prikaz prve stranice dokumenta K*0 production in Cu + Cu and Au + Au collisions at √sNN√=62.4 GeV and 200 GeV
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K*0 production in Cu + Cu and Au + Au collisions at √sNN√=62.4 GeV and 200 GeV
Physical Review C - Nuclear Physics, 84 (2011), 3; 034909. https://doi.org/10.1103/PhysRevC.84.034909
(STAR Collaboration) Aggarwal, M. M.; ...; Planinić, Mirko; ...; Poljak, Nikola; ...; Zoulkarneeva, Y.

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Aggarwal, M. M., Planinić, M., Poljak, N. i Zoulkarneeva, Y. (2011). K*0 production in Cu + Cu and Au + Au collisions at √sNN√=62.4 GeV and 200 GeV. Physical Review C - Nuclear Physics, 84. (3). doi: 10.1103/PhysRevC.84.034909

Aggarwal, M. M., et al. "K*0 production in Cu + Cu and Au + Au collisions at √sNN√=62.4 GeV and 200 GeV." Physical Review C - Nuclear Physics, vol. 84, br. 3, 2011. https://doi.org/10.1103/PhysRevC.84.034909

Aggarwal, M. M., Mirko Planinić, Nikola Poljak i Y. Zoulkarneeva. "K*0 production in Cu + Cu and Au + Au collisions at √sNN√=62.4 GeV and 200 GeV." Physical Review C - Nuclear Physics 84, br. 3 (2011). https://doi.org/10.1103/PhysRevC.84.034909

Aggarwal, M. M., et al. (2011) 'K*0 production in Cu + Cu and Au + Au collisions at √sNN√=62.4 GeV and 200 GeV', Physical Review C - Nuclear Physics, 84(3). doi: 10.1103/PhysRevC.84.034909

Aggarwal MM, Planinić M, Poljak N, Zoulkarneeva Y. K*0 production in Cu + Cu and Au + Au collisions at √sNN√=62.4 GeV and 200 GeV. Physical Review C - Nuclear Physics [Internet]. 2011. [pristupljeno 19.04.2024.];84(3). doi: 10.1103/PhysRevC.84.034909

M. M. Aggarwal, M. Planinić, N. Poljak i Y. Zoulkarneeva, "K*0 production in Cu + Cu and Au + Au collisions at √sNN√=62.4 GeV and 200 GeV", Physical Review C - Nuclear Physics, vol. 84, br. 3, 2011. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:306211. [Citirano: 19.04.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:306211
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Naslov (engleski)K*0 production in Cu + Cu and Au + Au collisions at √sNN√=62.4 GeV and 200 GeV
AutorM. M. Aggarwal
Autor
...
AutorMirko Planinić
Autor
...
AutorNikola Poljak
Autor
...
AutorY. Zoulkarneeva
KolaboracijaSTAR Collaboration
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
We report on K*0 production at midrapidity in Au + Au and Cu + Cu collisions at √sNN=62.4 and 200 GeV collected by the Solenoid Tracker at the Relativistic Heavy Ion Collider detector. The K*0 is reconstructed via the hadronic decays K*0→K+π− and K*0̅ →K−π+. Transverse momentum, pT, spectra are measured over a range of pT extending from 0.2 GeV/c up to 5 GeV/c. The center-of-mass energy and system size dependence of the rapidity density, dN/dy, and the average transverse momentum, 〈pT〉, are presented. The measured N(K*0)/N(K) and N(φ)/N(K*0) ratios favor the dominance of rescattering of decay daughters of K*0 over the hadronic regeneration for the K*0 production. In the intermediate pT region (2.0 <pT<4.0 GeV/c), the elliptic flow parameter, v2, and the nuclear modification factor, RCP, agree with the expectations from the quark coalescence model of particle production.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaPhysical Review C - Nuclear Physics
Brojčani podacivol. 84, br. 3, 034909
p-ISSN0556-2813
e-ISSN1089-490X
DOIhttps://doi.org/10.1103/PhysRevC.84.034909
URN:NBNurn:nbn:hr:217:306211
Datum objave publikacije2011
ProjektŠifra: 119-0982887-1006
Naziv (hrvatski): Istraživanje hadronskih sustava upotrebom relativističkih projektila
Voditelj: Mirko Planinić
Pravna nadležnost: Hrvatska
Financijer: MZOS
Linija financiranja: ZP
URL dokumentahttp://link.aps.org/doi/10.1103/PhysRevC.84.034909
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomenaCopyright (2011) by the American Physical Society. Received 11 June 2010; revised manuscript received 13 January 2011; published 20 September 2011.
Datum i vrijeme pohrane2019-11-15 16:04:21