Consolidated Grant New Applicant Scheme (The study of elementary particles and their interactions - ST/N000242/1)
Consolidated Grant New Applicant Scheme (The study of elementary particles and their interactions - ST/N000242/1)
批准号:
ST/P00377X/1
负责人:
Antonin Vacheret
金额:
$1.34万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2016
资助国家:
英国
项目状态:
已结题
起止时间:
2016 至 --
中文摘要
这是根据新申请者计划为Antonin Vacheret博士提供的综合赠款(CG)级别的支持,作为伦敦帝国理工学院的新学术人员。我在帝国理工学院的研究集中在两个领域:即Solid和LUX/Zeplin实验。SoLid是位于比利时莫尔的SCK CEN BR2研究反应堆的一个新的超短基线反应堆中微子实验。它将在一个强大的核反应堆堆芯附近(5-10米)对电子反中微子通量和能谱进行精确测量。这将使过去和现在的多个实验所观察到的“中微子反常”得到详细的探索。特别是,将以前的结果解释为稀有中微子的证据将受到挑战,因为该实验能够提供整个相关参数空间的排除。它还将通过测量几乎纯的235U反中微子通量来提高对反应堆通量形状的理解,该通量是动力反应堆反中微子通量计算的关键组成部分。Solid是英国的一项实验;它最初是由英国物理学家提出和设计的。它现在是一个国际合作项目,有来自欧洲和美国11个研究所的50人参与。Solid在Imperial是新的,但我从项目开始就一直是UK-PI,目前我是该实验的发言人。我负责建造五个探测器模块中的两个,并为整个实验提供电子学和数据采集卡。很大一部分工作将在帝国理工学院完成。固体实验的第一阶段目前正在建设中,计划在2017年初开始数据采集。LUX/Zeplin是最大的下一代直接暗物质搜索实验。它将使用7吨液体氙气,试图探测星系暗物质和普通物质之间的微弱相互作用。这将是10GeV WIMP质量以上区域最灵敏的暗物质实验。帝国理工学院LUX/Zeplin小组已经大量参与了这项实验的建设。我的工作将是承担英国数据中心的组织工作,为2019年的数据采集做准备
英文摘要
This is Consolidated Grant (CG)-level support under the New Applicant scheme for Dr Antonin Vacheret as a new member of academic staff at Imperial College London.My research at Imperial focuses on two areas: namely the SoLid and LUX/Zeplin experiments.SoLid is a new ultra-short-baseline reactor neutrino experiment at the SCK CEN BR2 research reactor located in Mol, Belgium. It will make a precision measurement of the electron antineutrino flux and energy spectrum close (5-10m) to a powerful nuclear reactor core. This will allow the 'neutrino anomalies' observed by multiple past and current experiments to be explored in detail. In particular, the interpretation of previous results as evidence for sterile neutrinos will be challenged, with the experiment able to provide exclusion over the entire relevant parameter space. It will also improve the understanding of the reactor flux shape by measuring an almost pure 235U antineutrino flux, a key ingredient of the power reactor antineutrino flux calculation. SoLid is a 'UK experiment'; it was originally proposed and designed by UK physicists. It is now an international collaboration with 50 people from 11 institutes in Europe and the US. SoLid is new at Imperial but I have been the UK-PI since the beginning of the project and I am currently the Spokesperson of the experiment. I am responsible for the construction of two of the five detector modules and the delivery of the electronics and DAQ for the full experiment. A large part of this work will be done at Imperial. Phase One of the SoLid experiment is currently under construction and is planned to start data-taking in early 2017.LUX/Zeplin is the biggest next generation direct dark matter search experiment. It will use seven tonnes of liquid xenon in an attempt to detect faint interactions between galactic dark matter and regular matter. It will be the most sensitive dark matter experiment in the region above 10 GeV WIMP mass. The Imperial College LUX/Zeplin group is already heavily involved in the construction of the experiment. My work will be to take on the organization of the UK data center in preparation for data taking in 2019
期刊论文(9)
专著(0)
科研奖励(0)
会议论文
登录
查看更多内容
DOI:
10.1140/epjc/s10052-020-8420-x
发表时间:
2020-11-10
期刊:
EUROPEAN PHYSICAL JOURNAL C
影响因子:
4.4
作者:
[Akerib, D. S., Akerlof, C. W., Zarzhitsky, P.]
通讯作者:
Zarzhitsky, P.
DOI:
10.1103/physrevd.104.062005
发表时间:
2021-02
期刊:
Physical Review D
影响因子:
5
作者:
[D. Akerib;S. Alsum;H. Araújo;X. Bai;J. Balajthy;J. Bang;A. Baxter;E. Bernard;A. Bernstein;T. Biesiadzinski;E. Boulton;B. Boxer;P. Br'as;S. Burdin;D. Byram;M. Carmona-Benitez;C. Chan;J. Cutter;L. de Viveiros;E. Druszkiewicz;A. Fan;S. Fiorucci;R. Gaitskell;C. Ghag;M. Gilchriese;C. Gwilliam;C. Hall;S. Haselschwardt;S. Hertel;D. Hogan;M. Horn;D. Huang;C. Ignarra;R. Jacobsen;O. Jahangir;W. Ji;K. Kamdin;K. Kazkaz;D. Khaitan;E. Korolkova;S. Kravitz;V. Kudryavtsev;E. Leason;B. Lenardo;K. Lesko;J. Liao;J. Lin;A. Lindote;M. Lopes;A. Manalaysay;R. Mannino;N. Marangou;D. Mckinsey;D. Mei;J. Morad;A. Murphy;A. Naylor;C. Nehrkorn;H. Nelson;F. Neves;A. Nilima;K. Oliver-Mallory;K. Palladino;C. Rhyne;Q. Riffard;G. Rischbieter;P. Rossiter;S. Shaw;T. Shutt;C. Silva;M. Solmaz;V. Solovov;P. Sorensen;T. Sumner;N. Swanson;M. Szydagis;D. Taylor;R. Taylor;W. Taylor;B. Tennyson;P. Terman;D. Tiedt;W. To;L. Tvrznikova;U. Utku;A. Vacheret;A. Vaitkus;V. Velan;R. Webb;J. White;T. J. Whitis;M. Witherell;F. Wolfs;D. Woodward;X. Xiang;J. Xu;C. Zhang]
通讯作者:
D. Akerib;S. Alsum;H. Araújo;X. Bai;J. Balajthy;J. Bang;A. Baxter;E. Bernard;A. Bernstein;T. Biesiadzinski;E. Boulton;B. Boxer;P. Br'as;S. Burdin;D. Byram;M. Carmona-Benitez;C. Chan;J. Cutter;L. de Viveiros;E. Druszkiewicz;A. Fan;S. Fiorucci;R. Gaitskell;C. Ghag;M. Gilchriese;C. Gwilliam;C. Hall;S. Haselschwardt;S. Hertel;D. Hogan;M. Horn;D. Huang;C. Ignarra;R. Jacobsen;O. Jahangir;W. Ji;K. Kamdin;K. Kazkaz;D. Khaitan;E. Korolkova;S. Kravitz;V. Kudryavtsev;E. Leason;B. Lenardo;K. Lesko;J. Liao;J. Lin;A. Lindote;M. Lopes;A. Manalaysay;R. Mannino;N. Marangou;D. Mckinsey;D. Mei;J. Morad;A. Murphy;A. Naylor;C. Nehrkorn;H. Nelson;F. Neves;A. Nilima;K. Oliver-Mallory;K. Palladino;C. Rhyne;Q. Riffard;G. Rischbieter;P. Rossiter;S. Shaw;T. Shutt;C. Silva;M. Solmaz;V. Solovov;P. Sorensen;T. Sumner;N. Swanson;M. Szydagis;D. Taylor;R. Taylor;W. Taylor;B. Tennyson;P. Terman;D. Tiedt;W. To;L. Tvrznikova;U. Utku;A. Vacheret;A. Vaitkus;V. Velan;R. Webb;J. White;T. J. Whitis;M. Witherell;F. Wolfs;D. Woodward;X. Xiang;J. Xu;C. Zhang
Identification of Radiopure Titanium for the LZ Dark Matter Experiment and Future Rare Event Searches
LZ 暗物质实验和未来稀有事件搜索中放射性纯钛的鉴定
DOI:
--
发表时间:
2017
期刊:
ArXiv e-prints
影响因子:
--
作者:
[Akerib D. S.]
通讯作者:
Akerib D. S.
DOI:
10.1103/physrevd.102.112002
发表时间:
2020-04
期刊:
Physical Review D
影响因子:
5
作者:
[D. Akerib;S. Alsum;H. Araújo;X. Bai;J. Balajthy;A. Baxter;E. Bernard;A. Bernstein;T. Biesiadzinski;E. Boulton;B. Boxer;P. Br'as;S. Burdin;D. Byram;M. Carmona-Benitez;C. Chan;J. Cutter;L. de Viveiros;E. Druszkiewicz;A. Fan;S. Fiorucci;R. Gaitskell;C. Ghag;M. Gilchriese;C. Gwilliam;C. Hall;S. Haselschwardt;S. Hertel;D. Hogan;M. Horn;D. Huang;C. Ignarra;R. Jacobsen;O. Jahangir;W. Ji;K. Kamdin;K. Kazkaz;D. Khaitan;E. Korolkova;S. Kravitz;V. Kudryavtsev;E. Leason;B. Lenardo;K. Lesko;J. Liao;J. Lin;A. Lindote;M. Lopes;A. Manalaysay;R. Mannino;N. Marangou;D. Mckinsey;D. Mei;M. Moongweluwan;J. Morad;A. Murphy;A. Naylor;C. Nehrkorn;H. Nelson;F. Neves;A. Nilima;K. Oliver-Mallory;K. Palladino;E. K. Pease;Q. Riffard;G. Rischbieter;C. Rhyne;P. Rossiter;S. Shaw;T. Shutt;C. Silva;M. Solmaz;V. Solovov;P. Sorensen;T. Sumner;M. Szydagis;D. Taylor;R. Taylor;W. Taylor;B. Tennyson;P. Terman;D. Tiedt;W. To;L. Tvrznikova;U. Utku;S. Uvarov;A. Vacheret;V. Velan;R. Webb;J. White;T. J. Whitis;M. Witherell;F. Wolfs;D. Woodward;J. Xu;C. Zhang]
通讯作者:
D. Akerib;S. Alsum;H. Araújo;X. Bai;J. Balajthy;A. Baxter;E. Bernard;A. Bernstein;T. Biesiadzinski;E. Boulton;B. Boxer;P. Br'as;S. Burdin;D. Byram;M. Carmona-Benitez;C. Chan;J. Cutter;L. de Viveiros;E. Druszkiewicz;A. Fan;S. Fiorucci;R. Gaitskell;C. Ghag;M. Gilchriese;C. Gwilliam;C. Hall;S. Haselschwardt;S. Hertel;D. Hogan;M. Horn;D. Huang;C. Ignarra;R. Jacobsen;O. Jahangir;W. Ji;K. Kamdin;K. Kazkaz;D. Khaitan;E. Korolkova;S. Kravitz;V. Kudryavtsev;E. Leason;B. Lenardo;K. Lesko;J. Liao;J. Lin;A. Lindote;M. Lopes;A. Manalaysay;R. Mannino;N. Marangou;D. Mckinsey;D. Mei;M. Moongweluwan;J. Morad;A. Murphy;A. Naylor;C. Nehrkorn;H. Nelson;F. Neves;A. Nilima;K. Oliver-Mallory;K. Palladino;E. K. Pease;Q. Riffard;G. Rischbieter;C. Rhyne;P. Rossiter;S. Shaw;T. Shutt;C. Silva;M. Solmaz;V. Solovov;P. Sorensen;T. Sumner;M. Szydagis;D. Taylor;R. Taylor;W. Taylor;B. Tennyson;P. Terman;D. Tiedt;W. To;L. Tvrznikova;U. Utku;S. Uvarov;A. Vacheret;V. Velan;R. Webb;J. White;T. J. Whitis;M. Witherell;F. Wolfs;D. Woodward;J. Xu;C. Zhang
DOI:
10.1103/physrevd.102.092004
发表时间:
2020-11-10
期刊:
PHYSICAL REVIEW D
影响因子:
5
作者:
[Akerib, D. S., Alsum, S., Zhang, C.]
通讯作者:
Zhang, C.
共 8 条
A search for the last neutrino flavour mixing angle with the T2K experiment and development of novel detector technique for safeguards application
-
批准号:ST/I00422X/2
-
项目类别:Fellowship
-
资助金额:$6.04万
-
财政年份:2016
-
负责人:Antonin Vacheret
-
依托单位:
SoLiD Electronics
-
批准号:ST/M001768/1
-
项目类别:Research Grant
-
资助金额:$3.08万
-
财政年份:2013
-
负责人:Antonin Vacheret
-
依托单位:
Development of new generation handheld and backpack neutron detectors
-
批准号:ST/L000113/1
-
项目类别:Research Grant
-
资助金额:$11.92万
-
财政年份:2013
-
负责人:Antonin Vacheret
-
依托单位:
A search for the last neutrino flavour mixing angle with the T2K experiment and development of novel detector technique for safeguards application
-
批准号:ST/I00422X/1
-
项目类别:Fellowship
-
资助金额:$59.22万
-
财政年份:2011
-
负责人:Antonin Vacheret
-
依托单位:
海外基金