Number of the records: 1  

Charged-pion production in Au plus Au collisions at root s(NN)=2.4 GeV

  1. 1.
    0534044 - ÚJF 2021 RIV US eng J - Journal Article
    Adamczewski-Musch, J. - Arnold, O. - Behnke, C. - Belounnas, A. - Chlad, Lukáš - Kugler, Andrej - Rodriguez Ramos, Pablo - Sobolev, Yuri, G. - Svoboda, Ondřej - Tlustý, Pavel - Wagner, Vladimír … Total 124 authors
    Charged-pion production in Au plus Au collisions at root s(NN)=2.4 GeV.
    European Physical Journal A. Roč. 56, č. 10 (2020), č. článku 259. ISSN 1434-6001. E-ISSN 1434-601X
    R&D Projects: GA MŠMT LTT17003; GA MŠMT EF16_013/0001677
    Research Infrastructure: FAIR-CZ II - 90112
    Institutional support: RVO:61389005
    Keywords : HADES collaboration * heavy ion collisions
    OECD category: Nuclear physics
    Impact factor: 3.043, year: 2020
    Method of publishing: Open access
    https://doi.org/10.1140/epja/s10050-020-00237-2

    We present high-statistic data on charged-pion emission from Au + Au collisions at root s(NN) = 2.4GeV = 2.4 GeV (corresponding to E-beam = 1.23A GeV) in four centrality classes in the range 0-40% of the most central collisions. The data are analyzed as a function of transverse momentum, transverse mass, rapidity, and polar angle. Pion multiplicity per participating nucleon decreases moderately with increasing centrality. The polar angular distributions are found to be non-isotropic even for the most central event class. Our results on pion multiplicity fit well into the general trend of the available world data, but undershoot by 2.5 sigma data from the FOPI experiment measured at slightly lower beam energy. We compare our data to state-of-the-art transport model calculations (PHSD, IQMD, PHQMD, GiBUU and SMASH) and find substantial differences between the measurement and the results of these calculations.
    Permanent Link: http://hdl.handle.net/11104/0312255

     
    FileDownloadSizeCommentaryVersionAccess
    0534044.pdf06.6 MBOpen Access - SCOAP3Publisher’s postprintopen-access
     
Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.