Particle Physics Consolidated Grant 2019

2019年粒子物理综合补助金

• 批准号: ST/S000933/1
• 负责人: Ian Shipsey
• 金额: $ 788.44万
• 依托单位: University of Oxford
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2019
• 资助国家: 英国
• 起止时间: 2019 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FS000933%2F1
• 关键词: Particle; Physics; Consolidated; Grant; 2019

Particle physics seeks to understand the Universe, its birth, evolution & fate in terms of the interplay of elementary particles (quarks & leptons), the fundamental forces (strong, electromagnetic & weak forces, & gravity) and force-particles that mediate them (photons, W/Z, gluons & gravitons) and the recently discovered Higgs particle that gives elementary particles mass. The last thirty years have seen the development of a theoretical framework, the Standard Model, in which almost all particle-physics data can be explained. But the model is incomplete. It explains what we encounter on Earth but studies of the cosmos suggest the presence of mysterious dark matter that holds galaxies together and more mysterious dark energy that is driving galaxies apart at an ever increasing rate. There are so many mysteries! There has never been a better time to be a particle physicist. Oxford's research will advance significantly our understanding of whatever "new-physics" theory will emerge to replace the Standard Model by providing the data to guide the theoretical work to develop it.The Large Hadron Collider (LHC) reproduces the conditions within a million millionth of a second of the Big Bang. Oxford plays a major role in ATLAS and LHCb. These experiments have the potential to completely revolutionise our understanding of the universe. In ATLAS, Oxford physicists participated in the exciting discovery of the "Higgs particle", which makes matter matter by giving it mass. The Higgs particle is like a curtain; now that we have found the Higgs we can draw back the curtain to see a new world. Accordingly, we are studying it in great detail. We are also searching for particles with "supersymmetry" (SUSY), a theory that would provide a solution to "dark-matter" that makes up about 80% of matter in the Universe; and ATLAS is searching for hidden extra spatial dimensions. Oxford physicists on LHCb strive for a better understanding of the origin of the matter-antimatter asymmetry in the Universe by studying subtle differences in the behaviour of quarks & antiquarks - "CP-violation". This asymmetry permits us to exist.Over the next decade, the LHC will upgrade to higher energy & intensity so detector improvements will be made for ATLAS & LHCb during this grant. The upgraded detectors will take particle physics to an unprecedented level of sensitivity for the nearly inevitable new-physics observations. Throughout our work we use powerful computing resources and develop cutting-edge analysis tools that are necessary for the extraction of important discoveries from vast volumes of data.We participate in high-precision experiments complementary to the large experiments at the LHC. LZ addresses one of the most important questions in particle physics & cosmology: a search for dark matter; a candidate is the lightest SUSY particle. Mu3e searches for new physics mediated by very heavy particles that would not be visible at the LHC but are expected in many theoretical models including SUSY. LSST will measure how quickly the expansion of the universe is speeding up due to the mysterious dark energy that represents 75% of all energy in the universe and acts like anti-gravity pushing galaxies apart. Through T2K, SK, HK, DUNE, & future projects, Oxford aims to understand the elusive neutrino, its "oscillation" from one type to another and whether there is a difference between neutrino and anti-neutrino properties - "CP-violation". SNO+ will measure other properties of the neutrino, e.g. whether or not it is its own antiparticle.Throughout, Oxford will continue to develop & enhance capabilities in mechanical & electronic design so that we retain the ability to construct the most sophisticated apparatus for our experiments. We will retain our world-leading role for scientific excellence & major state-of-the-art detector construction in particle physics for the future. These are exciting times for particle physics, and Oxford is playing a major role.

粒子物理学试图从基本力(夸克和轻子)、基本力(强、电磁和弱力，以及引力)和力粒子(光子、W/Z、胶子和引力子)以及最近发现的赋予基本粒子质量的希格斯粒子之间的相互作用来理解宇宙及其诞生、演化和命运。在过去的三十年里，我们看到了一个理论框架--标准模型的发展，在这个框架中，几乎所有的粒子物理数据都可以被解释。但这个模型是不完整的。它解释了我们在地球上遇到的情况，但对宇宙的研究表明，神秘暗物质的存在将星系聚集在一起，而更神秘的暗能量正在以越来越快的速度将星系分开。有这么多的谜团！没有比现在更适合做粒子物理学家的时候了。牛津大学的研究将极大地提高我们对任何将出现的取代标准模型的“新物理”理论的理解，通过提供数据来指导发展它的理论工作。大型强子对撞机(LHC)再现了大爆炸百万分之一秒内的条件。牛津在ATLAS和LHCb中扮演着重要角色。这些实验有可能彻底改变我们对宇宙的理解。在ATLAS中，牛津大学的物理学家参与了“希格斯粒子”的令人兴奋的发现，希格斯粒子通过赋予物质质量来制造物质。希格斯粒子就像一块窗帘；既然我们已经找到了希格斯粒子，我们就可以拉开窗帘，看到一个新的世界。因此，我们正在非常详细地研究它。我们还在寻找具有“超对称性”(SUSY)的粒子，这一理论将为构成宇宙中约80%的物质的“暗物质”提供解决方案；而ATLAS正在寻找隐藏的额外空间维度。牛津大学大型强子对撞机上的物理学家们通过研究夸克和反夸克行为的细微差别，努力更好地理解物质的起源--宇宙中的反物质不对称性--“CP破坏”。这种不对称性允许我们存在。在接下来的十年里，大型强子对撞机将升级到更高的能量和强度，因此在这次拨款期间，将对ATLAS和LHCb的探测器进行改进。对于几乎不可避免的新物理观测，升级后的探测器将把粒子物理学的灵敏度提高到前所未有的水平。在整个工作中，我们使用强大的计算资源并开发尖端分析工具，这些工具对于从海量数据中提取重要发现是必要的。我们参与与大型强子对撞机上的大型实验相辅相成的高精度实验。LZ解决了粒子物理学和宇宙学中最重要的问题之一：寻找暗物质；候选粒子是最轻的超对称粒子。MU3E正在寻找由非常重的粒子介导的新物理，这些粒子在大型强子对撞机上是看不到的，但在包括SUSY在内的许多理论模型中都是可以看到的。LSST将测量宇宙膨胀的速度，这是由于神秘的暗能量代表了宇宙中所有能量的75%，它的作用就像是反重力将星系推开。通过T2K、SK、HK、DUNE和未来的项目，牛津大学的目标是了解难以捉摸的中微子，它从一种类型到另一种类型的“振荡”，以及中微子和反中微子之间是否存在差异--“CP破坏”。SnO+将测量中微子的其他性质，例如它是否是它自己的反粒子。尽管如此，牛津大学将继续发展和增强机械和电子设计方面的能力，以便我们保持为我们的实验建造最复杂的设备的能力。我们将保持我们在科学上的领先地位，在未来的粒子物理中主要建造最先进的探测器。这是粒子物理学令人兴奋的时代，牛津大学正在发挥重要作用。

项目成果

Constraints on Higgs boson properties using $$WW^{*}(\rightarrow e\nu \mu \nu )jj$$ production in $$36.1\,\mathrm{fb}^{-1}$$ of $$\sqrt{s}=13$$ TeV pp collisions with the ATLAS detector

• DOI: 10.1140/epjc/s10052-022-10366-1
• 发表时间: 2022-07
• 期刊: The European Physical Journal C
• 作者: G. Aad;B. Abbott;D. Abbott;A. A. Abud-A.;K. Abeling;D. K. Abhayasinghe;S. H. Abidi;O. AbouZeid;N. Abraham;H. Abramowicz;H. Abreu;Y. Abulaiti;B. Acharya;B. Achkar;L. Adam;C. Bourdarios;L. Adamczyk;L. Adamek;J. Adelman;A. Adiguzel;S. Adorni;T. Adye;A. Affolder;Y. Afik;C. Agapopoulou;M. N. Agaras;A. Aggarwal;C. Agheorghiesei;J. A. Aguilar-Saavedra;A. Ahmad;F. Ahmadov;W. S. Ahmed;X. Ai;G. Aielli;S. Akatsuka;M. Akbiyik;T. Åkesson;E. Akilli;A. Akimov;K. Khoury;G. Alberghi;J. Albert;M. A. Verzini;S. Alderweireldt;M. Aleksa;I. Aleksandrov;C. Alexa;T. Alexopoulos;A. Alfonsi;F. Alfonsi;M. Alhroob;B. Ali;S. Ali;M. Aliev;G. Alimonti;C. Allaire;B. Allbrooke;P. Allport;A. Aloisio;F. Alonso;C. Alpigiani;E. Camelia;M. A. Estevez;M. Alviggi;Y. A. Coutinho;A. Ambler;L. Ambroz;C. Amelung;D. Amidei;S. D. Santos;S. Amoroso;C. Amrouche;C. Anastopoulos;N. Andari;T. Andeen;J. Anders;S. Y. Andrean;A. Andreazza;V. Andrei;C. Anelli;S. Angelidakis;A. Angerami;A. Anisenkov;A. Annovi;C. Antel;M. Anthony;E. Antipov;M. Antonelli;D. Antrim;F. Anulli;M. Aoki;J. A. Pozo;M. Aparo;L. A. Bella;N. Aranzabal;V. A. Ferraz;R. A. Pereira;C. Arcangeletti;A. Arce;J. Arguin;S. Argyropoulos;J. Arling;A. Armbruster;A. Armstrong;O. Arnaez;H. Arnold;Z. P. A. Tame;G. Artoni;H. Asada;K. Asai;S. Asai;T. Asawatavonvanich;N. Asbah;E. Asimakopoulou;L. Asquith;J. Assahsah;K. Assamagan;R. Astalos;R. Atkin;M. Atkinson;N. B. Atlay;H. Atmani;P. Atmasiddha;K. Augsten;V. A. Austrup;G. Avolio;M. Ayoub;G. Azuelos;D. Babal;H. Bachacou;K. Bachas;F. Backman;P. Bagnaia;H. Bahrasemani;A. Bailey;V. R. Bailey;J. Baines;C. Bakalis;O. Baker;P. Bakker;E. Bakos;D. B. Gupta;S. Balaji;R. Balasubramanian;E. Baldin;P. Balek;F. Balli;W. Balunas;J. Balz;E. Banas;M. Bandieramonte;A. Bandyopadhyay;L. Barak;W. Barbe;E. Barberio;D. Barberis;M. Barbero;G. Barbour;T. Barillari;M. Barisits;J. Barkeloo;T. Barklow;B. Barnett;R. Barnett;Z. Barnovska-Blenessy;A. Baroncelli;G. Barone;A. Barr;L. B. Navarro;F. Barreiro;J. G. D. da Costa;U. Barron;S. Barsov;F. Bartels;R. Bartoldus;G. Bartolini;A. Barton;P. Bartos;A. Basalaev;A. Basan;A. Bassalat;M. Basso;C. Basson;R. Bates;S. Batlamous;J. Batley;B. Batool;M. Battaglia;M. Bauce;F. Bauer;P. Bauer;H. Bawa;A. Bayirli;J. Beacham;T. Beau;P. Beauchemin;F. Becherer;P. Bechtle;H. Beck;K. Becker;C. Becot;A. Beddall;V. Bednyakov;C. Bee;T. Beermann;M. Begalli;M. Begel;A. Behera;J. Behr;F. Beisiegel;M. Belfkir;G. Bella;L. Bellagamba;A. Bellerive;P. Bellos;K. Beloborodov;K. Belotskiy;N. Belyaev;D. Benchekroun;N. Benekos;Y. Benhammou;D. Benjamin;M. Benoit;J. Bensinger;S. Bentvelsen;L. Beresford;M. Beretta;D. Berge;E. Kuutmann;N. Berger;B. Bergmann;L. Bergsten;J. Beringer;S. Berlendis;G. Bernardi;C. Bernius;F. Bernlochner;T. Berry;P. Berta;A. Berthold;I. Bertram;O. B. Bylund;S. Bethke;A. Betti;A. Bevan;S. Bhatta;D. Bhattacharya;P. Bhattarai;V. Bhopatkar;R. Bi;R. Bianchi;O. Biebel;D. Biedermann;R. Bielski;K. Bierwagen;N. Biesuz;M. Biglietti;T. Billoud;M. Bindi;A. Bingul;C. Bini;S. Biondi;C. Birch-sykes;M. Birman;T. Bisanz;J. Biswal;D. Biswas;A. Bitadze;C. Bittrich;K. Bjørke;T. Blažek;I. Bloch;C. Blocker;A. Blue;U. Blumenschein;J. Blumenthal;G. Bobbink;V. Bobrovnikov;D. Bogavac;A. Bogdanchikov;C. Bohm;V. Boisvert;P. Bokan;T. Bold;M. Bomben;M. Bona;J. Bonilla;M. Boonekamp;C. Booth;A. Borbély;H. Borecka-Bielska;L. S. Borgna;A. Borisov;G. Borissov;Daniela Bortoletto;D. Boscherini;M. Bosman;J. Sola;K. Bouaouda;J. Boudreau;E. Bouhova-Thacker;D. Boumediene;R. Bouquet;A. Boveia;J. Boyd;D. Boye;I. Boyko;A. J. Bozson;J. Bracinik;N. Brahimi;G. Brandt;O. Brandt;F. Braren;B. Brau;J. Brau;W. Madden;K. Brendlinger;R. Brener;L. Brenner;R. Brenner;S. Bressler;B. Brickwedde;D. Briglin;D. Britton;D. Britzger;I. Brock;R. Brock;G. Brooijmans;W. Brooks;E. Brost;P. B. D. de Renstrom;B. Brüers;D. Bruncko;A. Bruni;G. Bruni;M. Bruschi;N. Bruscino;L. Bryngemark;T. Buanes;Q. Buat;P. Buchholz;A. Buckley;I. Budagov;M. K. Bugge;O. Bulekov;B. Bullard;T. Burch;S. Burdin;C. Burgard;A. Burger;B. Burghgrave;J. Burr;C. Burton;J. Burzynski;V. Büscher;E. Buschmann;P. Bussey;J. Butler;C. Buttar;J. Butterworth;W. Buttinger;C. J. B. Vazquez;A. Buzykaev;G. Cabras;S. Urbán;D. Caforio;H. Cai;V. Cairo;O. Cakir;N. Calace;P. Calafiura;G. Calderini;P. Calfayan;G. Callea;L. Caloba;A. Caltabiano;S. Lopez;D. Calvet;S. Calvet;T. Calvet;M. Calvetti;R. Toro;S. Camarda;D. C. Munoz;P. Camarri;M. Camerlingo;D. Cameron;C. Camincher;M. Campanelli;A. Camplani;V. Canale;A. Canesse;M. C. Bret;J. Cantero;Y. Cao;M. Capua;R. Cardarelli;F. Cardillo;G. Carducci;T. Carli;G. Carlino;B. Carlson;E. Carlson;L. Carminati;R. Carney;S. Caron;E. Carquin;S. Carrá;G. Carratta;J. Carter;T. Carter;M. P. Casado;A. Casha;E. G. Castiglia;F. Castillo;L. C. Garcia;V. Gimenez;N. Castro;A. Catinaccio;J. Catmore;A. Cattai;V. Cavaliere;V. Cavasinni;E. Celebi;F. Celli;K. Cerny;A. Cerqueira;A. Cerri;L. Cerrito;F. Cerutti;A. Cervelli;S. Çetin;Z. Chadi;D. Chakraborty;J. Chan;W. Chan;W. Y. Chan;J. Chapman;B. Chargeishvili;D. Charlton;T. Charman;M. Chatterjee;C. Chau;S. Chekanov;S. Chekulaev;G. Chelkov;B. Chen;C. Chen;C. Chen;H. Chen;H. Chen;J. Chen;J. Chen;J. Chen;S. Chen;S. Chen;X. Chen;Y. Chen;Y. Chen;H. C. Cheng;H. J. Cheng;A. Cheplakov;E. Cheremushkina;R. C. Moursli;E. Cheu;K. Cheung;T. Chevalérias;L. Chevalier;V. Chiarella;G. Chiarelli;G. Chiodini;A. Chisholm;A. Chitan;I. Chiu;Y. Chiu;M. Chizhov;K. Choi;A. Chomont;Y. Chou;Y. S. Chow;L. D. Christopher;M. Chu;X. Chu;J. Chudoba;J. Chwastowski;D. Cieri;K. Ciesla;V. Cindro;I. A. Cioară;A. Ciocio;F. Cirotto;Z. Citron;M. Citterio;D. Ciubotaru;B. Ciungu;A. Clark;P. Clark;S. E. Clawson;C. Clement;L. Clissa;Y. Coadou;M. Cobal;A. Coccaro;J. Cochran;R. D. De Sa;H. Cohen;A. Coimbra;B. Cole;J. Collot;P. Muiño;S. Connell;I. Connelly;F. Conventi;A. Cooper-Sarkar;F. Cormier;L. Corpe;M. Corradi;E. Corrigan;F. Corriveau;M. Costa;F. Costanza;D. Costanzo;G. Cowan;J. Cowley;J. Crane;K. Cranmer;R. Creager;S. Crépé-Renaudin;F. Crescioli;M. Cristinziani;M. Cristoforetti;V. Croft;G. Crosetti;A. Cueto;T. C. Donszelmann;H. Cui;A. Cukierman;W. Cunningham;S. Czekierda;P. Czodrowski;M. Czurylo;M. Da Cunha Sargedas De Sousa;J. V. Da Fonseca Pinto;C. Da Via;W. Dąbrowski;F. Dachs;T. Dado;S. Dahbi;T. Dai;C. Dallapiccola;M. Dam;G. D'amen;V. D'Amico;J. Damp;J. Dandoy;M. F. Daneri;M. Danninger;V. Dao;G. Darbo;O. Dartsi;A. Dattagupta;S. D'Auria;C. David;T. Davidek;D. Davis;I. Dawson;K. De;R. De Asmundis;M. De Beurs;S. De Castro;N. de Groot;P. de Jong;H. De la Torre;A. De Maria;D. De Pedis;A. De Salvo;U. De Sanctis;M. De Santis;A. De Santo;J. De Vivie De Regie-J.-De-Vivie-De-Regie-1383287875;D. Dedovich;A. Deiana;J. Peso;Y. D. Diaz;D. Delgove;F. Déliot;C. Delitzsch;M. D. Pietra;D. Volpe;A. Dell'Acqua;L. Dell'Asta;M. Delmastro;C. Delporte;P. Delsart;S. Demers;M. Demichev;G. Demontigny;S. Denisov;L. D'Eramo;D. Derendarz;J. Derkaoui;F. Derue;P. Dervan;K. Desch;K. Dette;C. Deutsch;P. Deviveiros;F. Bello;A. Ciaccio;L. Ciaccio;C. Donato;A. Girolamo;G. Gregorio;A. Luca;B. Micco;R. Nardo;R. Sipio;C. Diaconu;F. Dias;T. Vale;M. Diaz;F. Capriles;J. Dickinson;M. Didenko;E. Diehl;J. Dietrich;S. D. Cornell;C. Pardos;A. Dimitrievska;W. Ding;J. Dingfelder;S. Dittmeier;F. Dittus;F. Djama;T. Djobava;J. Djuvsland;M. D. Vale;M. Dobre;D. Dodsworth;C. Doglioni;J. Dolejsi;Z. Doležal;M. Donadelli;B. Dong;J. Donini;A. D'onofrio;M. D’Onofrio;J. Dopke;Armanda Dória;M. Dova;A. Doyle;E. Drechsler;E. Dreyer;T. Dreyer;A. Drobac;D. Du;T. Pree;Y. Duan;F. Dubinin;M. Dubovsky;A. Dubreuil;E. Duchovni;G. Duckeck;O. Ducu;D. Duda;A. Dudarev;A. Dudder;M. D'uffizi;L. Duflot;M. Dührssen;C. Dülsen;M. Dumancic;A. E. Dumitriu;M. Dunford;S. Dungs;A. Duperrin;H. Yildiz;M. Düren;A. Durglishvili;B. Dutta;D. Duvnjak;B. Dwyer;G. Dyckes;M. Dyndał;S. Dysch;B. Dziedzic;M. G. Eggleston;T. Eifert;G. Eigen;K. Einsweiler;T. Ekelof;H. Jarrari;A. Moussaouy;V. Ellajosyula;M. Ellert;F. Ellinghaus;A. Elliot;N. Ellis;J. Elmsheuser;M. Elsing;D. Emeliyanov;A. Emerman;Y. Enari;J. Erdmann;A. Ereditato;P. 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Measurement of the relative B c ± / B ± production cross section with the ATLAS detector at s = 8 TeV

使用 ATLAS 探测器在 s = 8 TeV 下测量相对 B c ± / B ± 生产截面

• DOI: 10.1103/physrevd.104.012010
• 发表时间: 2021
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Aaboud M

Observation of WWW Production in pp Collisions at sqrt[s]=13 TeV with the ATLAS Detector.

• DOI: 10.1103/physrevlett.129.061803
• 发表时间: 2022-01
• 期刊: Physical review letters
• 影响因子: 8.6
• 作者: G. Aad;B. Abbott;D. Abbott;A. Abed Abud;K. Abeling;D. Abhayasinghe;S. H. Abidi;A. Aboulhorma-A.-Aboul