A newly developed observable for correlations between symmetry planes, which characterize the direction of the anisotropic emission of produced particles, is measured in Pb-Pb collisions at root s(NN) = 2.76 TeV with ALICE. This so-called Gaussian Estimator allows for the first time the study of these quantities without the influence of correlations between different flow amplitudes. The centrality dependence of various correlations between two, three and four symmetry planes is presented. The ordering of magnitude between these symmetry plane correlations is discussed and the results of the Gaussian Estimator are compared with measurements of previously used estimators. The results utilizing the new estimator lead to significantly smaller correlations than reported by studies using the Scalar Product method. Furthermore, the obtained symmetry plane correlations are compared to state-of-the-art hydrodynamic model calculations for the evolution of heavy-ion collisions. While the model predictions provide a qualitative description of the data, quantitative agreement is not always observed, particularly for correlators with significant non-linear response of the medium to initial state anisotropies of the collision system. As these results provide unique and independent information, their usage in future Bayesian analysis can further constrain our knowledge on the properties of the QCDmatter produced in ultrarelativistic heavy-ion collisions.
Symmetry plane correlations in Pb-Pb collisions at √sNN=2.76 TeV / Acharya, S; Adamová, D; Adler, A; Rinella, Ga; Agnello, M; Agrawal, N; Ahammed, Z; Ahmad, S; Ahn, Su; Ahuja, I; Akindinov, A; Al-Turany, M; Aleksandrov, D; Alessandro, B; Alfanda, Hm; Molina, Ra; Ali, B; Alici, A; Alizadehvandchali, N; Alkin, A; Alme, J; Alocco, G; Alt, T; Altsybeev, I; Anaam, Mn; Andrei, C; Andronic, A; Anguelov, V; Antinori, F; Antonioli, P; Apadula, N; Aphecetche, L; Appelshaeuser, H; Arata, C; Arcelli, S; Aresti, M; Arnaldi, R; Arneiro, Jgmca; Arsene, Ic; Arslandok, M; Augustinus, A; Averbeck, R; Azmi, Md; Badala, A; Bae, J; Baek, Yw; Bai, X; Bailhache, R; Bailung, Y; Balbino, A; Baldisseri, A; Balis, B; Banerjee, D; Banoo, Z; Barbera, R; Barile, F; Barioglio, L; Barlou, M; Barnafoldi, Gg; Barnby, Ls; Barret, V; Barreto, L; Bartels, C; Barth, K; Bartsch, E; Bastid, N; Basu, S; Batigne, G; Battistini, D; Batyunya, B; Bauri, D; Alba, Jlb; Bearden, Ig; Beattie, C; Becht, P; Behera, D; Belikov, I; Hechavarria, Adcb; Bellini, F; Bellwied, R; Belokurova, S; Belyaev, V; Bencedi, G; Beole, S; Bercuci, A; Berdnikov, Y; Berdnikova, A; Bergmann, L; Besoiu, Mg; Betev, L; Bhaduri, Pp; Bhasin, A; Bhat, Ma; Bhattacharjee, B; Bianchi, L; Bianchi, N; Bielcík, J; Bielcíková, J; Biernat, J; Bigot, Ap; Bilandzic, A; Biro, G; Biswas, S; Bize, N; Blair, Jt; Blau, D; Blidaru, Mb; Bluhme, N; Blume, C; Boca, G; Bock, F; Bodova, T; Bogdanov, A; Boi, S; Bok, J; Boldizsár, L; Bolozdynya, A; Bombara, M; Bond, Pm; Bonomi, G; Borel, H; Borissov, A; Carcamo, Agb; Bossi, H; Botta, E; Bouziani, Yem; Bratrud, L; Braun-Munzinger, P; Bregant, M; Broz, M; Bruno, Ge; Buckland, Md; Budnikov, D; Buesching, H; Bufalino, S; Bugnon, O; Buhler, P; Buthelezi, Z; Bysiak, Sa; Cai, M; Caines, H; Caliva, A; Villar, Ec; Camacho, Jmm; Camerini, P; Canedo, Fdm; Carabas, M; Carballo, Aa; Carnesecchi, F; Caron, R; Carvalho, Lad; Castellanos, Jc; Catalano, F; Sanchez, Cc; Chakaberia, I; Chakraborty, P; Chandra, S; Chapeland, S; Chartier, M; Chattopadhyay, S; Chattopadhyay, S; Chavez, Tg; Cheng, T; Cheshkov, C; Cheynis, B; Barroso, Vc; Chinellato, Dd; Chizzali, Es; Cho, J; Cho, S; Chochula, P; Christakoglou, P; Christensen, Ch; Christiansen, P; Chujo, T; Ciacco, M; Cicalo, C; Cindolo, F; Ciupek, Mr; Clai, G; Colamaria, F; Colburn, Js; Colella, D; Colocci, M; Concas, M; Balbastre, Gc; del Valle, Zc; Contin, G; Contreras, Jg; Coquet, Ml; Cormier, Tm; Cortese, P; Cosentino, Mr; Costa, F; Costanza, S; Cot, C; Crkovská, J; Crochet, P; Cruz-Torres, R; Cuautle, E; Cui, P; Dainese, A; Danisch, Mc; Danu, A; Das, P; Das, P; Das, S; Dash, Ar; Dash, S; De Caro, A; de Cataldo, G; de Cuveland, J; De Falco, A; De Gruttola, D; De Marco, N; De Martin, C; De Pasquale, S; Deb, S; Debski, Rj; Deja, Kr; Del Grande, R; Dello Stritto, L; Deng, W; Dhankher, P; Di Bari, D; Di Mauro, A; Diaz, Ra; Dietel, T; Ding, Y; Divia, R; Dixit, Du; Djuvsland, O; Dmitrieva, U; Dobrin, A; Doenigus, B; Dubinski, Jm; Dubla, A; Dudi, S; Dupieux, P; Durkac, M; Dzalaiova, N; Eder, Tm; Ehlers, Rj; Eikeland, Vn; Eisenhut, F; Elia, D; Erazmus, B; Ercolessi, F; Erhardt, F; Ersdal, Mr; Espagnon, B; Eulisse, G; Evans, D; Evdokimov, S; Fabbietti, L; Faggin, M; Faivre, J; Fan, F; Fan, W; Fantoni, A; Fasel, M; Fecchio, P; Feliciello, A; Feofilov, G; Tellez, Af; Ferrandi, L; Ferrer, Mb; Ferrero, A; Ferrero, C; Ferretti, A; Feuillard, Vjg; Filova, V; Finogeev, D; Fionda, Fm; Flor, F; Flores, An; Foertsch, S; Fokin, I; Fokin, S; Fragiacomo, E; Frajna, E; Fuchs, U; Funicello, N; Furget, C; Furs, A; Fusayasu, T; Gaardhoje, Jj; Gagliardi, M; Gago, Am; Galvan, Cd; Gangadharan, Dr; Ganoti, P; Garabatos, C; Garcia, Jra; Garcia-Solis, E; Garg, K; Gargiulo, C; Garner, K; Gasik, P; Gautam, A; Ducati, Mbg; Germain, M; Ghosh, C; Giacalone, M; Giubellino, P; Giubilato, P; Glaenzer, Amc; Glaessel, P; Glimos, E; Goh, Djq; Gonzalez, V; González-Trueba, Lh; Gorgon, M; Gotovac, S; Grabski, V; Graczykowski, Lk; Grecka, E; Grelli, A; Grigoras, C; Grigoriev, V; Grigoryan, S; Grosa, F; Grosse-Oetringhaus, Jf; 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C, PARTICLES AND FIELDS. - ISSN 1434-6044. - 83:7(2023). [10.1140/epjc/s10052-023-11658-w]
Symmetry plane correlations in Pb-Pb collisions at √sNN=2.76 TeV
Acharya, S; Adamová, D; Adler, A; Rinella, GA; Agnello, M; Agrawal, N; Ahammed, Z; Ahmad, S; Ahn, SU; Ahuja, I; Akindinov, A; Al-Turany, M; Aleksandrov, D; Alessandro, B; Alfanda, HM; Molina, RA; Ali, B; Alici, A; Alizadehvandchali, N; Alkin, A; Alme, J; Alocco, G; Alt, T; Altsybeev, I; Anaam, MN; Andrei, C; Andronic, A; Anguelov, V; Antinori, F; Antonioli, P; Apadula, N; Aphecetche, L; Appelshaeuser, H; Arata, C; Arcelli, S; Aresti, M; Arnaldi, R; Arneiro, JGMCA; Arsene, IC; Arslandok, M; Augustinus, A; Averbeck, R; Azmi, MD; Badala, A; Bae, J; Baek, YW; Bai, X; Bailhache, R; Bailung, Y; Balbino, A; Baldisseri, A; Balis, B; Banerjee, D; Banoo, Z; Barbera, R; Barile, F; Barioglio, L; Barlou, M; Barnafoldi, GG; Barnby, LS; Barret, V; Barreto, L; Bartels, C; Barth, K; Bartsch, E; Bastid, N; Basu, S; Batigne, G; Battistini, D; Batyunya, B; Bauri, D; Alba, JLB; Bearden, IG; Beattie, C; Becht, P; Behera, D; Belikov, I; Hechavarria, ADCB; Bellini, F; Bellwied, R; Belokurova, S; Belyaev, V; Bencedi, G; Beole, S; Bercuci, A; Berdnikov, Y; Berdnikova, A; Bergmann, L; Besoiu, MG; Betev, L; Bhaduri, PP; Bhasin, A; Bhat, MA; Bhattacharjee, B; Bianchi, L; Bianchi, N; Bielcík, J; Bielcíková, J; Biernat, J; Bigot, AP; Bilandzic, A; Biro, G; Biswas, S; Bize, N; Blair, JT; Blau, D; Blidaru, MB; Bluhme, N; Blume, C; Boca, G; Bock, F; Bodova, T; Bogdanov, A; Boi, S; Bok, J; Boldizsár, L; Bolozdynya, A; Bombara, M; Bond, PM; Bonomi, G; Borel, H; Borissov, A; Carcamo, AGB; Bossi, H; Botta, E; Bouziani, YEM; Bratrud, L; Braun-Munzinger, P; Bregant, M; Broz, M; Bruno, GE ;Buckland, MD; Budnikov, D; Buesching, H; Bufalino, S; Bugnon, O; Buhler, P; Buthelezi, Z; Bysiak, SA; Cai, M; Caines, H; Caliva, A; Villar, EC; Camacho, JMM; Camerini, P; Canedo, FDM; Carabas, M; Carballo, AA; Carnesecchi, F; Caron, R; Carvalho, LAD; Castellanos, JC; Catalano, F; Sanchez, CC; Chakaberia, I; Chakraborty, P; Chandra, S; Chapeland, S; Chartier, M; Chattopadhyay, S; Chattopadhyay, S; Chavez, TG; Cheng, T; Cheshkov, C; Cheynis, B; Barroso, VC; Chinellato, DD; Chizzali, ES; Cho, J; Cho, S; Chochula, P; Christakoglou, P; Christensen, CH; Christiansen, P; Chujo, T; Ciacco, M; Cicalo, C; Cindolo, F; Ciupek, MR; Clai, G; Colamaria, F; Colburn, JS; Colella, D ;Colocci, M; Concas, M; Balbastre, GC; del Valle, ZC; Contin, G; Contreras, JG; Coquet, ML; Cormier, TM; Cortese, P; Cosentino, MR; Costa, F; Costanza, S; Cot, C; Crkovská, J; Crochet, P; Cruz-Torres, R; Cuautle, E; Cui, P; Dainese, A; Danisch, MC; Danu, A; Das, P; Das, P; Das, S; Dash, AR; Dash, S; De Caro, A; de Cataldo, G; de Cuveland, J; De Falco, A; De Gruttola, D; De Marco, N; De Martin, C; De Pasquale, S; Deb, S; Debski, RJ; Deja, KR; Del Grande, R; Dello Stritto, L; Deng, W; Dhankher, P; Di Bari, D; Di Mauro, A; Diaz, RA; Dietel, T; Ding, Y; Divia, R; Dixit, DU; Djuvsland, O; Dmitrieva, U; Dobrin, A; Doenigus, B; Dubinski, JM; Dubla, A; Dudi, S; Dupieux, P; Durkac, M; Dzalaiova, N; Eder, TM; Ehlers, RJ; Eikeland, VN; Eisenhut, F; Elia, D; Erazmus, B; 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2023-01-01
Abstract
A newly developed observable for correlations between symmetry planes, which characterize the direction of the anisotropic emission of produced particles, is measured in Pb-Pb collisions at root s(NN) = 2.76 TeV with ALICE. This so-called Gaussian Estimator allows for the first time the study of these quantities without the influence of correlations between different flow amplitudes. The centrality dependence of various correlations between two, three and four symmetry planes is presented. The ordering of magnitude between these symmetry plane correlations is discussed and the results of the Gaussian Estimator are compared with measurements of previously used estimators. The results utilizing the new estimator lead to significantly smaller correlations than reported by studies using the Scalar Product method. Furthermore, the obtained symmetry plane correlations are compared to state-of-the-art hydrodynamic model calculations for the evolution of heavy-ion collisions. While the model predictions provide a qualitative description of the data, quantitative agreement is not always observed, particularly for correlators with significant non-linear response of the medium to initial state anisotropies of the collision system. As these results provide unique and independent information, their usage in future Bayesian analysis can further constrain our knowledge on the properties of the QCDmatter produced in ultrarelativistic heavy-ion collisions.
Citazione
Symmetry plane correlations in Pb-Pb collisions at √sNN=2.76 TeV / Acharya, S; Adamová, D; Adler, A; Rinella, Ga; Agnello, M; Agrawal, N; Ahammed, Z; Ahmad, S; Ahn, Su; Ahuja, I; Akindinov, A; Al-Turany, M; Aleksandrov, D; Alessandro, B; Alfanda, Hm; Molina, Ra; Ali, B; Alici, A; Alizadehvandchali, N; Alkin, A; Alme, J; Alocco, G; Alt, T; Altsybeev, I; Anaam, Mn; Andrei, C; Andronic, A; Anguelov, V; Antinori, F; Antonioli, P; Apadula, N; Aphecetche, L; Appelshaeuser, H; Arata, C; Arcelli, S; Aresti, M; Arnaldi, R; Arneiro, Jgmca; Arsene, Ic; Arslandok, M; Augustinus, A; Averbeck, R; Azmi, Md; Badala, A; Bae, J; Baek, Yw; Bai, X; Bailhache, R; Bailung, Y; Balbino, A; Baldisseri, A; Balis, B; Banerjee, D; Banoo, Z; Barbera, R; Barile, F; Barioglio, L; Barlou, M; Barnafoldi, Gg; Barnby, Ls; Barret, V; Barreto, L; Bartels, C; Barth, K; Bartsch, E; Bastid, N; Basu, S; Batigne, G; Battistini, D; Batyunya, B; Bauri, D; Alba, Jlb; Bearden, Ig; Beattie, C; Becht, P; Behera, D; Belikov, I; Hechavarria, Adcb; 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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.