课题基金 / 基金详情

Continuation of a Programme of Neutrino Factory Research and Development

Continuation of a Programme of Neutrino Factory Research and Development
继续中微子工厂研究与开发计划
批准号:
ST/H00369X/1
负责人:
Paul Harrison
金额:
$6.09万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2011
资助国家:
英国
项目状态:
已结题
起止时间:
2011 至 --

项目摘要

项目成果

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中文摘要
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英文摘要
Of the species of particles currently known to physics, the neutrinos, which come in three types: electron, muon, and tau, are probably among the most intriguing but least understood. The neutrinos have tiny masses and interact with matter only very weakly. The results of all particle physics experiments to date have been readily explained by the 'Standard Model' of particle physics, developed in the 1960s: that is, except, for a small set of results from a select few experiments investigating the behaviour of neutrinos. Neutrinos are naturally produced continuously in stars and the earth's atmosphere. Experiments to detect these neutrinos have consistently found fewer neutrinos than are produced. So where did they go? There is evidence that these 'missing' neutrinos have changed or 'oscillated' into different types of neutrino, that are not detected. More recently, experiments involving man-made neutrinos have demonstrated similar neutrino oscillation behaviour. For each particle type in nature, there is a corresponding anti-particle type - the anti-particles together are known as anti-matter. So, for each of the three types of neutrinos, there is a corresponding type of anti-neutrino. Of particular interest is the question of whether the oscillations of anti-neutrinos are the same as those of neutrinos, or do the anti-neutrinos behave differently? This question is believed to be related to the fact that the observable universe today is composed almost entirely of matter, whereas the Big Bang which created the Universe 14 billion years ago, should have created equal amounts of matter and anti-matter. The mystery of where the anti-matter has gone could be explained by a difference in the oscillation behaviour of neutrinos and anti-neutrinos. This question can only be answered by making ultra-sensitive measurements of neutrino oscillations using high-intensity man-made beams of neutrinos. The ultimate goal of the proposed research is to produce the most intense beams of neutrinos ever created by man in a 'Neutrino Factory'. These beams of neutrinos will be directed at various angles through the Earth, to different detectors in several parts of the world, allowing the neutrino oscillations to be measured over different distances. This will allow the properties of the neutrinos to be determined far more precisely than ever before, and will allow us to answer the fundamental question of whether the oscillations of neutrinos and anti-neutrinos are the same or not. This should solve the puzzle of where the anti-matter created at the Big Bang has gone, and therefore help to explain the existence of the universe as we know it today.
期刊论文(10)
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会议论文
Energy deposition studies for the Neutrino Factory target station
中微子工厂目标站的能量沉积研究
DOI: --
发表时间: 2011
期刊:
影响因子: --
作者: [[]]
通讯作者: []
DOI: 10.2172/1051488
发表时间: 2011-12
期刊: arXiv: High Energy Physics - Experiment
影响因子: --
作者: [R. Abrams;S. Agarwalla;A. Alekou;C. Andreopoulos;C. Ankenbrandt;S. Antusch;M. Apollonio;M. Aslaninejad;J. Back;P. Ballett;G. Barker;K. Beard;E. Benedetto;J. Bennett;J. Berg;S. Bhattacharya;V. Blackmore;M. Blennow;A. Blondel;A. Bogacz;M. Bonesini;C. Bontoiu;C. Booth;C. Bromberg;S. Brooks;A. Bross;O. Caretta;A. Cervera-Villanueva;S. Choubey;D. Cline;J. Cobb;P. Coloma;L. Coney;M. Cummings;T. Davenne;A. Gouvea;C. Densham;X. Ding;A. Donini;P. Dornan;M. Dracos;F. Dufour;R. Eccleston;R. Edgecock;I. Efthymiopoulos;M. Ellis;E. Fernandez-Martinez;R. Fernow;G. Flanagan;J. Gallardo;R. Gandhi;R. Garoby;B. Gavela;S. Geer;S. Gilardoni;J. Gómez-Cadenas;S. Goswami;V. Graves;Ramesh Gupta;G. Hanson;P. Harrison;T. Hart;P. Hernandez;Patrick Huber;D. Indumathi;R. Johnson;C. Johnstone;Y. Karadzhov;D. Kelliher;H. Kirk;J. Kopp;Y. Kudenko;Y. Kuno;A. Kurup;P. Kyberd;A. Laing;Ting Li;M. Lindner;K. Long;J. L. Pavón;P. Loveridge;S. Machida;D. Majumdar;M. Maltoni;J. Martín-Albo;M. Martini;R. Matev;K. McDonald;A. McFarland;D. Meloni;M. Mezzetto;P. Migliozzi;S. Mishra;N. Mokhov;N. Mondal;J. Morfín;Y. Mori;V. Morozov;D. Neuffer;T. Ota;V. Palladino;S. Parke;S. Pascoli;J. Pasternak;J. Peltoniemi;R. Petti;T. Planche;M. Popovic;J. Pozimski;G. Prior;C.R.Prior;G. Rees;S. Rigolin;T. Roberts;Y. Roblin;C. Rogers;R. Samulyak;T. Schwetz-Mangold;N. Simos;N. Sinha;G. Škoro;P. Snopok;F. Soler;N. Souchlas;J. Strait;D. Stratakis;S. Striganov;Jian-Kai Tang;J. Thomason;L. Tortora;R. Tsenov;W. Winter;H. Witte;O. Yasuda;C. Yoshikawa;M. Zisman]
通讯作者: R. Abrams;S. Agarwalla;A. Alekou;C. Andreopoulos;C. Ankenbrandt;S. Antusch;M. Apollonio;M. Aslaninejad;J. Back;P. Ballett;G. Barker;K. Beard;E. Benedetto;J. Bennett;J. Berg;S. Bhattacharya;V. Blackmore;M. Blennow;A. Blondel;A. Bogacz;M. Bonesini;C. Bontoiu;C. Booth;C. Bromberg;S. Brooks;A. Bross;O. Caretta;A. Cervera-Villanueva;S. Choubey;D. Cline;J. Cobb;P. Coloma;L. Coney;M. Cummings;T. Davenne;A. Gouvea;C. Densham;X. Ding;A. Donini;P. Dornan;M. Dracos;F. Dufour;R. Eccleston;R. Edgecock;I. Efthymiopoulos;M. Ellis;E. Fernandez-Martinez;R. Fernow;G. Flanagan;J. Gallardo;R. Gandhi;R. Garoby;B. Gavela;S. Geer;S. Gilardoni;J. Gómez-Cadenas;S. Goswami;V. Graves;Ramesh Gupta;G. Hanson;P. Harrison;T. Hart;P. Hernandez;Patrick Huber;D. Indumathi;R. Johnson;C. Johnstone;Y. Karadzhov;D. Kelliher;H. Kirk;J. Kopp;Y. Kudenko;Y. Kuno;A. Kurup;P. Kyberd;A. Laing;Ting Li;M. Lindner;K. Long;J. L. Pavón;P. Loveridge;S. Machida;D. Majumdar;M. Maltoni;J. Martín-Albo;M. Martini;R. Matev;K. McDonald;A. McFarland;D. Meloni;M. Mezzetto;P. Migliozzi;S. Mishra;N. Mokhov;N. Mondal;J. Morfín;Y. Mori;V. Morozov;D. Neuffer;T. Ota;V. Palladino;S. Parke;S. Pascoli;J. Pasternak;J. Peltoniemi;R. Petti;T. Planche;M. Popovic;J. Pozimski;G. Prior;C.R.Prior;G. Rees;S. Rigolin;T. Roberts;Y. Roblin;C. Rogers;R. Samulyak;T. Schwetz-Mangold;N. Simos;N. Sinha;G. Škoro;P. Snopok;F. Soler;N. Souchlas;J. Strait;D. Stratakis;S. Striganov;Jian-Kai Tang;J. Thomason;L. Tortora;R. Tsenov;W. Winter;H. Witte;O. Yasuda;C. Yoshikawa;M. Zisman
Characterisation of the muon beams for the Muon Ionisation Cooling Experiment
用于 μ 子电离冷却实验的 μ 子束表征
DOI: 10.1140/epjc/s10052-013-2582-8
发表时间: 2013
期刊: The European Physical Journal C
影响因子: --
作者: [Adams D]
通讯作者: Adams D
DOI: 10.1140/epjc/s10052-014-2832-4
发表时间: 2014
期刊: The European Physical Journal C
影响因子: --
作者: [Back J]
通讯作者: Back J
8
    ATLAS Upgrade 2018 Phase-II Construction - STFC/ATLAS UPGRADE/ST/R002576/1
    • 批准号:
      ST/V002333/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $2.85万
    • 财政年份:
      2020
    • 负责人:
      Paul Harrison
    • 依托单位:
    ATLAS Phase 2 Construction Proposal
    • 批准号:
      ST/R002401/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $80.31万
    • 财政年份:
      2018
    • 负责人:
      Paul Harrison
    • 依托单位:
    Warwick STFC Innovation Partnership Scheme Fellow
    • 批准号:
      ST/R003076/1
    • 项目类别:
      Fellowship
    • 资助金额:
      $15.62万
    • 财政年份:
      2018
    • 负责人:
      Paul Harrison
    • 依托单位:
    Warwick Elementary Particle Physics Capital Equipment 2016
    • 批准号:
      ST/P005926/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $11.03万
    • 财政年份:
      2017
    • 负责人:
      Paul Harrison
    • 依托单位:
    海外基金