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Received 23 May 2018
Received in revised form 28 October 2018 Accepted 12 November 2018
Available online 29 December 2018 Editor: M. Doser
1. Introduction
A detailed study of the properties of the Quark–Gluon Plasma (QGP) [1] is the main goal of heavy-ion experiments at ultra- relativistic energies [2–6]. Quarkonia, i.e. bound states of charm or bottom quark–antiquark pairs, are sensitive probes of color decon- finement, due to the Quantum-Chromo Dynamics Debye screening mechanism [7–9] leading to quarkonium suppression. Moreover, the various quarkonium states have different binding energies and therefore different dissociation temperatures in a QGP, leading to sequential suppression [7,10]. Theory estimates [11] indicate that bottomonium formation may occur before QGP thermalization [12] because of the large bottom quark mass. In this situation, a quan- titative description of the influence of the medium on the bound states becomes challenging. While the dissociation temperatures vary significantly between different models [8,9], it is commonly accepted that the widths of the spectral functions of the bottomo- nium states increase compared to the widths in vacuum, due to the high temperature of the surrounding medium [13]. Finally, taking into account that feed-down processes from higher-mass resonances (around 40% for the Υ(1S) and 30% for the Υ(2S) [9]) are not negligible, the evaluation of the medium temperature via bottomonium measurements remains a complex endeavour.
The first studies of quarkonium production in heavy-ion colli- sions were devoted to charmonium states, and a suppression of their yields was observed at the SPS [14–16], at RHIC [17,18] and
⋆ E-mail address: alice-publications@cern.ch.
abstract
Inclusive Υ(1S) and Υ(2S) production have been measured in Pb–Pb collisions at the centre-of-mass
energy per nucleon–nucleon pair √sNN = 5.02 TeV, using the ALICE detector at the CERN LHC. The Υ
mesons are reconstructed in the centre-of-mass rapidity interval 2.5 < y < 4 and in the transverse-
momentum range pT < 15 GeV/c, via their decays to muon pairs. In this Letter, we present results
on the inclusive Υ(1S) nuclear modification factor RAA as a function of collision centrality, transverse
momentum and rapidity. The Υ(1S) and Υ(2S) RAA, integrated over the centrality range 0–90%, are 0.37±
0.02(stat) ± 0.03(syst) and 0.10 ± 0.04(stat) ± 0.02(syst), respectively, leading to a ratio RΥ(2S)/RΥ(1S) of AA AA
0.28±0.12(stat)±0.06(syst). The observed Υ(1S) suppression increases with the centrality of the collision and no significant variation is observed as a function of transverse momentum and rapidity.
ϒ suppression at forward rapidity in Pb–Pb collisions at sNN=5.02TeV
Acharya S.;Acosta F. T.;Adamova D.;Adolfsson J.;Aggarwal M. M.;Aglieri Rinella G.;Agnello M.;Agrawal N.;Ahammed Z.;Ahn S. U.;Aiola S.;Akindinov A.;Al-Turany M.;Alam S. N.;Albuquerque D. S. D.;Aleksandrov D.;Alessandro B.;Alfaro Molina R.;Ali Y.;Alici A.;Alkin A.;Alme J.;Alt T.;Altenkamper L.;Altsybeev I.;Anaam M. N.;Andrei C.;Andreou D.;Andrews H. A.;Andronic A.;Angeletti M.;Anguelov V.;Anson C.;Anticic T.;Antinori F.;Antonioli P.;Anwar R.;Apadula N.;Aphecetche L.;Appelshauser H.;Arcelli S.;Arnaldi R.;Arnold O. W.;Arsene I. C.;Arslandok M.;Audurier B.;Augustinus A.;Averbeck R.;Azmi M. D.;Badala A.;Baek Y. W.;Bagnasco S.;Bailhache R.;Bala R.;Baldisseri A.;Ball M.;Baral R. C.;Barbano A. M.;Barbera R.;Barile F.;Barioglio L.;Barnafoldi G. G.;Barnby L. S.;Barret V.;Bartalini P.;Barth K.;Bartsch E.;Bastid N.;Basu S.;Batigne G.;Batyunya B.;Batzing P. C.;Bazo Alba J. L.;Bearden I. G.;Beck H.;Bedda C.;Behera N. K.;Belikov I.;Bellini F.;Bello Martinez H.;Bellwied R.;Beltran L. G. E.;Belyaev V.;Bencedi G.;Beole S.;Bercuci A.;Berdnikov Y.;Berenyi D.;Bertens R. A.;Berzano D.;Betev L.;Bhaduri P. P.;Bhasin A.;Bhat I. R.;Bhatt H.;Bhattacharjee B.;Bhom J.;Bianchi A.;Bianchi L.;Bianchi N.;Bielcik J.;Bielcikova J.;Bilandzic A.;Biro G.;Biswas R.;Biswas S.;Blair J. T.;Blau D.;Blume C.;Boca G.;Bock F.;Bogdanov A.;Boldizsar L.;Bombara M.;Bonomi G.;Bonora M.;Borel H.;Borissov A.;Borri M.;Botta E.;Bourjau C.;Bratrud L.;Braun-Munzinger P.;Bregant M.;Broker T. A.;Broz M.;Brucken E. J.;Bruna E.;Bruno G. E.;Budnikov D.;Buesching H.;Bufalino S.;Buhler P.;Buncic P.;Busch O.;Buthelezi Z.;Butt J. B.;Buxton J. T.;Cabala J.;Caffarri D.;Caines H.;Caliva A.;Calvo Villar E.;Camacho R. S.;Camerini P.;Capon A. A.;Carena F.;Carena W.;Carnesecchi F.;Castillo Castellanos J.;Castro A. J.;Casula E. A. R.;Ceballos Sanchez C.;Chandra S.;Chang B.;Chang W.;Chapeland S.;Chartier M.;Chattopadhyay S.;Chauvin A.;Cheshkov C.;Cheynis B.;Chibante Barroso V.;Chinellato D. D.;Cho S.;Chochula P.;Chowdhury T.;Christakoglou P.;Christensen C. H.;Christiansen P.;Chujo T.;Chung S. U.;Cicalo C.;Cifarelli L.;Cindolo F.;Cleymans J.;Colamaria F.;Colella D.;Collu A.;Colocci M.;Concas M.;Conesa Balbastre G.;Conesa del Valle Z.;Contreras J. G.;Cormier T. M.;Corrales Morales Y.;Cortese P.;Cosentino M. R.;Costa F.;Costanza S.;Crkovska J.;Crochet P.;Cuautle E.;Cunqueiro L.;Dahms T.;Dainese A.;Dani S.;Danisch M. C.;Danu A.;Das D.;Das I.;Das S.;Dash A.;Dash S.;De S.;De Caro A.;de Cataldo G.;de Conti C.;de Cuveland J.;De Falco A.;De Gruttola D.;De Marco N.;De Pasquale S.;De Souza R. D.;Degenhardt H. F.;Deisting A.;Deloff A.;Delsanto S.;Deplano C.;Dhankher P.;Di Bari D.;Di Mauro A.;Di Ruzza B.;Diaz R. A.;Dietel T.;Dillenseger P.;Ding Y.;Divia R.;Djuvsland O.;Dobrin A.;Domenicis Gimenez D.;Donigus B.;Dordic O.;Doremalen L. V. R.;Dubey A. K.;Dubla A.;Ducroux L.;Dudi S.;Duggal A. K.;Dukhishyam M.;Dupieux P.;Ehlers R. J.;Elia D.;Endress E.;Engel H.;Epple E.;Erazmus B.;Erhardt F.;Ersdal M. R.;Espagnon B.;Eulisse G.;Eum J.;Evans D.;Evdokimov S.;Fabbietti L.;Faggin M.;Faivre J.;Fantoni A.;Fasel M.;Feldkamp L.;Feliciello A.;Feofilov G.;Fernandez Tellez A.;Ferretti A.;Festanti A.;Feuillard V. J. G.;Figiel J.;Figueredo M. A. S.;Filchagin S.;Finogeev D.;Fionda F. M.;Fiorenza G.;Flor F.;Floris M.;Foertsch S.;Foka P.;Fokin S.;Fragiacomo E.;Francescon A.;Francisco A.;Frankenfeld U.;Fronze G. G.;Fuchs U.;Furget C.;Furs A.;Fusco Girard M.;Gaardhoje J. J.;Gagliardi M.;Gago A. M.;Gajdosova K.;Gallio M.;Galvan C. D.;Ganoti P.;Garabatos C.;Garcia-Solis E.;Garg K.;Gargiulo C.;Gasik P.;Gauger E. F.;Gay Ducati M. B.;Germain M.;Ghosh J.;Ghosh P.;Ghosh S. K.;Gianotti P.;Giubellino P.;Giubilato P.;Glassel P.;Gomez Coral D. M.;Gomez Ramirez A.;Gonzalez V.;Gonzalez-Zamora P.;Gorbunov S.;Gorlich L.;Gotovac S.;Grabski V.;Graczykowski L. K.;Graham K. L.;Greiner L.;Grelli A.;Grigoras C.;Grigoriev V.;Grigoryan A.;Grigoryan S.;Gronefeld J. M.;Grosa F.;Grosse-Oetringhaus J. F.;Grosso R.;Guernane R.;Guerzoni B.;Guittiere M.;Gulbrandsen K.;Gunji T.;Gupta A.;Gupta R.;Guzman I. B.;Haake R.;Habib M. K.;Hadjidakis C.;Hamagaki H.;Hamar G.;Hamid M.;Hamon J. C.;Hannigan R.;Haque M. R.;Harris J. W.;Harton A.;Hassan H.;Hatzifotiadou D.;Hayashi S.;Heckel S. T.;Hellbar E.;Helstrup H.;Herghelegiu A.;Hernandez E. G.;Herrera Corral G.;Herrmann F.;Hetland K. F.;Hilden T. E.;Hillemanns H.;Hills C.;Hippolyte B.;Hohlweger B.;Horak D.;Hornung S.;Hosokawa R.;Hota J.;Hristov P.;Huang C.;Hughes C.;Huhn P.;Humanic T. J.;Hushnud H.;Hussain N.;Hussain T.;Hutter D.;Hwang D. S.;Iddon J. P.;Iga Buitron S. A.;Ilkaev R.;Inaba M.;Ippolitov M.;Islam M. S.;Ivanov M.;Ivanov V.;Izucheev V.;Jacak B.;Jacazio N.;Jacobs P. M.;Jadhav M. B.;Jadlovska S.;Jadlovsky J.;Jaelani S.;Jahnke C.;Jakubowska M. J.;Janik M. A.;Jena C.;Jercic M.;Jevons O.;Jimenez Bustamante R. T.;Jin M.;Jones P. G.;Jusko A.;Kalinak P.;Kalweit A.;Kang J. H.;Kaplin V.;Kar S.;Karasu Uysal A.;Karavichev O.;Karavicheva T.;Karczmarczyk P.;Karpechev E.;Kebschull U.;Keidel R.;Keijdener D. L. D.;Keil M.;Ketzer B.;Khabanova Z.;Khan A. M.;Khan S.;Khan S. A.;Khanzadeev A.;Kharlov Y.;Khatun A.;Khuntia A.;Kielbowicz M. M.;Kileng B.;Kim B.;Kim D.;Kim D. J.;Kim E. J.;Kim H.;Kim J. S.;Kim J.;Kim M.;Kim S.;Kim T.;Kirsch S.;Kisel I.;Kiselev S.;Kisiel A.;Klay J. L.;Klein C.;Klein J.;Klein-Bosing C.;Klewin S.;Kluge A.;Knichel M. L.;Knospe A. G.;Kobdaj C.;Kofarago M.;Kohler M. K.;Kollegger T.;Kondratyeva N.;Kondratyuk E.;Konevskikh A.;Konyushikhin M.;Kovalenko O.;Kovalenko V.;Kowalski M.;Kralik I.;Kravcakova A.;Kreis L.;Krivda M.;Krizek F.;Kruger M.;Kryshen E.;Krzewicki M.;Kubera A. M.;Kucera V.;Kuhn C.;Kuijer P. G.;Kumar J.;Kumar L.;Kumar S.;Kundu S.;Kurashvili P.;Kurepin A.;Kurepin A. B.;Kuryakin A.;Kushpil S.;Kvapil J.;Kweon M. J.;Kwon Y.;La Pointe S. L.;La Rocca P.;Lai Y. S.;Lakomov I.;Langoy R.;Lapidus K.;Lardeux A.;Larionov P.;Laudi E.;Lavicka R.;Lea R.;Leardini L.;Lee S.;Lehas F.;Lehner S.;Lehrbach J.;Lemmon R. C.;Leon Monzon I.;Levai P.;Li X.;Li X. L.;Lien J.;Lietava R.;Lim B.;Lindal S.;Lindenstruth V.;Lindsay S. W.;Lippmann C.;Lisa M. A.;Litichevskyi V.;Liu A.;Ljunggren H. M.;Llope W. J.;Lodato D. F.;Loginov V.;Loizides C.;Loncar P.;Lopez X.;Lopez Torres E.;Lowe A.;Luettig P.;Luhder J. R.;Lunardon M.;Luparello G.;Lupi M.;Maevskaya A.;Mager M.;Mahmood S. M.;Maire A.;Majka R. D.;Malaev M.;Malik Q. W.;Malinina L.;Mal'Kevich D.;Malzacher P.;Mamonov A.;Manko V.;Manso F.;Manzari V.;Mao Y.;Marchisone M.;Mares J.;Margagliotti G. V.;Margotti A.;Margutti J.;Marin A.;Markert C.;Marquard M.;Martin N. A.;Martinengo P.;Martinez J. L.;Martinez M. I.;Martinez Garcia G.;Martinez Pedreira M.;Masciocchi S.;Masera M.;Masoni A.;Massacrier L.;Masson E.;Mastroserio A.;Mathis A. M.;Matuoka P. F. T.;Matyja A.;Mayer C.;Mazzilli M.;Mazzoni M. A.;Meddi F.;Melikyan Y.;Menchaca-Rocha A.;Meninno E.;Mercado Perez J.;Meres M.;Meza C. S.;Mhlanga S.;Miake Y.;Micheletti L.;Mieskolainen M. M.;Mihaylov D. L.;Mikhaylov K.;Mischke A.;Mishra A. N.;Miskowiec D.;Mitra J.;Mitu C. M.;Mohammadi N.;Mohanty A. P.;Mohanty B.;Mohisin Khan M.;Moreira De Godoy D. A.;Moreno L. A. P.;Moretto S.;Morreale A.;Morsch A.;Muccifora V.;Mudnic E.;Muhlheim D.;Muhuri S.;Mukherjee M.;Mulligan J. D.;Munhoz M. G.;Munning K.;Munoz M. I. A.;Munzer R. H.;Murakami H.;Murray S.;Musa L.;Musinsky J.;Myers C. J.;Myrcha J. W.;Naik B.;Nair R.;Nandi B. K.;Nania R.;Nappi E.;Narayan A.;Naru M. U.;Nassirpour A. F.;Natal da Luz H.;Nattrass C.;Navarro S. R.;Nayak K.;Nayak R.;Nayak T. K.;Nazarenko S.;Negrao De Oliveira R. A.;Nellen L.;Nesbo S. V.;Neskovic G.;Ng F.;Nicassio M.;Niedziela J.;Nielsen B. S.;Nikolaev S.;Nikulin S.;Nikulin V.;Noferini F.;Nomokonov P.;Nooren G.;Noris J. C. C.;Norman J.;Nyanin A.;Nystrand J.;Oh H.;Ohlson A.;Oleniacz J.;Oliveira Da Silva A. C.;Oliver M. H.;Onderwaater J.;Oppedisano C.;Orava R.;Oravec M.;Ortiz Velasquez A.;Oskarsson A.;Otwinowski J.;Oyama K.;Pachmayer Y.;Pacik V.;Pagano D.;Paic G.;Palni P.;Pan J.;Pandey A. K.;Panebianco S.;Papikyan V.;Pareek P.;Park J.;Parkkila J. E.;Parmar S.;Passfeld A.;Pathak S. P.;Patra R. N.;Paul B.;Pei H.;Peitzmann T.;Peng X.;Pereira L. G.;Pereira Da Costa H.;Peresunko D.;Perez Lezama E.;Peskov V.;Pestov Y.;Petracek V.;Petrovici M.;Petta C.;Pezzi R. P.;Piano S.;Pikna M.;Pillot P.;Pimentel L. O. D. L.;Pinazza O.;Pinsky L.;Pisano S.;Piyarathna D. B.;Ploskon M.;Planinic M.;Pliquett F.;Pluta J.;Pochybova S.;Podesta-Lerma P. L. M.;Poghosyan M. G.;Polichtchouk B.;Poljak N.;Poonsawat W.;Pop A.;Poppenborg H.;Porteboeuf-Houssais S.;Pozdniakov V.;Prasad S. K.;Preghenella R.;Prino F.;Pruneau C. A.;Pshenichnov I.;Puccio M.;Punin V.;Putschke J.;Raha S.;Rajput S.;Rak J.;Rakotozafindrabe A.;Ramello L.;Rami F.;Raniwala R.;Raniwala S.;Rasanen S. S.;Rascanu B. T.;Ratza V.;Ravasenga I.;Read K. F.;Redlich K.;Rehman A.;Reichelt P.;Reidt F.;Ren X.;Renfordt R.;Reshetin A.;Revol J. -P.;Reygers K.;Riabov V.;Richert T.;Richter M.;Riedler P.;Riegler W.;Riggi F.;Ristea C.;Rode S. P.;Rodriguez Cahuantzi M.;Roed K.;Rogalev R.;Rogochaya E.;Rohr D.;Rohrich D.;Rokita P. S.;Ronchetti F.;Rosas E. D.;Roslon K.;Rosnet P.;Rossi A.;Rotondi A.;Roukoutakis F.;Roy C.;Roy P.;Rueda O. V.;Rui R.;Rumyantsev B.;Rustamov A.;Ryabinkin E.;Ryabov Y.;Rybicki A.;Saarinen S.;Sadhu S.;Sadovsky S.;Safarik K.;Saha S. K.;Sahoo B.;Sahoo P.;Sahoo R.;Sahoo S.;Sahu P. K.;Saini J.;Sakai S.;Saleh M. A.;Sambyal S.;Samsonov V.;Sandoval A.;Sarkar A.;Sarkar D.;Sarkar N.;Sarma P.;Sas M. H. P.;Scapparone E.;Scarlassara F.;Schaefer B.;Scheid H. S.;Schiaua C.;Schicker R.;Schmidt C.;Schmidt H. R.;Schmidt M. O.;Schmidt M.;Schmidt N. V.;Schukraft J.;Schutz Y.;Schwarz K.;Schweda K.;Scioli G.;Scomparin E.;Sefcik M.;Seger J. E.;Sekiguchi Y.;Sekihata D.;Selyuzhenkov I.;Senosi K.;Senyukov S.;Serradilla E.;Sett P.;Sevcenco A.;Shabanov A.;Shabetai A.;Shahoyan R.;Shaikh W.;Shangaraev A.;Sharma A.;Sharma M.;Sharma N.;Sheikh A. I.;Shigaki K.;Shimomura M.;Shirinkin S.;Shou Q.;Shtejer K.;Sibiriak Y.;Siddhanta S.;Sielewicz K. M.;Siemiarczuk T.;Silvermyr D.;Simatovic G.;Simonetti G.;Singaraju R.;Singh R.;Singhal V.;Sinha T.;Sitar B.;Sitta M.;Skaali T. B.;Slupecki M.;Smirnov N.;Snellings R. J. M.;Snellman T. W.;Song J.;Soramel F.;Sorensen S.;Sozzi F.;Sputowska I.;Stachel J.;Stan I.;Stankus P.;Stenlund E.;Stocco D.;Storetvedt M. M.;Strmen P.;Suaide A. A. P.;Sugitate T.;Suire C.;Suleymanov M.;Suljic M.;Sultanov R.;Sumbera M.;Sumowidagdo S.;Suzuki K.;Swain S.;Szabo A.;Szarka I.;Tabassam U.;Takahashi J.;Tambave G. J.;Tanaka N.;Tarhini M.;Tariq M.;Tarzila M. G.;Tauro A.;Tejeda Munoz G.;Telesca A.;Terrevoli C.;Teyssier B.;Thakur D.;Thakur S.;Thomas D.;Thoresen F.;Tieulent R.;Tikhonov A.;Timmins A. R.;Toia A.;Topilskaya N.;Toppi M.;Torres S. R.;Tripathy S.;Trogolo S.;Trombetta G.;Tropp L.;Trubnikov V.;Trzaska W. H.;Trzcinski T. P.;Trzeciak B. A.;Tsuji T.;Tumkin A.;Turrisi R.;Tveter T. S.;Ullaland K.;Umaka E. N.;Uras A.;Usai G. L.;Utrobicic A.;Vala M.;Van Hoorne J. W.;van Leeuwen M.;Vande Vyvre P.;Varga D.;Vargas A.;Vargyas M.;Varma R.;Vasileiou M.;Vasiliev A.;Vauthier A.;Vazquez Doce O.;Vechernin V.;Veen A. M.;Vercellin E.;Vergara Limon S.;Vermunt L.;Vernet R.;Vertesi R.;Vickovic L.;Viinikainen J.;Vilakazi Z.;Villalobos Baillie O.;Villatoro Tello A.;Vinogradov A.;Virgili T.;Vislavicius V.;Vodopyanov A.;Volkl M. A.;Voloshin K.;Voloshin S. A.;Volpe G.;von Haller B.;Vorobyev I.;Voscek D.;Vranic D.;Vrlakova J.;Wagner B.;Wang H.;Wang M.;Watanabe Y.;Weber M.;Weber S. G.;Wegrzynek A.;Weiser D. F.;Wenzel S. C.;Wessels J. P.;Westerhoff U.;Whitehead A. M.;Wiechula J.;Wikne J.;Wilk G.;Wilkinson J.;Willems G. A.;Williams M. C. S.;Willsher E.;Windelband B.;Witt W. E.;Xu R.;Yalcin S.;Yamakawa K.;Yano S.;Yin Z.;Yokoyama H.;Yoo I. -K.;Yoon J. H.;Yurchenko V.;Zaccolo V.;Zaman A.;Zampolli C.;Zanoli H. J. C.;Zardoshti N.;Zarochentsev A.;Zavada P.;Zaviyalov N.;Zbroszczyk H.;Zhalov M.;Zhang X.;Zhang Y.;Zhang Z.;Zhao C.;Zherebchevskii V.;Zhigareva N.;Zhou D.;Zhou Y.;Zhou Z.;Zhu H.;Zhu J.;Zhu Y.;Zichichi A.;Zimmermann M. B.;Zinovjev G.;Zmeskal J.;Zou S.
2019-01-01
Abstract
Received 23 May 2018
Received in revised form 28 October 2018 Accepted 12 November 2018
Available online 29 December 2018 Editor: M. Doser
1. Introduction
A detailed study of the properties of the Quark–Gluon Plasma (QGP) [1] is the main goal of heavy-ion experiments at ultra- relativistic energies [2–6]. Quarkonia, i.e. bound states of charm or bottom quark–antiquark pairs, are sensitive probes of color decon- finement, due to the Quantum-Chromo Dynamics Debye screening mechanism [7–9] leading to quarkonium suppression. Moreover, the various quarkonium states have different binding energies and therefore different dissociation temperatures in a QGP, leading to sequential suppression [7,10]. Theory estimates [11] indicate that bottomonium formation may occur before QGP thermalization [12] because of the large bottom quark mass. In this situation, a quan- titative description of the influence of the medium on the bound states becomes challenging. While the dissociation temperatures vary significantly between different models [8,9], it is commonly accepted that the widths of the spectral functions of the bottomo- nium states increase compared to the widths in vacuum, due to the high temperature of the surrounding medium [13]. Finally, taking into account that feed-down processes from higher-mass resonances (around 40% for the Υ(1S) and 30% for the Υ(2S) [9]) are not negligible, the evaluation of the medium temperature via bottomonium measurements remains a complex endeavour.
The first studies of quarkonium production in heavy-ion colli- sions were devoted to charmonium states, and a suppression of their yields was observed at the SPS [14–16], at RHIC [17,18] and
⋆ E-mail address: alice-publications@cern.ch.
abstract
Inclusive Υ(1S) and Υ(2S) production have been measured in Pb–Pb collisions at the centre-of-mass
energy per nucleon–nucleon pair √sNN = 5.02 TeV, using the ALICE detector at the CERN LHC. The Υ
mesons are reconstructed in the centre-of-mass rapidity interval 2.5 < y < 4 and in the transverse-
momentum range pT < 15 GeV/c, via their decays to muon pairs. In this Letter, we present results
on the inclusive Υ(1S) nuclear modification factor RAA as a function of collision centrality, transverse
momentum and rapidity. The Υ(1S) and Υ(2S) RAA, integrated over the centrality range 0–90%, are 0.37±
0.02(stat) ± 0.03(syst) and 0.10 ± 0.04(stat) ± 0.02(syst), respectively, leading to a ratio RΥ(2S)/RΥ(1S) of AA AA
0.28±0.12(stat)±0.06(syst). The observed Υ(1S) suppression increases with the centrality of the collision and no significant variation is observed as a function of transverse momentum and rapidity.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/1710786
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simulazione ASN
Il report seguente simula gli indicatori relativi alla 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 presenta gli indicatori calcolati alla data indicata sul report. Si ricorda che in sede di domanda ASN presso il MIUR gli indicatori saranno invece calcolati a partire dal 1° gennaio rispettivamente del quinto/decimo/quindicesimo anno precedente la scadenza del quadrimestre di presentazione della domanda (art 2 del DM 598/2018).
In questa simulazione pertanto il valore degli indicatori potrà differire da quello conteggiato all’atto della domanda ASN effettuata presso il MIUR a seguito di:
Correzioni imputabili a eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori.
Presenza di eventuali errori di catalogazione e/o dati mancanti in IRIS
Variabilità nel tempo dei valori citazionali (per i settori bibliometrici)
Variabilità della finestra temporale considerata in funzione della sessione di domanda ASN a cui si partecipa.
La presente simulazione è stata realizzata sulla base delle regole riportate nel DM 598/2018 e dell'allegata Tabella A e delle specifiche definite all'interno del Focus Group Cineca relativo al modulo IRIS ER. Il Cineca non si assume alcuna responsabilità in merito all'uso che il diretto interessato o terzi faranno della simulazione.