How to Measure Specific Heat Using Event-by-Event Average Fluctuations
arXiv:nucl-ex/0512004
Abstract
A simple way to visualize event-by-event average fluctuations is by assuming that each collision has a different temperature parameter (inverse slope) and that the ensemble of events has a temperature distribution about the mean, , with standard deviation . PHENIX characterizes the non-random fluctuation of , the event-by-event average , by , the fractional difference of the standard deviation of the data from that of a random sample obtained with mixed events. This can be related to the temperature fluctuation: \[ F_{p_T}=σ^{\rm data}_{M_{p_T}}/σ^{\rm random}_{M_{p_T}}-1\simeq(< n > -1) σ^2_{T}/< T>^2 \] Combining this with the Gavai, {\it et al.},\cite{Gavai05} and Korus, {\it et al.},\cite{Korus} definitions of the specific heat per particle, a simple relationship is obtained: \[ c_v/T^3={\mean{n}\over \mean{N_{tot}}} {1\over F_{p_T}} \] is measured with a fraction $\mean{n}/\mean{N_{tot}}$ of the total particles produced, a purely geometrical factor representing the fractional acceptance, in PHENIX. Gavai, {\it et al.} predict that , which corresponds to % in PHENIX, which may be accessible by measurements of in the range GeV/c. In order to test the Gavai, {\it et al.} prediction that is reduced in a QGP compared to the ideal gas value (15 compared to 21), precision measurements of in the range 0.20% for GeV/c may be practical.
8 pages, 5 figures. To appear in the Quark Matter 2005 Poster Proceedings in Nukleonika