Skewness, kurtosis and the 5th and 6th order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data
Bazavov A, Bollweg D, Ding H-T, Enns P, Goswami J, Hegde P, Kaczmarek O, Karsch F, Larsen R, Mukherjee S, Ohno H, et al. (2020)
arXiv:2001.08530.
Preprint | Englisch
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Autor*in
Bazavov, A.;
Bollweg, DennisUniBi;
Ding, H. -T.;
Enns, P.;
Goswami, JishnuUniBi ;
Hegde, P.;
Kaczmarek, OlafUniBi ;
Karsch, FrithjofUniBi;
Larsen, R.;
Mukherjee, Swagato;
Ohno, H.;
Petreczky, P.
Alle
Alle
Abstract / Bemerkung
We present new results on up to $6^{th}$ order cumulants of net baryon-number
fluctuations at small values of the baryon chemical potential, $\mu_B$,
obtained in lattice QCD calculations with physical values of light and strange
quark masses. Representation of the Taylor expansions of higher order cumulants
in terms of the ratio of the two lowest order cumulants,
$M_B/\sigma_B^2=\chi_1^B(T,\mu_B)/\chi_2^B(T,\mu_B)$, allows for a parameter
free comparison with data on net proton-number cumulants obtained by the STAR
Collaboration in the Beam Energy Scan at RHIC. We show that recent high
statistics data on skewness and kurtosis ratios of net proton-number
distributions, obtained at beam energy $\sqrt{s_{_{NN}}}=54.4$ GeV, agree well
with lattice QCD results on cumulants of net baryon-number fluctuations close
to the pseudo-critical temperature, $T_{pc}(\mu_B)$, for the chiral transition
in QCD. We also present first results from a next-to-leading order expansion of
$5^{th}$ and $6^{th}$ order cumulants on the line of pseudo-critical
temperatures.
Erscheinungsjahr
2020
Zeitschriftentitel
arXiv:2001.08530
Page URI
https://pub.uni-bielefeld.de/record/2941822
Zitieren
Bazavov A, Bollweg D, Ding H-T, et al. Skewness, kurtosis and the 5th and 6th order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data. arXiv:2001.08530. 2020.
Bazavov, A., Bollweg, D., Ding, H. - T., Enns, P., Goswami, J., Hegde, P., Kaczmarek, O., et al. (2020). Skewness, kurtosis and the 5th and 6th order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data. arXiv:2001.08530
Bazavov, A., Bollweg, Dennis, Ding, H. -T., Enns, P., Goswami, Jishnu, Hegde, P., Kaczmarek, Olaf, et al. 2020. “Skewness, kurtosis and the 5th and 6th order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data”. arXiv:2001.08530.
Bazavov, A., Bollweg, D., Ding, H. - T., Enns, P., Goswami, J., Hegde, P., Kaczmarek, O., Karsch, F., Larsen, R., Mukherjee, S., et al. (2020). Skewness, kurtosis and the 5th and 6th order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data. arXiv:2001.08530.
Bazavov, A., et al., 2020. Skewness, kurtosis and the 5th and 6th order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data. arXiv:2001.08530.
A. Bazavov, et al., “Skewness, kurtosis and the 5th and 6th order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data”, arXiv:2001.08530, 2020.
Bazavov, A., Bollweg, D., Ding, H.-T., Enns, P., Goswami, J., Hegde, P., Kaczmarek, O., Karsch, F., Larsen, R., Mukherjee, S., Ohno, H., Petreczky, P., Schmidt, C., Sharma, S., Steinbrecher, P.: Skewness, kurtosis and the 5th and 6th order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data. arXiv:2001.08530. (2020).
Bazavov, A., Bollweg, Dennis, Ding, H. -T., Enns, P., Goswami, Jishnu, Hegde, P., Kaczmarek, Olaf, Karsch, Frithjof, Larsen, R., Mukherjee, Swagato, Ohno, H., Petreczky, P., Schmidt, Christian, Sharma, S., and Steinbrecher, P. “Skewness, kurtosis and the 5th and 6th order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data”. arXiv:2001.08530 (2020).