My interests were focused on the studies of phase transition in nuclear matter. My scientific activity was devoted the extraction of different temperatures, freezeout volume and flow velocity bys using different hydrodynamic models. In particular we use the blast wave model with botlzmann Gibbs statistics and Tsallis statisitics, Hagedorn thermal model, and Standard distribition. Later I was involved in the Quark-gluon plasma(QGP) because as we know that more than 99% of the normal matter we see every day exists in protons and neutrons (nucleons). Nucleons are further composed of quarks and gluons, whose interactions are well described by the Quantum Chromo Dynamics theory (QCD). Under normal conditions, quarks are confined inside the nucleons and can only be detectable on the scale smaller than 0.3 femtometer. At extremely high temperature and density, matter turns into the so called Quark-gluon plasma (QGP) phase where quarks become deconfined. This phase is believed to have existed during the first 10 microseconds after the universe was born in the Big Bang. The QGP can be created by heating matter above the temperature of 170 MeV. Experimentally, this is done by colliding two large nuclei (typically Gold or Lead) at very high energy. The resulting hot and dense fireball is expected to expand under its own pressure, and cool down. Recenlty i am also working on the production of light nuclei.
My interests were focused on the studies of phase transition in nuclear matter. My scientific activity was devoted the extraction of different temperatures, freezeout volume and flow velocity bys using different hydrodynamic models. In particular we use the blast wave model with botlzmann Gibbs statistics and Tsallis statisitics, Hagedorn thermal model, and Standard distribition. Later I was involved in the Quark-gluon plasma(QGP) because as we know that more than 99% of the normal matter we see every day exists in protons and neutrons (nucleons). Nucleons are further composed of quarks and gluons, whose interactions are well described by the Quantum Chromo Dynamics theory (QCD). Under normal conditions, quarks are confined inside the nucleons and can only be detectable on the scale smaller than 0.3 femtometer. At extremely high temperature and density, matter turns into the so called Quark-gluon plasma (QGP) phase where quarks become deconfined. This phase is believed to have existed during the first 10 microseconds after the universe was born in the Big Bang. The QGP can be created by heating matter above the temperature of 170 MeV. Experimentally, this is done by colliding two large nuclei (typically Gold or Lead) at very high energy. The resulting hot and dense fireball is expected to expand under its own pressure, and cool down. Recenlty i am also working on the production of light nuclei.