Cite
Skewness, kurtosis, and the fifth and sixth order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data
MLA
Sayantan Sharma, et al. “Skewness, Kurtosis, and the Fifth and Sixth Order Cumulants of Net Baryon-Number Distributions from Lattice QCD Confront High-Statistics STAR Data.” Physical Review D, vol. 101, Apr. 2020. EBSCOhost, widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsair&AN=edsair.doi.dedup.....06592b020362ab9ab9493082219d500f&authtype=sso&custid=ns315887.
APA
Sayantan Sharma, P. Enns, P. Steinbrecher, J. Goswami, Rasmus Larsen, Alexei Bazavov, Peter Petreczky, Frithjof Karsch, Heng-Tong Ding, D. Bollweg, Christian Schmidt, Swagata Mukherjee, Hiroshi Ohno, P. Hegde, & Olaf Kaczmarek. (2020). Skewness, kurtosis, and the fifth and sixth order cumulants of net baryon-number distributions from lattice QCD confront high-statistics STAR data. Physical Review D, 101.
Chicago
Sayantan Sharma, P. Enns, P. Steinbrecher, J. Goswami, Rasmus Larsen, Alexei Bazavov, Peter Petreczky, et al. 2020. “Skewness, Kurtosis, and the Fifth and Sixth Order Cumulants of Net Baryon-Number Distributions from Lattice QCD Confront High-Statistics STAR Data.” Physical Review D 101 (April). http://widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsair&AN=edsair.doi.dedup.....06592b020362ab9ab9493082219d500f&authtype=sso&custid=ns315887.