Matches in SemOpenAlex for { <https://semopenalex.org/work/W2025493385> ?p ?o ?g. }
- W2025493385 abstract "It is crucially important to find an acceptance and late collision process independent observable in searching for the possible critical point predicted by QCD. By utilizing a multiphase transport (AMPT) model and ultrarelativistic quantum molecular dynamics (UrQMD) model, we study the centrality and evolution time dependence of higher moments of net baryon distribution in $mathrm{Au}+mathrm{Au}$ collisions at $sqrt{{s}_{mathit{NN}}}=17.3$ GeV. The results suggest that kurtosis and skewness are less sensitive to the acceptance effect and late collision process. Thus, they should be good observables providing the information on the early stage of a heavy-ion collision. In addition, our study shows that the product of kurtosis times ${ensuremath{sigma}}^{2}$ of the net proton distribution is quite different from that of the net baryon distribution when the collision energy is lower than $sqrt{{s}_{mathit{NN}}}=20$ GeV, the Monte Carlo calculations on kurtosis$ifmmodecdotelsetextperiodcenteredfi{}{ensuremath{sigma}}^{2}$ have a deviation from the theoretical predictions." @default.
- W2025493385 created "2016-06-24" @default.
- W2025493385 creator A5007751532 @default.
- W2025493385 creator A5026150311 @default.
- W2025493385 creator A5048652481 @default.
- W2025493385 creator A5075754921 @default.
- W2025493385 creator A5080424148 @default.
- W2025493385 date "2010-07-21" @default.
- W2025493385 modified "2023-09-26" @default.
- W2025493385 title "Higher moments of net baryon distribution as probes of the QCD critical point" @default.
- W2025493385 cites W1541448464 @default.
- W2025493385 cites W1964512472 @default.
- W2025493385 cites W1965193220 @default.
- W2025493385 cites W1972940382 @default.
- W2025493385 cites W1975834858 @default.
- W2025493385 cites W1979605646 @default.
- W2025493385 cites W1986245600 @default.
- W2025493385 cites W1990594795 @default.
- W2025493385 cites W1995919116 @default.
- W2025493385 cites W2004840381 @default.
- W2025493385 cites W2006444959 @default.
- W2025493385 cites W2012573093 @default.
- W2025493385 cites W2041281433 @default.
- W2025493385 cites W2044775944 @default.
- W2025493385 cites W2049143866 @default.
- W2025493385 cites W2057967594 @default.
- W2025493385 cites W2058538085 @default.
- W2025493385 cites W2064412362 @default.
- W2025493385 cites W2065030493 @default.
- W2025493385 cites W2067678014 @default.
- W2025493385 cites W2068634700 @default.
- W2025493385 cites W2068680257 @default.
- W2025493385 cites W2076205064 @default.
- W2025493385 cites W2080740823 @default.
- W2025493385 cites W2086930451 @default.
- W2025493385 cites W2092017103 @default.
- W2025493385 cites W2092822046 @default.
- W2025493385 cites W2097249011 @default.
- W2025493385 cites W2098003815 @default.
- W2025493385 cites W2099773209 @default.
- W2025493385 cites W2101512932 @default.
- W2025493385 cites W2103189471 @default.
- W2025493385 cites W2106233117 @default.
- W2025493385 cites W2109441268 @default.
- W2025493385 cites W2112764601 @default.
- W2025493385 cites W2118937159 @default.
- W2025493385 cites W2118989459 @default.
- W2025493385 cites W2154066223 @default.
- W2025493385 cites W2164244194 @default.
- W2025493385 cites W2174024475 @default.
- W2025493385 cites W2601668516 @default.
- W2025493385 cites W3102749173 @default.
- W2025493385 cites W3105273110 @default.
- W2025493385 doi "https://doi.org/10.1103/physrevc.82.014905" @default.
- W2025493385 hasPublicationYear "2010" @default.
- W2025493385 type Work @default.
- W2025493385 sameAs 2025493385 @default.
- W2025493385 citedByCount "14" @default.
- W2025493385 countsByYear W20254933852012 @default.
- W2025493385 countsByYear W20254933852013 @default.
- W2025493385 countsByYear W20254933852014 @default.
- W2025493385 countsByYear W20254933852015 @default.
- W2025493385 countsByYear W20254933852016 @default.
- W2025493385 countsByYear W20254933852018 @default.
- W2025493385 crossrefType "journal-article" @default.
- W2025493385 hasAuthorship W2025493385A5007751532 @default.
- W2025493385 hasAuthorship W2025493385A5026150311 @default.
- W2025493385 hasAuthorship W2025493385A5048652481 @default.
- W2025493385 hasAuthorship W2025493385A5075754921 @default.
- W2025493385 hasAuthorship W2025493385A5080424148 @default.
- W2025493385 hasBestOaLocation W20254933852 @default.
- W2025493385 hasConcept C105795698 @default.
- W2025493385 hasConcept C109214941 @default.
- W2025493385 hasConcept C110121322 @default.
- W2025493385 hasConcept C117137515 @default.
- W2025493385 hasConcept C121332964 @default.
- W2025493385 hasConcept C121704057 @default.
- W2025493385 hasConcept C122342681 @default.
- W2025493385 hasConcept C134306372 @default.
- W2025493385 hasConcept C154153549 @default.
- W2025493385 hasConcept C166963901 @default.
- W2025493385 hasConcept C185544564 @default.
- W2025493385 hasConcept C196298200 @default.
- W2025493385 hasConcept C2778049214 @default.
- W2025493385 hasConcept C32848918 @default.
- W2025493385 hasConcept C33923547 @default.
- W2025493385 hasConcept C38652104 @default.
- W2025493385 hasConcept C41008148 @default.
- W2025493385 hasConcept C62520636 @default.
- W2025493385 hasConceptScore W2025493385C105795698 @default.
- W2025493385 hasConceptScore W2025493385C109214941 @default.
- W2025493385 hasConceptScore W2025493385C110121322 @default.
- W2025493385 hasConceptScore W2025493385C117137515 @default.
- W2025493385 hasConceptScore W2025493385C121332964 @default.
- W2025493385 hasConceptScore W2025493385C121704057 @default.
- W2025493385 hasConceptScore W2025493385C122342681 @default.
- W2025493385 hasConceptScore W2025493385C134306372 @default.
- W2025493385 hasConceptScore W2025493385C154153549 @default.
- W2025493385 hasConceptScore W2025493385C166963901 @default.
- W2025493385 hasConceptScore W2025493385C185544564 @default.