Attenzione: i dati modificati non sono ancora stati salvati. Per confermare inserimenti o cancellazioni di voci è necessario confermare con il tasto SALVA/INSERISCI in fondo alla pagina
IRIS Institutional Research Information System - AIR Archivio Istituzionale della Ricerca
The Deep Underground Neutrino Experiment (DUNE) will produce world-leading neutrino oscillation measurements over the lifetime of the experiment. In this work, we explore DUNE's sensitivity to observe charge-parity violation (CPV) in the neutrino sector, and to resolve the mass ordering, for exposures of up to 100 kiloton-megawatt-years (kt-MW-yr). The analysis includes detailed uncertainties on the flux prediction, the neutrino interaction model, and detector effects. We demonstrate that DUNE will be able to unambiguously resolve the neutrino mass ordering at a 3σ (5σ) level, with a 66 (100) kt-MW-yr far detector exposure, and has the ability to make strong statements at significantly shorter exposures depending on the true value of other oscillation parameters. We also show that DUNE has the potential to make a robust measurement of CPV at a 3σ level with a 100 kt-MW-yr exposure for the maximally CP-violating values $delta_{m CP}} = pmpi/2$. Additionally, the dependence of DUNE's sensitivity on the exposure taken in neutrino-enhanced and antineutrino-enhanced running is discussed. An equal fraction of exposure taken in each beam mode is found to be close to optimal when considered over the entire space of interest.
Low exposure long-baseline neutrino oscillation sensitivity of the DUNE experiment / A. Abed Abud, B.A.. - In: PHYSICAL REVIEW D. - ISSN 2470-0010. - 106:7(2022 Apr 25), pp. 072006.1-072006.32. [10.1103/PhysRevD.105.072006]
Low exposure long-baseline neutrino oscillation sensitivity of the DUNE experiment
A. Abed Abud;B. Abi;R. Acciarri;M. A. Acero;M. R. Adames;G. Adamov;D. Adams;M. Adinolfi;A. Aduszkiewicz;J. Aguilar;Z. Ahmad;J. Ahmed;B. Aimard;B. Ali-Mohammadzadeh;T. Alion;K. Allison;S. Alonso Monsalve;M. AlRashed;C. Alt;A. Alton;P. Amedo;J. Anderson;C. Andreopoulos;M. Andreotti;M. P. Andrews;F. Andrianala;S. Andringa;N. Anfimov;A. Ankowski;M. Antoniassi;M. Antonova;A. Antoshkin;S. Antusch;A. Aranda-Fernandez;L. O. Arnold;M. A. Arroyave;J. Asaadi;L. Asquith;A. Aurisano;V. Aushev;D. Autiero;M. Ayala-Torres;F. Azfar;A. Back;H. Back;J. J. Back;C. Backhouse;I. Bagaturia;L. Bagby;N. Balashov;S. Balasubramanian;P. Baldi;B. Baller;B. Bambah;F. Barao;G. Barenboim;G. J. Barker;W. Barkhouse;C. Barnes;G. Barr;J. Barranco Monarca;A. Barros;N. Barros;J. L. Barrow;A. Basharina-Freshville;A. Bashyal;V. Basque;E. Belchior;J. B. R. Battat;F. Battisti;F. Bay;J. L. Bazo Alba;J. F. Beacom;E. Bechetoille;B. Behera;L. Bellantoni;G. Bellettini;V. Bellini;O. Beltramello;N. Benekos;C. Benitez Montiel;F. Bento Neves;J. Berger;S. Berkman;P. Bernardini;R. M. Berner;S. Bertolucci;M. Betancourt;A. Betancur Rodríguez;A. Bevan;Y. Bezawada;T. J. C. Bezerra;A. Bhardwaj;V. Bhatnagar;M. Bhattacharjee;S. Bhuller;B. Bhuyan;S. Biagi;J. Bian;M. Biassoni;K. Biery;B. Bilki;M. Bishai;A. Bitadze;A. Blake;F. D. M. Blaszczyk;G. C. Blazey;E. Blucher;J. Boissevain;S. Bolognesi;T. Bolton;L. Bomben;M. Bonesini;M. Bongrand;C. Bonilla-Diaz;F. Bonini;A. Booth;F. Boran;S. Bordoni;A. Borkum;N. Bostan;P. Bour;C. Bourgeois;D. Boyden;J. Bracinik;D. Braga;D. Brailsford;A. Branca;A. Brandt;J. Bremer;C. Brew;S. J. Brice;C. Brizzolari;C. Bromberg;J. Brooke;A. Bross;G. Brunetti;M. Brunetti;N. Buchanan;H. Budd;I. Butorov;I. Cagnoli;D. Caiulo;R. Calabrese;P. Calafiura;J. Calcutt;M. Calin;S. Calvez;E. Calvo;A. Caminata;M. Campanelli;D. Caratelli;G. Carini;B. Carlus;M. F. Carneiro;P. Carniti;I. Caro Terrazas;H. Carranza;T. Carroll;J. F. Castaño Forero;A. Castillo;C. Castromonte;E. Catano-Mur;C. Cattadori;F. Cavalier;F. Cavanna;S. Centro;G. Cerati;A. Cervelli;A. Cervera Villanueva;M. Chalifour;A. Chappell;E. Chardonnet;N. Charitonidis;A. Chatterjee;S. Chattopadhyay;H. Chen;M. Chen;Y. Chen;Z. Chen;Y. Cheon;D. Cherdack;C. Chi;S. Childress;A. Chiriacescu;G. Chisnall;K. Cho;S. Choate;D. Chokheli;P. S. Chong;A. Christensen;D. Christian;G. Christodoulou;A. Chukanov;M. Chung;E. Church;V. Cicero;P. Clarke;T. E. Coan;A. G. Cocco;J. A. B. Coelho;N. Colton;E. Conley;R. Conley;J. M. Conrad;M. Convery;S. Copello;L. Cremaldi;L. Cremonesi;J. I. Crespo-Anadón;M. Crisler;E. Cristaldo;R. Cross;A. Cudd;C. Cuesta;Y. Cui;D. Cussans;O. Dalager;H. da Motta;L. Da Silva Peres;C. David;Q. David;G. S. Davies;S. Davini;J. Dawson;K. De;P. Debbins;I. De Bonis;M. P. Decowski;A. de Gouvêa;P. C. De Holanda;I. L. De Icaza Astiz;A. Deisting;P. De Jong;A. Delbart;D. Delepine;M. Delgado;A. Dell'Acqua;P. De Lurgio;J. R. T. de Mello Neto;D. M. DeMuth;S. Dennis;C. Densham;G. W. Deptuch;A. De Roeck;V. De Romeri;G. De Souza;R. Devi;R. Dharmapalan;M. Dias;F. Diaz;J. S. Díaz;S. Di Domizio;L. Di Giulio;P. Ding;L. Di Noto;C. Distefano;R. Diurba;M. Diwan;Z. Djurcic;D. Doering;S. Dolan;F. Dolek;M. J. Dolinski;L. Domine;D. Douglas;D. Douillet;G. Drake;F. Drielsma;L. Duarte;D. Duchesneau;K. Duffy;P. Dunne;H. Duyang;O. Dvornikov;D. A. Dwyer;A. S. Dyshkant;M. Eads;A. Earle;D. Edmunds;J. Eisch;L. Emberger;S. Emery;A. Ereditato;T. Erjavec;C. O. Escobar;G. Eurin;J. J. Evans;E. Ewart;A. C. Ezeribe;K. Fahey;A. Falcone;M. Fani';C. Farnese;Y. Farzan;D. Fedoseev;J. Felix;Y. Feng;E. Fernandez-Martinez;P. Fernandez Menendez;M. Fernandez Morales;F. Ferraro;L. Fields;P. Filip;F. Filthaut;A. Fiorentini;M. Fiorini;R. S. Fitzpatrick;W. Flanagan;B. Fleming;R. Flight;S. Fogarty;W. Foreman;D. V. Forero;J. Fowler;W. Fox;J. Franc;K. Francis;D. Franco;J. Freeman;J. Freestone;J. Fried;A. Friedland;F. Fuentes Robayo;S. Fuess;I. K. Furic;A. P. Furmanski;A. Gabrielli;A. Gago;H. Gallagher;A. Gallas;A. Gallego-Ros;N. Gallice;V. Galymov;E. Gamberini;T. Gamble;F. Ganacim;R. Gandhi;R. Gandrajula;F. Gao;S. Gao;D. Garcia-Gamez;M. Á. García-Peris;S. Gardiner;D. Gastler;J. Gauvreau;G. Ge;N. Geffroy;B. Gelli;A. Gendotti;S. Gent;Z. Ghorbani-Moghaddam;P. Giammaria;T. Giammaria;D. Gibin;I. Gil-Botella;S. Gilligan;C. Girerd;A. K. Giri;D. Gnani;O. Gogota;M. Gold;S. Gollapinni;K. Gollwitzer;R. A. Gomes;L. V. Gomez Bermeo;L. S. Gomez Fajardo;F. Gonnella;J. A. Gonzalez-Cuevas;D. Gonzalez-Diaz;M. Gonzalez-Lopez;M. C. Goodman;O. Goodwin;S. Goswami;C. Gotti;E. Goudzovski;C. Grace;R. Gran;E. Granados;P. Granger;A. Grant;C. Grant;D. Gratieri;P. Green;L. Greenler;J. Greer;J. Grenard;W. C. Griffith;M. Groh;J. Grudzinski;K. Grzelak;W. Gu;E. Guardincerri;V. Guarino;M. Guarise;R. Guenette;E. Guerard;M. Guerzoni;D. Guffanti;A. Guglielmi;B. Guo;V. Gupta;K. K. Guthikonda;R. Gutierrez;P. Guzowski;M. M. Guzzo;S. Gwon;C. Ha;A. Habig;H. Hadavand;R. Haenni;A. Hahn;J. Haiston;P. Hamacher-Baumann;T. Hamernik;P. Hamilton;J. Han;D. A. Harris;J. Hartnell;T. Hartnett;J. Harton;T. Hasegawa;C. Hasnip;R. Hatcher;K. W. Hatfield;A. Hatzikoutelis;C. Hayes;K. Hayrapetyan;J. Hays;E. Hazen;M. He;A. Heavey;K. M. Heeger;J. Heise;S. Henry;M. A. Hernandez Morquecho;K. Herner;J. Hewes;T. Hill;S. J. Hillier;A. Himmel;E. Hinkle;L. R. Hirsch;J. Ho;J. Hoff;A. Holin;E. Hoppe;G. A. Horton-Smith;M. Hostert;A. Hourlier;B. Howard;R. Howell;I. Hristova;M. S. Hronek;J. Huang;G. Iles;N. Ilic;A. M. Iliescu;R. Illingworth;G. Ingratta;A. Ioannisian;B. Irwin;L. Isenhower;R. Itay;C. M. Jackson;V. Jain;E. James;W. Jang;B. Jargowsky;F. Jediny;D. Jena;Y. S. Jeong;C. Jesús-Valls;X. Ji;L. Jiang;S. Jiménez;A. Jipa;R. Johnson;N. Johnston;B. Jones;S. B. Jones;M. Judah;C. K. Jung;T. Junk;Y. Jwa;M. Kabirnezhad;A. Kaboth;I. Kadenko;D. Kaira;I. Kakorin;A. Kalitkina;F. Kamiya;N. Kaneshige;G. Karagiorgi;G. Karaman;A. Karcher;M. Karolak;Y. Karyotakis;S. Kasai;S. P. Kasetti;L. Kashur;N. Kazaryan;E. Kearns;P. Keener;K. J. Kelly;E. Kemp;O. Kemularia;W. Ketchum;S. H. Kettell;M. Khabibullin;A. Khotjantsev;A. Khvedelidze;D. Kim;B. King;B. Kirby;M. Kirby;J. Klein;K. Koehler;L. W. Koerner;D. H. Koh;S. Kohn;P. P. Koller;L. Kolupaeva;D. Korablev;M. Kordosky;T. Kosc;U. Kose;V. A. Kostelecký;K. Kothekar;L. Kreczko;F. Krennrich;I. Kreslo;W. Kropp;Y. Kudenko;V. A. Kudryavtsev;S. Kulagin;J. Kumar;P. Kumar;P. Kunze;N. Kurita;C. Kuruppu;V. Kus;T. Kutter;J. Kvasnicka;D. Kwak;A. Lambert;B. J. Land;C. E. Lane;K. Lang;T. Langford;M. Langstaff;J. Larkin;P. Lasorak;D. Last;C. Lastoria;A. Laundrie;G. Laurenti;A. Lawrence;I. Lazanu;R. LaZur;M. Lazzaroni;T. Le;S. Leardini;J. Learned;P. LeBrun;T. LeCompte;C. Lee;S. Y. Lee;G. Lehmann Miotto;R. Lehnert;M. A. Leigui de Oliveira;M. Leitner;L. M. Lepin;S. W. Li;T. Li;Y. Li;H. Liao;C. S. Lin;Q. Lin;S. Lin;R. A. Lineros;J. Ling;A. Lister;B. R. Littlejohn;J. Liu;S. Lockwitz;T. Loew;M. Lokajicek;I. Lomidze;K. Long;T. Lord;J. M. LoSecco;W. C. Louis;X. -G. Lu;K. B. Luk;B. Lunday;X. Luo;E. Luppi;T. Lux;V. P. Luzio;D. MacFarlane;A. A. Machado;P. Machado;C. T. Macias;J. R. Macier;A. Maddalena;A. Madera;P. Madigan;S. Magill;K. Mahn;A. Maio;A. Major;J. A. Maloney;G. Mandrioli;R. C. Mandujano;J. Maneira;L. Manenti;S. Manly;A. Mann;K. Manolopoulos;M. Manrique Plata;V. N. Manyam;L. Manzanillas;M. Marchan;A. Marchionni;W. Marciano;D. Marfatia;C. Mariani;J. Maricic;R. Marie;F. Marinho;A. D. Marino;D. Marsden;M. Marshak;C. M. Marshall;J. Marshall;J. Marteau;J. Martin-Albo;N. Martinez;D. A. Martinez Caicedo;P. Martínez Miravé;S. Martynenko;V. Mascagna;K. Mason;A. Mastbaum;F. Matichard;S. Matsuno;J. Matthews;C. Mauger;N. Mauri;K. Mavrokoridis;I. Mawby;R. Mazza;A. Mazzacane;E. Mazzucato;T. McAskill;E. McCluskey;N. McConkey;K. S. McFarland;C. McGrew;A. McNab;A. Mefodiev;P. Mehta;P. Melas;O. Mena;H. Mendez;P. Mendez;D. P. Méndez;A. Menegolli;G. Meng;M. D. Messier;W. Metcalf;T. Mettler;M. Mewes;H. Meyer;T. Miao;G. Michna;T. Miedema;V. Mikola;R. Milincic;G. Miller;W. Miller;J. Mills;C. Milne;O. Mineev;A. Minotti;O. G. Miranda;S. Miryala;C. S. Mishra;S. R. Mishra;A. Mislivec;D. Mladenov;I. Mocioiu;K. Moffat;N. Moggi;R. Mohanta;T. A. Mohayai;N. Mokhov;J. Molina;L. Molina Bueno;E. Montagna;A. Montanari;C. Montanari;D. Montanari;L. M. Montano Zetina;J. Moon;S. H. Moon;M. Mooney;A. F. Moor;D. Moreno;C. Morris;C. Mossey;E. Motuk;C. A. Moura;J. Mousseau;G. Mouster;W. Mu;L. Mualem;J. Mueller;M. Muether;S. Mufson;F. Muheim;A. Muir;M. Mulhearn;D. Munford;H. Muramatsu;S. Murphy;J. Musser;J. Nachtman;S. Nagu;M. Nalbandyan;R. Nandakumar;D. Naples;S. Narita;A. Nath;A. Navrer-Agasson;N. Nayak;M. Nebot-Guinot;K. Negishi;J. K. Nelson;J. Nesbit;M. Nessi;D. Newbold;M. Newcomer;D. Newhart;H. Newton;R. Nichol;F. Nicolas-Arnaldos;E. Niner;K. Nishimura;A. Norman;A. Norrick;R. Northrop;P. Novella;J. A. Nowak;M. Oberling;J. P. Ochoa-Ricoux;A. Olivier;A. Olshevskiy;Y. Onel;Y. Onishchuk;J. Ott;L. Pagani;S. Pakvasa;G. Palacio;O. Palamara;S. Palestini;J. M. Paley;M. Pallavicini;C. Palomares;J. L. Palomino-Gallo;W. Panduro Vazquez;E. Pantic;V. Paolone;V. Papadimitriou;R. Papaleo;A. Papanestis;S. Paramesvaran;S. Parke;E. Parozzi;Z. Parsa;M. Parvu;S. Pascoli;L. Pasqualini;J. Pasternak;J. Pater;C. Patrick;L. Patrizii;R. B. Patterson;S. J. Patton;T. Patzak;A. Paudel;B. Paulos;L. Paulucci;Z. Pavlovic;G. Pawloski;D. Payne;V. Pec;S. J. M. Peeters;E. Pennacchio;A. Penzo;O. L. G. Peres;J. Perry;D. Pershey;G. Pessina;G. Petrillo;C. Petta;R. Petti;V. Pia;F. Piastra;L. Pickering;F. Pietropaolo;R. Plunkett;R. Poling;X. Pons;N. Poonthottathil;F. Poppi;S. Pordes;J. Porter;M. Potekhin;R. Potenza;B. V. K. S. Potukuchi;J. Pozimski;M. Pozzato;S. Prakash;T. Prakash;M. Prest;S. Prince;F. Psihas;D. Pugnere;X. Qian;J. L. Raaf;V. Radeka;J. Rademacker;B. Radics;A. Rafique;E. Raguzin;M. Rai;M. Rajaoalisoa;I. Rakhno;A. Rakotonandrasana;L. Rakotondravohitra;Y. A. Ramachers;R. Rameika;M. A. Ramirez Delgado;B. Ramson;A. Rappoldi;G. Raselli;P. Ratoff;S. Raut;R. F. Razakamiandra;E. Rea;J. S. Real;B. Rebel;M. Reggiani-Guzzo;T. Rehak;J. Reichenbacher;S. D. Reitzner;H. Rejeb Sfar;A. Renshaw;S. Rescia;F. Resnati;A. Reynolds;M. Ribas;S. Riboldi;C. Riccio;G. Riccobene;L. C. J. Rice;J. Ricol;A. Rigamonti;Y. Rigaut;D. Rivera;A. Robert;L. Rochester;M. Roda;P. Rodrigues;M. J. Rodriguez Alonso;E. Rodriguez Bonilla;J. Rodriguez Rondon;S. Rosauro-Alcaraz;M. Rosenberg;P. Rosier;B. Roskovec;M. Rossella;M. Rossi;J. Rout;P. Roy;A. Rubbia;C. Rubbia;B. Russell;D. Ruterbories;A. Rybnikov;A. Saa-Hernandez;R. Saakyan;S. Sacerdoti;T. Safford;N. Sahu;P. Sala;N. Samios;O. Samoylov;M. C. Sanchez;V. Sandberg;D. A. Sanders;D. Sankey;S. Santana;M. Santos-Maldonado;N. Saoulidou;P. Sapienza;C. Sarasty;I. Sarcevic;G. Savage;V. Savinov;A. Scaramelli;A. Scarff;A. Scarpelli;H. Schellman;S. Schifano;P. Schlabach;D. Schmitz;K. Scholberg;A. Schukraft;E. Segreto;A. Selyunin;C. R. Senise;J. Sensenig;M. Seoane;A. Sergi;D. Sgalaberna;M. H. Shaevitz;S. Shafaq;M. Shamma;R. Sharankova;H. R. Sharma;R. Sharma;R. Kumar;T. Shaw;C. Shepherd-Themistocleous;A. Sheshukov;S. Shin;I. Shoemaker;D. Shooltz;R. Shrock;H. Siegel;L. Simard;F. Simon;J. Sinclair;G. Sinev;Jaydip Singh;J. Singh;L. Singh;V. Singh;R. Sipos;F. W. Sippach;G. Sirri;A. Sitraka;K. Siyeon;K. Skarpaas;A. Smith;E. Smith;P. Smith;J. Smolik;M. Smy;E. L. Snider;P. Snopok;D. Snowden-Ifft;M. Soares Nunes;H. Sobel;M. Soderberg;S. Sokolov;C. J. Solano Salinas;S. Söldner-Rembold;S. R. Soleti;N. Solomey;V. Solovov;W. E. Sondheim;M. Sorel;A. Sotnikov;J. Soto-Oton;A. Sousa;K. Soustruznik;F. Spagliardi;M. Spanu;J. Spitz;N. J. C. Spooner;K. Spurgeon;M. Stancari;L. Stanco;R. Stein;H. M. Steiner;A. F. Steklain Lisbôa;J. Stewart;B. Stillwell;J. Stock;F. Stocker;T. Stokes;M. Strait;T. Strauss;A. Stuart;J. G. Suarez;H. Sullivan;D. Summers;A. Surdo;V. Susic;L. Suter;C. M. Sutera;R. Svoboda;B. Szczerbinska;A. M. Szelc;H. A. Tanaka;B. Tapia Oregui;A. Tapper;S. Tariq;E. Tatar;R. Tayloe;A. M. Teklu;M. Tenti;K. Terao;C. A. Ternes;F. Terranova;G. Testera;T. Thakore;A. Thea;J. L. Thompson;C. Thorn;S. C. Timm;V. Tishchenko;L. Tomassetti;A. Tonazzo;D. Torbunov;M. Torti;M. Tortola;F. Tortorici;N. Tosi;D. Totani;M. Toups;C. Touramanis;R. Travaglini;J. Trevor;S. Trilov;W. H. Trzaska;Y. Tsai;Y. -T. Tsai;Z. Tsamalaidze;K. V. Tsang;N. Tsverava;S. Tufanli;C. Tull;E. Tyley;M. Tzanov;L. Uboldi;M. A. Uchida;J. Urheim;T. Usher;S. Uzunyan;M. R. Vagins;P. Vahle;G. A. Valdiviesso;R. Valentim;Z. Vallari;E. Vallazza;J. W. F. Valle;S. Vallecorsa;R. Van Berg;R. G. Van de Water;F. Varanini;D. Vargas;G. Varner;J. Vasel;S. Vasina;G. Vasseur;N. Vaughan;K. Vaziri;S. Ventura;A. Verdugo;S. Vergani;M. A. Vermeulen;M. Verzocchi;M. Vicenzi;H. Vieira de Souza;C. Vignoli;C. Vilela;B. Viren;T. Vrba;T. Wachala;A. V. Waldron;M. Wallbank;C. Wallis;H. Wang;J. Wang;L. Wang;M. H. L. S. Wang;Y. Wang;Y. Wang;K. Warburton;D. Warner;M. O. Wascko;D. Waters;A. Watson;P. Weatherly;A. Weber;M. Weber;H. Wei;A. Weinstein;D. Wenman;M. Wetstein;A. White;L. H. Whitehead;D. Whittington;M. J. Wilking;C. Wilkinson
The Deep Underground Neutrino Experiment (DUNE) will produce world-leading neutrino oscillation measurements over the lifetime of the experiment. In this work, we explore DUNE's sensitivity to observe charge-parity violation (CPV) in the neutrino sector, and to resolve the mass ordering, for exposures of up to 100 kiloton-megawatt-years (kt-MW-yr). The analysis includes detailed uncertainties on the flux prediction, the neutrino interaction model, and detector effects. We demonstrate that DUNE will be able to unambiguously resolve the neutrino mass ordering at a 3σ (5σ) level, with a 66 (100) kt-MW-yr far detector exposure, and has the ability to make strong statements at significantly shorter exposures depending on the true value of other oscillation parameters. We also show that DUNE has the potential to make a robust measurement of CPV at a 3σ level with a 100 kt-MW-yr exposure for the maximally CP-violating values $delta_{m CP}} = pmpi/2$. Additionally, the dependence of DUNE's sensitivity on the exposure taken in neutrino-enhanced and antineutrino-enhanced running is discussed. An equal fraction of exposure taken in each beam mode is found to be close to optimal when considered over the entire space of interest.
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/868942
Citazioni
ND
38
30
ND
social impact
Conferma cancellazione
Sei sicuro che questo prodotto debba essere cancellato?
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.