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IRIS - Res&Arch Institutional Research Information System - Research &Archive
The first collider search for dark matter arising from a strongly coupled hidden sector is presented and uses a data sample corresponding to 138 fb(-1), collected with the CMS detector at the CERN LHC, at root s = 13 TeV. The hidden sector is hypothesized to couple to the standard model (SM) via a heavy leptophobic Z' mediator produced as a resonance in proton-proton collisions. The mediator decay results in two "semivisible" jets, containing both visible matter and invisible dark matter. The final state therefore includes moderate missing energy aligned with one of the jets, a signature ignored by most dark matter searches. No structure in the dijet transverse mass spectra compatible with the signal is observed. Assuming the Z' boson has a universal coupling of 0.25 to the SM quarks, an inclusive search, relevant to any model that exhibits this kinematic behavior, excludes mediator masses of 1.5-4.0 TeV at 95% confidence level, depending on the other signal model parameters. To enhance the sensitivity of the search for this particular class of hidden sector models, a boosted decision tree (BDT) is trained using jet substructure variables to distinguish between semivisible jets and SM jets from background processes. When the BDT is employed to identify each jet in the dijet system as semivisible, the mediator mass exclusion increases to 5.1 TeV, for wider ranges of the other signal model parameters. These limits exclude a wide range of strongly coupled hidden sector models for the first time.
Search for resonant production of strongly coupled dark matter in proton-proton collisions at 13 TeV
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Cuevas;C. Erice;J. Fernandez Menendez;S. Folgueras;I. Gonzalez Caballero;J. R. Gonz??lez Fern??ndez;E. Palencia Cortezon;C. Ram??n ??lvarez;V. Rodr??guez Bouza;A. Soto Rodr??guez;A. Trapote;N. Trevisani;C. Vico Villalba;J. A. Brochero Cifuentes;I. J. Cabrillo;A. Calderon;J. Duarte Campderros;M. Fernandez;C. Fernandez Madrazo;P. J. Fern??ndez Manteca;A. Garc??a Alonso;G. Gomez;C. Martinez Rivero;P. Martinez Ruiz del Arbol;F. Matorras;P. Matorras Cuevas;J. Piedra Gomez;C. Prieels;A. Ruiz-Jimeno;L. Scodellaro;I. Vila;J. M. Vizan Garcia;M. K. Jayananda;B. Kailasapathy;D. U. J. Sonnadara;D. D. C. Wickramarathna;W. G. D. Dharmaratna;K. Liyanage;N. Perera;N. Wickramage;T. K. Aarrestad;D. Abbaneo;J. Alimena;E. Auffray;G. Auzinger;J. Baechler;P. Baillon;D. Barney;J. Bendavid;M. Bianco;A. Bocci;C. Caillol;T. Camporesi;M. Capeans Garrido;G. Cerminara;N. Chernyavskaya;S. S. Chhibra;S. Choudhury;M. Cipriani;L. Cristella;D. d???Enterria;A. Dabrowski;A. David;A. De Roeck;M. M. Defranchis;M. Deile;M. 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Boran;S. Damarseckin;Z. S. Demiroglu;F. Dolek;I. Dumanoglu;E. Eskut;Y. Guler;E. Gurpinar Guler;C. Isik;O. Kara;A. Kayis Topaksu;U. Kiminsu;G. Onengut;K. Ozdemir;A. Polatoz;A. E. Simsek;B. Tali;U. G. Tok;S. Turkcapar;I. S. Zorbakir;G. Karapinar;K. Ocalan;M. Yalvac;B. Akgun;I. O. Atakisi;E. Gulmez;M. Kaya;O. Kaya;??. ??z??elik;S. Tekten;E. A. Yetkin;A. Cakir;K. Cankocak;Y. Komurcu;S. Sen;S. Cerci;I. Hos;B. Isildak;B. Kaynak;S. Ozkorucuklu;H. Sert;C. Simsek;D. Sunar Cerci;C. Zorbilmez;B. Grynyov;L. Levchuk;D. Anthony;E. Bhal;S. Bologna;J. J. Brooke;A. Bundock;E. Clement;D. Cussans;H. Flacher;M. Glowacki;J. Goldstein;G. P. Heath;H. F. Heath;L. Kreczko;B. Krikler;S. Paramesvaran;S. Seif El Nasr-Storey;V. J. Smith;N. Stylianou;K. Walkingshaw Pass;R. White;K. W. Bell;A. Belyaev;C. Brew;R. M. Brown;D. J. A. Cockerill;C. Cooke;K. V. Ellis;K. Harder;S. Harper;M. -L. Holmberg;J. Linacre;K. Manolopoulos;D. M. Newbold;E. Olaiya;D. Petyt;T. Reis;T. Schuh;C. H. Shepherd-Themistocleous;I. R. 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Benelli;B. Burkle;X. Coubez;D. Cutts;M. Hadley;U. Heintz;J. M. Hogan;T. Kwon;G. Landsberg;K. T. Lau;D. Li;M. Lukasik;J. Luo;M. Narain;N. Pervan;S. Sagir;F. Simpson;E. Usai;W. Y. Wong;X. Yan;D. Yu;W. Zhang;J. Bonilla;C. Brainerd;R. Breedon;M. Calderon De La Barca Sanchez;M. Chertok;J. Conway;P. T. Cox;R. Erbacher;G. Haza;F. Jensen;O. Kukral;R. Lander;M. Mulhearn;D. Pellett;B. Regnery;D. Taylor;Y. Yao;F. Zhang;M. Bachtis;R. Cousins;A. Datta;D. Hamilton;J. Hauser;M. Ignatenko;M. A. Iqbal;T. Lam;W. A. Nash;S. Regnard;D. Saltzberg;B. Stone;V. Valuev;Y. Chen;R. Clare;J. W. Gary;M. Gordon;G. Hanson;G. Karapostoli;O. R. Long;N. Manganelli;W. Si;S. Wimpenny;Y. Zhang;J. G. Branson;P. Chang;S. Cittolin;S. Cooperstein;D. Diaz;J. Duarte;R. Gerosa;L. Giannini;J. Guiang;R. Kansal;V. Krutelyov;R. Lee;J. Letts;M. Masciovecchio;F. Mokhtar;M. Pieri;B. V. Sathia Narayanan;V. Sharma;M. Tadel;F. W??rthwein;Y. Xiang;A. Yagil;N. Amin;C. Campagnari;M. Citron;G. Collura;A. Dorsett;V. Dutta;J. Incandela;M. Kilpatrick;J. Kim;B. Marsh;H. Mei;M. Oshiro;M. Quinnan;J. Richman;U. Sarica;F. Setti;J. Sheplock;P. Siddireddy;D. Stuart;S. Wang;A. Bornheim;O. Cerri;I. Dutta;J. M. Lawhorn;N. Lu;J. Mao;H. B. Newman;T. Q. Nguyen;M. Spiropulu;J. R. Vlimant;C. Wang;S. Xie;Z. Zhang;R. Y. Zhu;J. Alison;S. An;M. B. Andrews;P. Bryant;T. Ferguson;A. Harilal;C. Liu;T. Mudholkar;M. Paulini;A. Sanchez;W. Terrill;J. P. Cumalat;W. T. Ford;A. Hassani;G. Karathanasis;E. MacDonald;R. Patel;A. Perloff;C. Savard;N. Schonbeck;K. Stenson;K. A. Ulmer;S. R. Wagner;N. Zipper;J. Alexander;S. Bright-Thonney;X. Chen;Y. Cheng;D. J. Cranshaw;S. Hogan;J. Monroy;J. R. Patterson;D. Quach;J. Reichert;M. Reid;A. Ryd;W. Sun;J. Thom;P. Wittich;R. Zou;M. Albrow;M. Alyari;G. Apollinari;A. Apresyan;A. Apyan;L. A. T. Bauerdick;D. Berry;J. Berryhill;P. C. Bhat;K. Burkett;J. N. Butler;A. Canepa;G. B. Cerati;H. W. K. Cheung;F. Chlebana;K. F. Di Petrillo;J. Dickinson;V. D. Elvira;Y. Feng;J. Freeman;Z. Gecse;L. Gray;D. Green;S. Gr??nendahl;O. 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Yumiceva;M. R. Adams;H. Becerril Gonzalez;R. Cavanaugh;S. Dittmer;O. Evdokimov;C. E. Gerber;D. J. Hofman;A. H. Merrit;C. Mills;G. Oh;T. Roy;S. Rudrabhatla;M. B. Tonjes;N. Varelas;J. Viinikainen;X. Wang;Z. Ye;M. Alhusseini;K. Dilsiz;L. Emediato;R. P. Gandrajula;O. K. K??seyan;J. -P. Merlo;A. Mestvirishvili;J. Nachtman;H. Ogul;Y. Onel;A. Penzo;C. Snyder;E. Tiras;O. Amram;B. Blumenfeld;L. Corcodilos;J. Davis;A. V. Gritsan;S. Kyriacou;P. Maksimovic;J. Roskes;M. Swartz;T. ??. V??mi;A. Abreu;J. Anguiano;C. Baldenegro Barrera;P. Baringer;A. Bean;Z. Flowers;T. Isidori;S. Khalil;J. King;G. Krintiras;A. Kropivnitskaya;M. Lazarovits;C. Le Mahieu;C. Lindsey;J. Marquez;N. Minafra;M. Murray;M. Nickel;C. Rogan;C. Royon;R. Salvatico;S. Sanders;E. Schmitz;C. Smith;Q. Wang;Z. Warner;J. Williams;G. Wilson;S. Duric;A. Ivanov;K. Kaadze;D. Kim;Y. Maravin;T. Mitchell;A. Modak;K. Nam;F. Rebassoo;D. Wright;E. Adams;A. Baden;O. Baron;A. Belloni;S. C. Eno;N. J. Hadley;S. Jabeen;R. G. Kellogg;T. Koeth;Y. Lai;S. Lascio;A. C. Mignerey;S. Nabili;C. Palmer;M. Seidel;A. Skuja;L. Wang;K. Wong;D. Abercrombie;G. Andreassi;R. Bi;W. Busza;I. A. Cali;Y. Chen;M. D???Alfonso;J. Eysermans;C. Freer;G. Gomez Ceballos;M. Goncharov;P. Harris;M. Hu;M. Klute;D. Kovalskyi;J. Krupa;Y. -J. Lee;C. Mironov;C. Paus;D. Rankin;C. Roland;G. Roland;Z. Shi;G. S. F. Stephans;J. Wang;Z. Wang;B. Wyslouch;R. M. Chatterjee;A. Evans;J. Hiltbrand;Sh. Jain;B. M. Joshi;M. Krohn;Y. Kubota;J. Mans;M. Revering;R. Rusack;R. Saradhy;N. Schroeder;N. Strobbe;M. A. Wadud;K. Bloom;M. Bryson;S. Chauhan;D. R. Claes;C. Fangmeier;L. Finco;F. Golf;C. Joo;I. Kravchenko;I. Reed;J. E. Siado;G. R. Snow;W. Tabb;A. Wightman;F. Yan;A. G. Zecchinelli;G. Agarwal;H. Bandyopadhyay;L. Hay;I. Iashvili;A. Kharchilava;C. McLean;D. Nguyen;J. Pekkanen;S. Rappoccio;A. Williams;G. Alverson;E. Barberis;Y. Haddad;Y. Han;A. Hortiangtham;A. Krishna;J. Li;J. Lidrych;G. Madigan;B. Marzocchi;D. M. Morse;V. Nguyen;T. Orimoto;A. Parker;L. Skinnari;A. Tishelman-Charny;T. Wamorkar;B. Wang;A. Wisecarver;D. Wood;S. Bhattacharya;J. Bueghly;Z. Chen;A. Gilbert;T. Gunter;K. A. Hahn;Y. Liu;N. Odell;M. H. Schmitt;M. Velasco;R. Band;R. Bucci;M. Cremonesi;A. Das;N. Dev;R. Goldouzian;M. Hildreth;K. Hurtado Anampa;C. Jessop;K. Lannon;J. Lawrence;N. Loukas;D. Lutton;J. Mariano;N. Marinelli;I. Mcalister;T. McCauley;C. Mcgrady;K. Mohrman;C. Moore;Y. Musienko;R. Ruchti;A. Townsend;M. Wayne;M. Zarucki;L. Zygala;B. Bylsma;L. S. Durkin;B. Francis;C. Hill;M. Nunez Ornelas;K. Wei;B. L. Winer;B. R. Yates;F. M. Addesa;B. Bonham;P. Das;G. Dezoort;P. Elmer;A. Frankenthal;B. Greenberg;N. Haubrich;S. Higginbotham;A. Kalogeropoulos;G. Kopp;S. Kwan;D. Lange;D. Marlow;K. Mei;I. Ojalvo;J. Olsen;D. Stickland;C. Tully;S. Malik;S. Norberg;A. S. Bakshi;V. E. Barnes;R. Chawla;S. Das;L. Gutay;M. Jones;A. W. Jung;D. Kondratyev;A. M. Koshy;M. Liu;G. Negro;N. Neumeister;G. Paspalaki;S. Piperov;A. Purohit;J. F. Schulte;M. Stojanovic;J. Thieman;F. Wang;R. Xiao;W. Xie;J. Dolen;N. Parashar;D. Acosta;A. Baty;T. Carnahan;M. Decaro;S. Dildick;K. M. Ecklund;S. Freed;P. Gardner;F. J. M. Geurts;A. Kumar;W. Li;B. P. Padley;R. Redjimi;J. Rotter;W. Shi;A. G. Stahl Leiton;S. Yang;L. Zhang;Y. Zhang;A. Bodek;P. de Barbaro;R. Demina;J. L. Dulemba;C. Fallon;T. Ferbel;M. Galanti;A. Garcia-Bellido;O. Hindrichs;A. Khukhunaishvili;E. Ranken;C. L. Tan;R. Taus;G. P. Van Onsem;K. Goulianos;B. Chiarito;J. P. Chou;A. Gandrakota;Y. Gershtein;E. Halkiadakis;A. Hart;M. Heindl;O. Karacheban;I. Laflotte;A. Lath;R. Montalvo;K. Nash;M. Osherson;S. Salur;S. Schnetzer;S. Somalwar;R. Stone;S. A. Thayil;S. Thomas;H. Wang;H. Acharya;A. G. Delannoy;S. Fiorendi;S. Spanier;O. Bouhali;M. Dalchenko;A. Delgado;R. Eusebi;J. Gilmore;T. Huang;T. Kamon;H. Kim;S. Luo;S. Malhotra;R. Mueller;D. Overton;D. Rathjens;A. Safonov;N. Akchurin;J. Damgov;V. Hegde;K. Lamichhane;S. W. Lee;T. Mengke;S. Muthumuni;T. Peltola;I. Volobouev;Z. Wang;A. Whitbeck;E. Appelt;S. Greene;A. Gurrola;W. Johns;A. Melo;K. Padeken;F. Romeo;P. Sheldon;S. Tuo;J. Velkovska;M. W. Arenton;B. Cardwell;B. Cox;G. Cummings;J. Hakala;R. Hirosky;M. Joyce;A. Ledovskoy;A. Li;C. Neu;C. E. Perez Lara;B. Tannenwald;S. White;N. Poudyal;S. Banerjee;K. Black;T. Bose;S. Dasu;I. De Bruyn;P. Everaerts;C. Galloni;H. He;M. Herndon;A. Herve;U. Hussain;A. Lanaro;A. Loeliger;R. Loveless;J. Madhusudanan Sreekala;A. Mallampalli;A. Mohammadi;D. Pinna;A. Savin;V. Shang;V. Sharma;W. H. Smith;D. Teague;S. Trembath-Reichert;W. Vetens
2022
Abstract
The first collider search for dark matter arising from a strongly coupled hidden sector is presented and uses a data sample corresponding to 138 fb(-1), collected with the CMS detector at the CERN LHC, at root s = 13 TeV. The hidden sector is hypothesized to couple to the standard model (SM) via a heavy leptophobic Z' mediator produced as a resonance in proton-proton collisions. The mediator decay results in two "semivisible" jets, containing both visible matter and invisible dark matter. The final state therefore includes moderate missing energy aligned with one of the jets, a signature ignored by most dark matter searches. No structure in the dijet transverse mass spectra compatible with the signal is observed. Assuming the Z' boson has a universal coupling of 0.25 to the SM quarks, an inclusive search, relevant to any model that exhibits this kinematic behavior, excludes mediator masses of 1.5-4.0 TeV at 95% confidence level, depending on the other signal model parameters. To enhance the sensitivity of the search for this particular class of hidden sector models, a boosted decision tree (BDT) is trained using jet substructure variables to distinguish between semivisible jets and SM jets from background processes. When the BDT is employed to identify each jet in the dijet system as semivisible, the mediator mass exclusion increases to 5.1 TeV, for wider ranges of the other signal model parameters. These limits exclude a wide range of strongly coupled hidden sector models for the first time.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11391/1547743
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simulazione ASN
Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione. La simulazione si basa sui dati IRIS e sugli indicatori bibliometrici alla data indicata e non tiene conto di eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori. La simulazione può differire dall'esito di un’eventuale domanda ASN sia per errori di catalogazione e/o dati mancanti in IRIS, sia per la variabilità dei dati bibliometrici nel tempo. Si consideri che Anvur calcola i valori degli indicatori all'ultima data utile per la presentazione delle domande.
La presente simulazione è stata realizzata sulla base delle specifiche raccolte sul tavolo ER del Focus Group IRIS coordinato dall’Università di Modena e Reggio Emilia e delle regole riportate nel DM 589/2018 e allegata Tabella A. Cineca, l’Università di Modena e Reggio Emilia e il Focus Group IRIS non si assumono alcuna responsabilità in merito all’uso che il diretto interessato o terzi faranno della simulazione. Si specifica inoltre che la simulazione contiene calcoli effettuati con dati e algoritmi di pubblico dominio e deve quindi essere considerata come un mero ausilio al calcolo svolgibile manualmente o con strumenti equivalenti.