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15 papers · 2 filters
Higher-order symmetry energy of nuclear matter and the inner edge of neutron star crusts
W. M. Seif, D. N. Basu
The parabolic approximation to the equation of state of the isospin asymmetric nuclear matter (ANM) is widely used in the literature to make predictions for the nuclear structure a…
Cosmic Separation of Phases: the microsecond universe and the neutron star
Bikash Sinha
It is entirely plausible under reasonable condition, that a first order QCD phase transition occurred from quarks to hadrons when the universe was about a microsecond old. Relics,…
Effect of high frequency modes of medium on an open quantum system
Nirupam Dutta, A. K. Chaudhuri, P. K. Panigrahi
We present a method to calculate the real time effective propagator of a generic open quantum system, immersed in a medium using a wave function based framework. The medium is char…
Estimates for temperature in projectile like fragment in geometric and transport models
S. Mallik, S. Das Gupta, G. Chaudhuri
Projectile like fragments emerging from heavy ion collision have an excitation energy which is often labeled by a temperature. This temperature was recently calculated using a geom…
Effective interaction: From nuclear reactions to neutron stars
D. N. Basu
An equation of state (EoS) for symmetric nuclear matter is constructed using the density dependent M3Y effective interaction and extended for isospin asymmetric nuclear matter. The…
Charm Quark Energy Loss In Infinite QCD Matter Using A Parton Cascade Model
Mohammed Younus, Christopher E. Coleman-Smith, Steffen A. Bass +1
We utilize the Parton Cascade Model to study the evolution of charm quarks propagating through a thermal brick of QCD matter. We determine the energy loss and the transport coeffic…