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Production of protons and light nuclei in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>Au</mml:mi><mml:mo>+</mml:mo><mml:mi>Au</mml:mi></mml:math> collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msqrt><mml:msub><mml:mi>s</mml:mi><mml:mrow><mml:mi>N</mml:mi><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mspace width="0.16em"/><mml:mo>=</mml:mo><mml:mspace width="0.16em"/><mml:mn>3</mml:mn></mml:mrow></mml:math> GeV with the STAR detector

M. I. AbdulhamidAmerican University in CairoB. E. AboonaTexas A&M UniversityJ. AdamCzech Technical University in PragueLidia AdamczykAGH University of KrakowJ. R. AdamsThe Ohio State UniversityI. AggarwalPanjab UniversityM. M. AggarwalPanjab UniversityZ. AhammedVariable Energy Cyclotron CentreE. C. AschenauerBrookhaven National LaboratoryS. AslamIndian Institute TechnologyJ. AtchisonAbilene Christian UniversityV. BairathiJ. G. Ball CapUniversity of HoustonK. BarishUniversity of CaliforniaR. BellwiedUniversity of HoustonP. BhagatUniversity of JammuA. BhasinUniversity of JammuS. BhattaState University of New YorkS. R. BhosaleELTE Eötvös Loránd UniversityJ. BielcikCzech Technical University in PragueJ. BielčíkováNuclear Physics Institute of the CASJ. D. BrandenburgThe Ohio State UniversityC. BroodoUniversity of HoustonX. Z. CaiShanghai Institute of Applied PhysicsH. CainesYale UniversityM. Calderón de la Barca SánchezUniversity of CaliforniaD. CebraUniversity of CaliforniaJ. CeskaCzech Technical University in PragueI. ChakaberiaLawrence Berkeley National LaboratoryP. ChaloupkaCzech Technical University in PragueB. K. ChanUniversity of CaliforniaZ. ChangIndiana UniversityA. ChatterjeeNational Institute of Technology DurgapurD. ChenUniversity of CaliforniaJing ChenFudan UniversityJ. H. ChenFudan UniversityQinyu ChenGuangxi Normal UniversityZ. ChenShandong UniversityJ. ChengTsinghua UniversityY. ChengUniversity of CaliforniaW. ChristieBrookhaven National LaboratoryX. ChuBrookhaven National LaboratoryH. J. CrawfordUniversity of CaliforniaM. CsanádELTE Eötvös Loránd UniversityG. Dale-GauUniversity of Illinois at ChicagoArpan DasCzech Technical University in PragueI. M. DeppnerUniversity of HeidelbergA. DeshpandeState University of New YorkA. DhamijaPanjab UniversityP. DixitIndian Institute of Science Education and Research (IISER)Xiang-Kun DongLawrence Berkeley National LaboratoryJ. L. DrachenbergAbilene Christian UniversityE. DuckworthKent State UniversityJ. C. DunlopBrookhaven National LaboratoryJ. EngelageUniversity of CaliforniaG. EppleyRice UniversityS. EsumiUniversity of TsukubaO. EvdokimovUniversity of Illinois at ChicagoO. EyserBrookhaven National LaboratoryR. FatemiUniversity of KentuckyS. FazioUniversity of Calabria & INFN-CosenzaC. FengNational Cheng Kung UniversityYuliang FengPurdue UniversityE. FinchSouthern Connecticut State UniversityY. FisyakBrookhaven National LaboratoryF. FlorYale UniversityC. D. FuInstitute of Modern PhysicsC. A. GagliardiTexas A&M UniversityT. GalatyukTechnische Universität DarmstadtTong GaoShandong UniversityF. J. M. GeurtsRice UniversityN. GhimireTemple UniversityA. GibsonValparaiso UniversityK. GopalIndian Institute of Science Education and Research (IISER) TirupatiX. GouShandong UniversityD. GrosnickValparaiso UniversityA. GuptaUniversity of JammuW. GurynBrookhaven National LaboratoryA. HamedAmerican University in CairoYimo HanRice UniversityS. HarabaszTechnische Universität DarmstadtM. D. HarastyUniversity of CaliforniaJ. W. HarrisYale UniversityH. Harrison-SmithUniversity of KentuckyW. HeFudan UniversityX. H. HeInstitute of Modern PhysicsYang HeShandong UniversityN. HerrmannUniversity of HeidelbergL. HolubCzech Technical University in PragueCong HuUniversity of Chinese Academy of SciencesQingmao HuInstitute of Modern PhysicsY. HuLawrence Berkeley National LaboratoryH. Z. HuangNational Cheng Kung UniversityS. HuangState University of New YorkTao HuangUniversity of Illinois at ChicagoYidong HuangCentral China Normal UniversityT. J. HumanicThe Ohio State UniversityM. IsshikiUniversity of Tsukuba
Physical review. Cjournal2024lv
ABI

Аннотация

We report the systematic measurement of protons and light nuclei production in $\mathrm{Au}+\mathrm{Au}$ collisions at $\sqrt{{s}_{NN}}\phantom{\rule{0.16em}{0ex}}=\phantom{\rule{0.16em}{0ex}}3\phantom{\rule{0.16em}{0ex}}\mathrm{GeV}$ by the STAR experiment at the Relativistic Heavy Ion Collider (RHIC). The transverse momentum $({p}_{T})$ spectra of protons $(p)$, deuterons $(d)$, tritons $(t)$, $^{3}\mathrm{He}$, and $^{4}\mathrm{He}$ have been measured from midrapidity to target rapidity for different collision centralities. We present the rapidity and centrality dependence of particle yields $(dN/dy)$, average transverse momentum $(\ensuremath{\langle}{p}_{T}\ensuremath{\rangle})$, yield ratios $(d/p,$ $t/p,^{3}\mathrm{He}/p,$ $^{4}\mathrm{He}/p)$, as well as the coalescence parameters $({B}_{2},$ ${B}_{3})$. The $4\ensuremath{\pi}$ yields for various particles are determined by utilizing the measured rapidity distributions, $dN/dy$. Furthermore, we present the energy, centrality, and rapidity dependence of the compound yield ratios $({N}_{p}\ifmmode\times\else\texttimes\fi{}{N}_{t}/{N}_{d}^{2})$ and compare them with various model calculations. The physics implications of these results on the production mechanism of light nuclei and the QCD phase structure are discussed.

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