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The production of K*(892)(+/-) meson resonance is measured at midrapidity (|y| < 0.5) in Pb-Pb collisions at root s(NN) = 5.02 TeV using the ALICE detector at the CERN Large Hadron Collider. The resonance is reconstructed via its hadronic decay channel K *( 892)(+/-) -> K-S(0)pi(+/-). The transverse momentum distributions are obtained for various centrality intervals in the p(T) range of 0.4-16 GeV/c. Measurements of integrated yields, mean transverse momenta, and particle yield ratios are reported and found to be consistent with previous ALICE measurements for K *(892)(0) within uncertainties. The p(T)-integrated yield ratio 2 K*(892)(+/-)/(K+ + K-) in central Pb-Pb collisions shows a significant suppression at a level of 9.3 sigma relative to pp collisions. Thermal model calculations result in an overprediction of the particle yield ratio. Although both hadron resonance gas in partial chemical equilibrium (HRG-PCE) and MUSIC + SMASH simulations consider the hadronic phase, only HRG-PCE accurately represents the measurements, whereas MUSIC + SMASH simulations tend to overpredict the particle yield ratio. These observations, along with the kinetic freeze-out temperatures extracted from the yields measured for light-flavored hadrons using the HRG-PCE model, indicate a finite hadronic phase lifetime, which decreases with increasing collision centrality percentile. The p(T)-differential yield ratios 2 K*(892)(+/-)/(K+ + K-) and 2 K *(892)(+/-) /( pi(+) + pi(-)) are presented and compared with measurements in pp collisions at root s = 5.02 TeV. Both particle ratios are found to be suppressed by up to a factor of five at p(T) < 2.0 GeV/c in central Pb-Pb collisions and are qualitatively consistent with expectations for rescattering effects in the hadronic phase. The nuclear modification factor (R-AA) shows a smooth evolution with centrality and is found to be below unity at p(T) > 8 GeV/c, consistent with measurements for other light-flavored hadrons. The smallest values are observed in most central collisions, indicating larger energy loss of partons traversing the dense medium.
Acharya, S., Adamová, D., Aglieri Rinella, G., Agnello, M., Agrawal, N., Ahammed, Z., et al. (2024). K*(892)± resonance production in Pb-Pb collisions at sqrt(sNN)=5.02 TeV. PHYSICAL REVIEW C, 109(4), 1-18 [10.1103/physrevc.109.044902].
K*(892)± resonance production in Pb-Pb collisions at sqrt(sNN)=5.02 TeV
Acharya, S.;Adamová, D.;Aglieri Rinella, G.;Agnello, M.;Agrawal, N.;Ahammed, Z.;Ahmad, S.;Ahn, S. U.;Ahuja, I.;Akindinov, A.;Al-Turany, M.;Aleksandrov, D.;Alessandro, B.;Alfanda, H. M.;Alfaro Molina, R.;Ali, B.;Alici, A.;Alizadehvandchali, N.;Alkin, A.;Alme, J.;Alocco, G.;Alt, T.;Altamura, A. R.;Altsybeev, I.;Alvarado, J. R.;Anaam, M. N.;Andrei, C.;Andreou, N.;Andronic, A.;Anguelov, V.;Antinori, F.;Antonioli, P.;Apadula, N.;Aphecetche, L.;Appelshäuser, H.;Arata, C.;Arcelli, S.;Aresti, M.;Arnaldi, R.;Arneiro, J. G. M. C. A.;Arsene, I. C.;Arslandok, M.;Augustinus, A.;Averbeck, R.;Azmi, M. D.;Baba, H.;Badalà, A.;Bae, J.;Baek, Y. W.;Bai, X.;Bailhache, R.;Bailung, Y.;Balbino, A.;Baldisseri, A.;Balis, B.;Banerjee, D.;Banoo, Z.;Barbera, R.;Barile, F.;Barioglio, L.;Barlou, M.;Barman, B.;Barnaföldi, G. G.;Barnby, L. S.;Barret, V.;Barreto, L.;Bartels, C.;Barth, K.;Bartsch, E.;Bastid, N.;Basu, S.;Batigne, G.;Battistini, D.;Batyunya, B.;Bauri, D.;Bazo Alba, J. L.;Bearden, I. G.;Beattie, C.;Becht, P.;Behera, D.;Belikov, I.;Bell Hechavarria, A. D. C.;Bellini, F.;Bellwied, R.;Belokurova, S.;Beltran, Y. A. V.;Bencedi, G.;Beole, S.;Berdnikov, Y.;Berdnikova, A.;Bergmann, L.;Besoiu, M. G.;Betev, L.;Bhaduri, P. P.;Bhasin, A.;Bhat, M. A.;Bhattacharjee, B.;Bianchi, L.;Bianchi, N.;Bielčík, J.;Bielčíková, J.;Biernat, J.;Bigot, A. P.;Bilandzic, A.;Biro, G.;Biswas, S.;Bize, N.;Blair, J. T.;Blau, D.;Blidaru, M. B.;Bluhme, N.;Blume, C.;Boca, G.;Bock, F.;Bodova, T.;Bogdanov, A.;Boi, S.;Bok, J.;Boldizsár, L.;Bombara, M.;Bond, P. M.;Bonomi, G.;Borel, H.;Borissov, A.;Borquez Carcamo, A. G.;Bossi, H.;Botta, E.;Bouziani, Y. E. M.;Bratrud, L.;Braun-Munzinger, P.;Bregant, M.;Broz, M.;Bruno, G. E.;Buckland, M. D.;Budnikov, D.;Buesching, H.;Bufalino, S.;Buhler, P.;Burmasov, N.;Buthelezi, Z.;Bylinkin, A.;Bysiak, S. A.;Cai, M.;Caines, H.;Caliva, A.;Calvo Villar, E.;Camacho, J. M. M.;Camerini, P.;Canedo, F. D. M.;Cantway, S. L.;Carabas, M.;Carballo, A. A.;Carnesecchi, F.;Caron, R.;Carvalho, L. A. D.;Castillo Castellanos, J.;Catalano, F.;Ceballos Sanchez, C.;Chakaberia, I.;Chakraborty, P.;Chandra, S.;Chapeland, S.;Chartier, M.;Chattopadhyay, S.;Chattopadhyay, S.;Cheng, T.;Cheshkov, C.;Cheynis, B.;Chibante Barroso, V.;Chinellato, D. D.;Chizzali, E. S.;Cho, J.;Cho, S.;Chochula, P.;Choudhury, D.;Christakoglou, P.;Christensen, C. H.;Christiansen, P.;Chujo, T.;Ciacco, M.;Cicalo, C.;Cindolo, F.;Ciupek, M. R.;Clai, G.;Colamaria, F.;Colburn, J. S.;Colella, D.;Colocci, M.;Concas, M.;Conesa Balbastre, G.;Conesa del Valle, Z.;Contin, G.;Contreras, J. G.;Coquet, M. L.;Cortese, P.;Cosentino, M. R.;Costa, F.;Costanza, S.;Cot, C.;Crkovská, J.;Crochet, P.;Cruz-Torres, R.;Cui, P.;Dainese, A.;Danisch, M. C.;Danu, A.;Das, P.;Das, P.;Das, S.;Dash, A. 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L.;Mikhaylov, K.;Mishra, A. N.;Miśkowiec, D.;Modak, A.;Mohanty, B.;Mohisin Khan, M.;Molander, M. A.;Monira, S.;Mordasini, C.;Moreira De Godoy, D. A.;Morozov, I.;Morsch, A.;Mrnjavac, T.;Muccifora, V.;Muhuri, S.;Mulligan, J. D.;Mulliri, A.;Munhoz, M. G.;Munzer, R. H.;Murakami, H.;Murray, S.;Musa, L.;Musinsky, J.;Myrcha, J. W.;Naik, B.;Nambrath, A. I.;Nandi, B. K.;Nania, R.;Nappi, E.;Nassirpour, A. F.;Nath, A.;Nattrass, C.;Naydenov, M. N.;Neagu, A.;Negru, A.;Nellen, L.;Nepeivoda, R.;Nese, S.;Neskovic, G.;Nicassio, N.;Nielsen, B. S.;Nielsen, E. G.;Nikolaev, S.;Nikulin, S.;Nikulin, V.;Noferini, F.;Noh, S.;Nomokonov, P.;Norman, J.;Novitzky, N.;Nowakowski, P.;Nyanin, A.;Nystrand, J.;Ogino, M.;Oh, S.;Ohlson, A.;Okorokov, V. A.;Oleniacz, J.;Oliveira Da Silva, A. C.;Onnerstad, A.;Oppedisano, C.;Ortiz Velasquez, A.;Otwinowski, J.;Oya, M.;Oyama, K.;Pachmayer, Y.;Padhan, S.;Pagano, D.;Paić, G.;Paisano-Guzmán, S.;Palasciano, A.;Panebianco, S.;Park, H.;Park, H.;Park, J.;Parkkila, J. E.;Patley, Y.;Patra, R. N.;Paul, B.;Pei, H.;Peitzmann, T.;Peng, X.;Pennisi, M.;Perciballi, S.;Peresunko, D.;Perez, G. M.;Pestov, Y.;Petrov, V.;Petrovici, M.;Pezzi, R. P.;Piano, S.;Pikna, M.;Pillot, P.;Pinazza, O.;Pinsky, L.;Pinto, C.;Pisano, S.;Płoskoń, M.;Planinic, M.;Pliquett, F.;Poghosyan, M. G.;Polichtchouk, B.;Politano, S.;Poljak, N.;Pop, A.;Porteboeuf-Houssais, S.;Pozdniakov, V.;Pozos, I. Y.;Pradhan, K. K.;Prasad, S. K.;Prasad, S.;Preghenella, R.;Prino, F.;Pruneau, C. A.;Pshenichnov, I.;Puccio, M.;Pucillo, S.;Pugelova, Z.;Qiu, S.;Quaglia, L.;Ragoni, S.;Rai, A.;Rakotozafindrabe, A.;Ramello, L.;Rami, F.;Rancien, T. A.;Rasa, M.;Räsänen, S. S.;Rath, R.;Rauch, M. P.;Ravasenga, I.;Read, K. F.;Reckziegel, C.;Redelbach, A. R.;Redlich, K.;Reetz, C. A.;Regules-Medel, H. D.;Rehman, A.;Reidt, F.;Reme-Ness, H. A.;Rescakova, Z.;Reygers, K.;Riabov, A.;Riabov, V.;Ricci, R.;Richter, M.;Riedel, A. A.;Riegler, W.;Riffero, A. G.;Ristea, C.;Rodriguez, M. V.;Rodríguez Cahuantzi, M.;Rodríguez Ramírez, S. A.;Røed, K.;Rogalev, R.;Rogochaya, E.;Rogoschinski, T. S.;Rohr, D.;Röhrich, D.;Rojas, P. F.;Rojas Torres, S.;Rokita, P. S.;Romanenko, G.;Ronchetti, F.;Rosano, A.;Rosas, E. D.;Roslon, K.;Rossi, A.;Roy, A.;Roy, S.;Rubini, N.;Ruggiano, D.;Rui, R.;Russek, P. G.;Russo, R.;Rustamov, A.;Ryabinkin, E.;Ryabov, Y.;Rybicki, A.;Rytkonen, H.;Ryu, J.;Rzesa, W.;Saarimaki, O. A. M.;Sadhu, S.;Sadovsky, S.;Saetre, J.;Šafařík, K.;Saha, P.;Saha, S. K.;Saha, S.;Sahoo, B.;Sahoo, B.;Sahoo, R.;Sahoo, S.;Sahu, D.;Sahu, P. K.;Saini, J.;Sajdakova, K.;Sakai, S.;Salvan, M. P.;Sambyal, S.;Samitz, D.;Sanna, I.;Saramela, T. B.;Sarma, P.;Sarritzu, V.;Sarti, V. M.;Sas, M. H. P.;Sawan, S.;Schambach, J.;Scheid, H. S.;Schiaua, C.;Schicker, R.;Schmah, A.;Schmidt, C.;Schmidt, H. R.;Schmidt, M. O.;Schmidt, M.;Schmidt, N. V.;Schmier, A. R.;Schotter, R.;Schröter, A.;Schukraft, J.;Schweda, K.;Scioli, G.;Scomparin, E.;Seger, J. E.;Sekiguchi, Y.;Sekihata, D.;Selina, M.;Selyuzhenkov, I.;Senyukov, S.;Seo, J. J.;Serebryakov, D.;Šerkšnytė, L.;Sevcenco, A.;Shaba, T. J.;Shabetai, A.;Shahoyan, R.;Shangaraev, A.;Sharma, A.;Sharma, B.;Sharma, D.;Sharma, H.;Sharma, M.;Sharma, S.;Sharma, S.;Sharma, U.;Shatat, A.;Sheibani, O.;Shigaki, K.;Shimomura, M.;Shin, J.;Shirinkin, S.;Shou, Q.;Sibiriak, Y.;Siddhanta, S.;Siemiarczuk, T.;Silva, T. F.;Silvermyr, D.;Simantathammakul, T.;Simeonov, R.;Singh, B.;Singh, B.;Singh, K.;Singh, R.;Singh, R.;Singh, R.;Singh, S.;Singh, V. K.;Singhal, V.;Sinha, T.;Sitar, B.;Sitta, M.;Skaali, T. B.;Skorodumovs, G.;Slupecki, M.;Smirnov, N.;Snellings, R. J. M.;Solheim, E. H.;Song, J.;Sonnabend, C.;Soramel, F.;Soto-hernandez, A. B.;Spijkers, R.;Sputowska, I.;Staa, J.;Stachel, J.;Stan, I.;Steffanic, P. J.;Stiefelmaier, S. F.;Stocco, D.;Storehaug, I.;Stratmann, P.;Strazzi, S.;Sturniolo, A.;Stylianidis, C. P.;Suaide, A. A. 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H.;Yu, H.;Yuan, S.;Yuncu, A.;Zaccolo, V.;Zampolli, C.;Zanone, F.;Zardoshti, N.;Zarochentsev, A.;Závada, P.;Zaviyalov, N.;Zhalov, M.;Zhang, B.;Zhang, C.;Zhang, L.;Zhang, S.;Zhang, X.;Zhang, Y.;Zhang, Z.;Zhao, M.;Zherebchevskii, V.;Zhi, Y.;Zhou, D.;Zhou, Y.;Zhu, J.;Zhu, Y.;Zugravel, S. C.;Zurlo, N.;null, null
2024
Abstract
The production of K*(892)(+/-) meson resonance is measured at midrapidity (|y| < 0.5) in Pb-Pb collisions at root s(NN) = 5.02 TeV using the ALICE detector at the CERN Large Hadron Collider. The resonance is reconstructed via its hadronic decay channel K *( 892)(+/-) -> K-S(0)pi(+/-). The transverse momentum distributions are obtained for various centrality intervals in the p(T) range of 0.4-16 GeV/c. Measurements of integrated yields, mean transverse momenta, and particle yield ratios are reported and found to be consistent with previous ALICE measurements for K *(892)(0) within uncertainties. The p(T)-integrated yield ratio 2 K*(892)(+/-)/(K+ + K-) in central Pb-Pb collisions shows a significant suppression at a level of 9.3 sigma relative to pp collisions. Thermal model calculations result in an overprediction of the particle yield ratio. Although both hadron resonance gas in partial chemical equilibrium (HRG-PCE) and MUSIC + SMASH simulations consider the hadronic phase, only HRG-PCE accurately represents the measurements, whereas MUSIC + SMASH simulations tend to overpredict the particle yield ratio. These observations, along with the kinetic freeze-out temperatures extracted from the yields measured for light-flavored hadrons using the HRG-PCE model, indicate a finite hadronic phase lifetime, which decreases with increasing collision centrality percentile. The p(T)-differential yield ratios 2 K*(892)(+/-)/(K+ + K-) and 2 K *(892)(+/-) /( pi(+) + pi(-)) are presented and compared with measurements in pp collisions at root s = 5.02 TeV. Both particle ratios are found to be suppressed by up to a factor of five at p(T) < 2.0 GeV/c in central Pb-Pb collisions and are qualitatively consistent with expectations for rescattering effects in the hadronic phase. The nuclear modification factor (R-AA) shows a smooth evolution with centrality and is found to be below unity at p(T) > 8 GeV/c, consistent with measurements for other light-flavored hadrons. The smallest values are observed in most central collisions, indicating larger energy loss of partons traversing the dense medium.
Acharya, S., Adamová, D., Aglieri Rinella, G., Agnello, M., Agrawal, N., Ahammed, Z., et al. (2024). K*(892)± resonance production in Pb-Pb collisions at sqrt(sNN)=5.02 TeV. PHYSICAL REVIEW C, 109(4), 1-18 [10.1103/physrevc.109.044902].
Acharya, S.; Adamová, D.; Aglieri Rinella, G.; Agnello, M.; Agrawal, N.; Ahammed, Z.; Ahmad, S.; Ahn, S. U.; Ahuja, I.; Akindinov, A.; Al-Turany, M.; ...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/995410
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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.
