STFC Experimental Particle Physics 2018 Consolidated Grant

STFC实验粒子物理2018年综合资助

• 批准号: ST/S000798/1
• 负责人: Simon Peeters
• 金额: $ 223.15万
• 依托单位: University of Sussex
• 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%2FS000798%2F1
• 关键词: STFC; Experimental; Particle; Physics; 2018

The Sussex Experimental Particle Physics (EPP) group counts eleven academic faculty members and focuses on the following main research areas: - the exploration of the Energy Frontier (using the ATLAS experiment, ATLAS Upgrades, future opportunities at colliders)- Neutrino Physics (using the SNO+, NOVA, DUNE, SBND, and JSNS2 experiments)- liquid argon-based direct matter searches (with the DEAP/DarkSide experiments)- precision measurements of the neutron electric dipole moment (the nEDM experiment). The group participates in GridPP and Sussex hosts a certified Grid Tier-2 computing cluster.At ATLAS, we search for physics beyond the current understanding of particle physics. We study in detail the particle interactions to verify our current understanding, but also look for evidence of new processes. This includes the search for Dark Matter - the matter that seems to exist in the Universe but has not been observed or is accounted for in our current models describing our understanding of matter. We will continue to lead on analysis and the trigger (which makes fast real-time decisions about what data is important and should be kept) at the upcoming LHC luminosity upgrades. In parallel with the exploitation of ATLAS and the ATLAS upgrade work, we will maintain a low-level involvement in R&D and physics studies for possible future colliders, aiming to further deepen our understanding of matter and the Universe.We also search directly for Dark Matter by building and operating experiments to try and observe Dark Matter interacting directly inside these experiments. We are involved in the DEAP-3600 experiment in Canada. The international community in direct detection searches using liquid argon has come together to put its weight behind the DarkSide-20k experiment, which will provide the best sensitivity that is currently technically possible.The neutrino has already provided some unexpected surprises and its study promises to answer fundamental questions about the nature of matter. At SNO+, we search for rare decays that could reveal the fundamental nature of neutrinos. At NOvA, we hope to better understand the extremely small masses of neutrinos and test whether matter and anti-matter perhaps behave in different ways. This study will be continued at the DUNE (a future, large-scale liquid-argon experiment). The combination of the studies at the SNO+ and DUNE/NOvA experiments has the potential to explain one of science's biggest questions to date: why is the Universe currently made out of matter and why is there no anti-matter any more?There have been some hints that there are more than the three neutrinos that we so far know about. The SBND experiment will look for evidence for new neutrinos and allow us to build up direct experience with the technology for the future DUNE experiment. The JSNS2 experiment will provide a direct test of previous (but disputed) observations of extra neutrinos, but with significantly fewer backgrounds and better detector technology. It also provides a good test-bed for liquid scintillator detector technology and optical calibration developments.The nEDM experiment studies the properties of neutrons with exquisite precision, complementing the ATLAS, neutrino and dark matter programmes by looking in a completely different way for evidence of a difference in behaviour between matter and antimatter.We participate in experiments through the analysis of data and contributions to technical deliverables. This builds skills among our PhD students and our researches and these developments have led to strong impact. We will continue to do this, in particular in the area of Artificial Intelligence, exploiting techniques that we use in our research. We will continue to actively interact with local industry and forge stronger links. Furthermore, we will bring our research to schools, teachers and the general public in innovative ways on a local, national and international level.

The Sussex Experimental Particle Physics (EPP) group counts eleven academic faculty members and focuses on the following main research areas: - the exploration of the Energy Frontier (using the ATLAS experiment, ATLAS U​​pgrades, future opportunities at colliders)- Neutrino Physics (using the SNO+, NOVA, DUNE, SBND, and JSNS2 experiments)- liquid argon-based direct matter searches (with the DEAP/DarkSide实验） - 中子电偶极矩的精确测量（NEDM实验）。该小组参加了Gridpp，苏塞克斯（Sussex）拥有经过认证的网格层计算集群。我们详细研究粒子相互作用以验证我们当前的理解，但也寻找新过程的证据。这包括对暗物质的搜索 - 宇宙中似乎存在的物质，但尚未观察到或在我们当前的模型中描述了我们对物质的理解。我们将继续领导分析和触发器（这对哪些数据重要而应保留的数据做出快速实时决策）在即将到来的LHC亮度升级处。与Atlas和Atlas升级工作的开发同时，我们将在R＆D和物理研究中保持低级参与可能的未来攻略者，旨在进一步加深对物质和宇宙的理解。我们还通过在这些实验中直接建立和观察到的暗物质来直接搜索暗物质，从而在这些实验中直接进行这些实验相互作用。我们参与了加拿大的DEAP-3600实验。使用Liquid Argon进行直接检测搜索的国际社会已经聚集在一起，将其重量放在了Darkside-20k实验后面，这将提供当前技术上可能的最佳灵敏度。中微子已经提供了一些意外的惊喜，其研究承诺回答有关物质本质的基本问题。在SNO+，我们寻找可能揭示中微子基本本质的罕见衰变。在Nova，我们希望更好地了解中微子极为小的中微子，并测试物质和反物质是否以不同的方式行事。这项研究将在沙丘上进行（未来的大规模液态 - 阿贡实验）。 SNO+和Dune/Nova实验的研究的结合有可能解释迄今为止科学最大的问题之一：为什么目前是由物质制成的宇宙，为什么没有更多的反物质？有一些暗示，迄今为止，这三个中微子比这三个中微子还多。 SBND实验将为新的中微子寻求证据，并让我们在未来的《沙丘实验》中建立直接经验。 JSNS2实验将直接测试以前（但有争议的）观察到额外的中微子，但背景和更好的检测器技术明显较少。它还为液体闪烁体检测器技术和光学校准开发提供了良好的测试床。NEDM实验研究中子的特性具有精确的精度，通过以完全不同的方式来补充Atlas，Neutrino和Dark Matter程序，以完全不同的方式证明了Matter和Antimatter之间的行为和Antimatter之间的差异。我们参与了数据和贡献数据和贡献数据和能力分析技术和能力分析。这在我们的博士生和我们的研究中建立了技能，这些发展导致了强烈的影响。我们将继续这样做，特别是在人工智能领域，利用我们在研究中使用的技术。我们将继续与当地行业进行积极互动，并建立更牢固的联系。此外，我们将以创新的方式将我们的研究带入学校，教师和公众。

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. Erland;M. Errenst;M. Escalier;C. Escobar;O. E. Pastor;E. Etzion;G. Evans;H. Evans;M. Evans;A. Ezhilov;F. Fabbri;L. Fabbri;V. Fabiani;G. Facini;R. Fakhrutdinov;S. Falciano;P. Falke;S. Falke;J. Faltova;Y. Fang;Y. Fang;G. Fanourakis;M. Fanti;M. Faraj;A. Farbin;A. Farilla;E. Farina;T. Farooque;S. Farrington;P. Farthouat;F. Fassi;D. Fassouliotis;M. Giannelli;W. Fawcett;L. Fayard;O. Fedin;M. Feickert;L. Feligioni;A. Fell;C. Feng;M. Feng;M. Fenton;A. Fenyuk;S. W. Ferguson;J. Ferrando;A. Ferrari;P. Ferrari;R. Ferrari;D. Ferrere;C. Ferretti;F. Fiedler;A. Filipčič;F. Filthaut;K. Finelli;M. Fiolhais;L. Fiorini;F. Fischer;W. Fisher;T. Fitschen;I. Fleck;P. Fleischmann;T. Flick;B. Flierl;L. Flores;L. Castillo;F. Follega;N. Fomin;J. H. Foo;G. Forcolin;B. Forland;A. Formica;F. Förster;A. Forti;E. Fortin;M. Foti;D. Fournier;H. Fox;P. Francavilla;S. Francescato;M. Franchini;S. Franchino;D. Francis;L. Franco;L. Franconi;M. Franklin;G. Frattari;P. Freeman;B. Freund;W. Freund;E. Freundlich;D. Frizzell;D. 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Pontecorvo;S. Popa;G. Popeneciu;L. Portalès;D. M. P. Quintero;S. Pospíšil;P. Postolache;K. Potamianos;I. Potrap;C. Potter;H. Potti;T. Poulsen;J. Poveda;T. Powell;G. Pownall;M. Astigarraga;A. Ibanez;P. Pralavorio;M. Prapa;S. Prell;D. Price;M. Primavera;M. Proffitt;N. Proklova;K. Prokofiev;F. Prokoshin;S. Protopopescu;J. Proudfoot;M. Przybycien;D. Pudzha;A. Puri;P. Puzo;D. Pyatiizbyantseva;J. Qian;Y. Qin;A. Quadt;M. Queitsch-Maitland;G. R. Bolanos;M. Racko;F. Ragusa;G. Rahal;J. Raine;S. Rajagopalan;K. Ran;D. F. Rassloff;D. Rauch;S. Rave;B. Ravina;I. Ravinovich;M. Raymond;A. Read;N. P. Readioff;M. Reale;D. Rebuzzi;G. Redlinger;K. Reeves;D. Reikher;A. Reiss;A. Rej;C. Rembser;A. Renardi;M. Renda;M. Rendel;A. Rennie;S. Resconi;E. Resseguie;S. Rettie;B. Reynolds;E. Reynolds;O. Rezanova;P. Reznicek;E. Ricci;R. Richter;S. Richter;E. Richter-Was;M. Ridel;P. Rieck;O. Rifki

A search for the dimuon decay of the Standard Model Higgs boson with the ATLAS detector

• DOI: 10.1016/j.physletb.2020.135980
• 发表时间: 2021-01-10
• 期刊: PHYSICS LETTERS B
• 影响因子: 4.4
• 作者: Aaboud, M.;Aad, G.;Zwalinski, L.
• 通讯作者: Zwalinski, L.

Search for squarks and gluinos in final states with hadronically decaying $\tau$-leptons, jets, and missing transverse momentum using $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector

使用 ATLAS 探测器在 $sqrt{s}$ = 13 TeV 处进行 $pp$ 碰撞，搜索具有强子衰变 $ au$-轻子、喷流和缺失横向动量的最终态夸克和胶子

• DOI: 10.1103/physrevd.99.012009
• 发表时间: 2019
• 作者: M. Aaboud;O. Ricken;S. Schaepe;P. Koenig;P. Bechtle;K. Desch (on behalf of the ATLAS Collaboration)
• 通讯作者: K. Desch (on behalf of the ATLAS Collaboration)

Measurements of top-quark pair single- and double-differential cross-sections in the all-hadronic channel in pp collisions at $$ \sqrt{\mathrm{s}} $$ = 13 TeV using the ATLAS detector

• DOI: 10.1007/jhep01(2021)033
• 发表时间: 2021-01
• 期刊: Journal of High Energy Physics
• 影响因子: 5.4
• 作者: G. Aad;B. Abbott;D. Abbott;A. A. Abud-A.;K. Abeling;D. K. Abhayasinghe;S. H. Abidi;O. AbouZeid-