pith. machine review for the scientific record. sign in

arxiv: 1506.07605 · v1 · pith:PO3VROEInew · submitted 2015-06-25 · ⚛️ nucl-ex

Probing Parton Dynamics of QCD Matter with Ω and φ Production

STAR Collaboration: L. Adamczyk , J. K. Adkins , G. Agakishiev , M. M. Aggarwal , Z. Ahammed , I. Alekseev , J. Alford , A. Aparin
show 320 more authors
D. Arkhipkin E. C. Aschenauer G. S. Averichev V. Bairathi A. Banerjee R. Bellwied A. Bhasin A. K. Bhati P. Bhattarai J. Bielcik J. Bielcikova L. C. Bland I. G. Bordyuzhin J. Bouchet A. V. Brandin I. Bunzarov J. Butterworth H. Caines M. Calder\'on de la Barca S\'anchez J. M. Campbell D. Cebra M. C. Cervantes I. Chakaberia P. Chaloupka Z. Chang S. Chattopadhyay J. H. Chen X. Chen J. Cheng M. Cherney W. Christie G. Contin H. J. Crawford S. Das L. C. De Silva R. R. Debbe T. G. Dedovich J. Deng A. A. Derevschikov B. Di Ruzza L. Didenko C. Dilks X. Dong J. L. Drachenberg J. E. Draper C. M. Du L. E. Dunkelberger J. C. Dunlop L. G. Efimov J. Engelage G. Eppley R. Esha O. Evdokimov O. Eyser R. Fatemi S. Fazio P. Federic J. Fedorisin Z. Feng P. Filip Y. Fisyak C. E. Flores L. Fulek C. A. Gagliardi D. Garand F. Geurts A. Gibson M. Girard L. Greiner D. Grosnick D. S. Gunarathne Y. Guo A. Gupta S. Gupta W. Guryn A. Hamad A. Hamed R. Haque J. W. Harris L. He S. Heppelmann A. Hirsch G. W. Hoffmann D. J. Hofman S. Horvat B. Huang H. Z. Huang X. Huang P. Huck T. J. Humanic G. Igo W. W. Jacobs H. Jang K. Jiang E. G. Judd S. Kabana D. Kalinkin K. Kang K. Kauder H. W. Ke D. Keane A. Kechechyan Z. H. Khan D. P. Kiko{\l}a I. Kisel A. Kisiel L. Kochenda D. D. Koetke T. Kollegger L. K. Kosarzewski A. F. Kraishan P. Kravtsov K. Krueger I. Kulakov L. Kumar R. A. Kycia M. A. C. Lamont J. M. Landgraf K. D. Landry J. Lauret A. Lebedev R. Lednicky J. H. Lee X. Li Z. M. Li Y. Li W. Li C. Li M. A. Lisa F. Liu T. Ljubicic W. J. Llope M. Lomnitz R. S. Longacre X. Luo G. L. Ma R. Ma Y. G. Ma L. Ma N. Magdy R. Majka A. Manion S. Margetis C. Markert H. Masui H. S. Matis D. McDonald K. Meehan N. G. Minaev S. Mioduszewski D. Mishra B. Mohanty M. M. Mondal D. A. Morozov M. K. Mustafa B. K. Nandi Md. Nasim T. K. Nayak G. Nigmatkulov L. V. Nogach S. Y. Noh J. Novak S. B. Nurushev G. Odyniec A. Ogawa K. Oh V. Okorokov D. Olvitt Jr. B. S. Page R. Pak Y. X. Pan Y. Pandit Y. Panebratsev B. Pawlik H. Pei C. Perkins A. Peterson P. Pile M. Planinic J. Pluta N. Poljak K. Poniatowska J. Porter M. Posik A. M. Poskanzer J. Putschke H. Qiu A. Quintero S. Ramachandran R. Raniwala S. Raniwala R. L. Ray H. G. Ritter J. B. Roberts O. V. Rogachevskiy J. L. Romero A. Roy L. Ruan J. Rusnak O. Rusnakova N. R. Sahoo P. K. Sahu I. Sakrejda S. Salur J. Sandweiss A. Sarkar J. Schambach R. P. Scharenberg A. M. Schmah W. B. Schmidke N. Schmitz J. Seger P. Seyboth N. Shah E. Shahaliev P. V. Shanmuganathan M. Shao M. K. Sharma B. Sharma W. Q. Shen S. S. Shi Q. Y. Shou E. P. Sichtermann R. Sikora M. Simko M. J. Skoby N. Smirnov D. Smirnov L. Song P. Sorensen H. M. Spinka B. Srivastava T. D. S. Stanislaus M. Stepanov R. Stock M. Strikhanov B. Stringfellow M. Sumbera B. Summa Z. Sun X. M. Sun Y. Sun X. Sun B. Surrow N. Svirida M. A. Szelezniak Z. Tang A. H. Tang T. Tarnowsky A. Tawfik J. H. Thomas A. R. Timmins D. Tlusty M. Tokarev S. Trentalange R. E. Tribble P. Tribedy S. K. Tripathy B. A. Trzeciak O. D. Tsai T. Ullrich D. G. Underwood I. Upsal G. Van Buren G. van Nieuwenhuizen M. Vandenbroucke R. Varma A. N. Vasiliev R. Vertesi F. Videb{\ae}k Y. P. Viyogi S. Vokal S. A. Voloshin A. Vossen G. Wang H. Wang J. S. Wang Y. Wang F. Wang J. C. Webb G. Webb L. Wen G. D. Westfall H. Wieman S. W. Wissink R. Witt Y. F. Wu Z. G. Xiao W. Xie K. Xin Y. F. Xu Q. H. Xu H. Xu N. Xu Z. Xu Y. Yang C. Yang S. Yang Q. Yang Z. Ye P. Yepes L. Yi K. Yip I. -K. Yoo N. Yu H. Zbroszczyk W. Zha J. B. Zhang Z. Zhang J. Zhang S. Zhang X. P. Zhang Y. Zhang F. Zhao J. Zhao C. Zhong L. Zhou X. Zhu Y. Zoulkarneeva M. Zyzak
This is my paper
classification ⚛️ nucl-ex
keywords collisionsomegastrangecentralenergiesquarkratiosproduction
0
0 comments X
read the original abstract

We present measurements of $\Omega$ and $\phi$ production at mid-rapidity from Au+Au collisions at nucleon-nucleon center-of-mass energies $\sqrt{s_{NN}}$ = 7.7, 11.5, 19.6, 27 and 39 GeV by the STAR experiment at the Relativistic Heavy Ion Collider (RHIC). Motivated by the coalescence formation mechanism for these strange hadrons, we study the ratios of $N(\Omega^{-}+\Omega^{+})/(2N(\phi))$. These ratios as a function of transverse momentum ($p_T$) fall on a consistent trend at high collision energies, but start to show deviations in peripheral collisions at $\sqrt{s_{NN}}$ = 19.6, 27 and 39 GeV, and in central collisions at 11.5 GeV in the intermediate $p_T$ region of 2.4-3.6 GeV/c. We further evaluate empirically the strange quark $p_T$ distributions at hadronization by studying the $\Omega/\phi$ ratios scaled by the number of constituent quarks. The NCQ-scaled $\Omega/\phi$ ratios show a suppression of strange quark production in central collisions at 11.5 GeV compared to $\sqrt{s_{NN}} >= 19.6$ GeV. The shapes of the presumably thermal strange quark distributions in 0-60% most central collisions at 7.7 GeV show significant deviations from those in 0-10% most central collisions at higher energies. These features suggest that there is likely a change of the underlying strange quark dynamics in the transition from quark-matter to hadronic matter at collision energies below 19.6 GeV.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Probing Late-Stage Hadronic Interactions at High Baryon Density via $K^{*0}$ Production in the RHIC Beam Energy Scan Program

    nucl-ex 2026-01 accept novelty 7.0

    K*0/K yield ratios in central Au+Au collisions at BES energies are suppressed relative to peripheral collisions and thermal predictions, indicating hadronic rescattering that strengthens at lower energies.