Specific heat of matter formed in relativistic nuclear collisions

Sumit Basu, Sandeep Chatterjee, Rupa Chatterjee, Tapan K. Nayak, and Basanta K. Nandi
Phys. Rev. C 94, 044901 – Published 3 October 2016

Abstract

We report the excitation energy dependence of specific heat (cv) of hadronic matter at freeze-out in Au+Au and Cu+Cu collisions at the BNL Relativistic Heavy Ion Collider energies by analyzing the published data on event-by-event mean transverse momentum (pT) distributions. The pT distributions in finite pT ranges are converted to distributions of effective temperatures, and dynamical fluctuations in temperature are extracted by subtracting widths of the corresponding mixed event distributions. The heat capacity per particle at the kinetic freeze-out surface is presented as a function of collision energy, which shows a sharp rise in cv below sNN=62.4 GeV. We employ the hadron resonance gas (HRG) model to estimate cv at the chemical and kinetic freeze-out surfaces. The experimental results are compared to the HRG and other theoretical model calculations. HRG results show good agreement with data. Model predictions for cv at the CERN Large Hadron Collider energy are presented.

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  • Received 21 January 2016

DOI:https://doi.org/10.1103/PhysRevC.94.044901

©2016 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Sumit Basu, Sandeep Chatterjee, Rupa Chatterjee, and Tapan K. Nayak

  • Variable Energy Cyclotron Centre, Kolkata 700064, India

Basanta K. Nandi

  • Indian Institute of Technology Bombay, Mumbai 400076, India

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Issue

Vol. 94, Iss. 4 — October 2016

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