Search for Low-Mass Axion Dark Matter with ABRACADABRA-10 cm
使用 ABRACADABRA-10 cm 搜索低质量轴子暗物质
DOI:
10.1103/physrevlett.127.081801
发表时间:
2021
期刊:
Physical Review Letters
影响因子:
8.6
作者:
[Salemi, Chiara P., Foster, Joshua W., Ouellet, Jonathan L., Gavin, Andrew, Pappas, Kaliroë M. W., Cheng, Sabrina, Richardson, Kate A., Henning, Reyco, Kahn, Yonatan, Nguyen, Rachel]
通讯作者:
Nguyen, Rachel
共 11 条
WoU-MMA: Collaborative Research: Advancing the SuperNova Early Warning System
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批准号:2209120
-
项目类别:Standard Grant
-
资助金额:$6.79万
-
财政年份:2022
-
负责人:Lindley Winslow
-
依托单位:
WoU-MMA: Collaborative Research: A Next-Generation SuperNova Early Warning System for Multimessenger Astronomy
-
批准号:1914418
-
项目类别:Standard Grant
-
资助金额:$31.89万
-
财政年份:2019
-
负责人:Lindley Winslow
-
依托单位:
Rare Event Searches at MIT
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批准号:1806440
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项目类别:Continuing Grant
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资助金额:$70.0万
-
财政年份:2018
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负责人:Lindley Winslow
-
依托单位:
EAGER: A Broadband Approach to Cosmic Axion Detection
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批准号:1658693
-
项目类别:Standard Grant
-
资助金额:$12.3万
-
财政年份:2016
-
负责人:Lindley Winslow
-
依托单位:
CAREER: Next-Generation Liquid Scintillator Detectors: Picosecond Timing and Quantum-Dot-Doped Scintillator
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批准号:1554875
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项目类别:Continuing Grant
-
资助金额:$78.42万
-
财政年份:2015
-
负责人:Lindley Winslow
-
依托单位:
CAREER: Next-Generation Liquid Scintillator Detectors: Picosecond Timing and Quantum-Dot-Doped Scintillator
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批准号:1352116
-
项目类别:Continuing Grant
-
资助金额:$79.36万
-
财政年份:2014
-
负责人:Lindley Winslow
-
依托单位:
国内基金
海外基金
甲醇合成汽油工艺中烯烃催化聚合过程的单元步骤(single event)微动力学理论研究
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批准号:21306143
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项目类别:青年科学基金项目
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资助金额:25.0万元
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批准年份:2013
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负责人:金放
-
依托单位: