403 research outputs found
Jet Transport Coefficient at the Large Hadron Collider Energies in a Color String Percolation Approach
Within the color string percolation model (CSPM), jet transport coefficient,
, is calculated for various multiplicity classes in proton-proton and
for centrality classes in nucleus-nucleus collisions at the Large Hadron
Collider energies for a better understanding of the matter formed in
ultra-relativistic collisions. is studied as a function of final
state charged particle multiplicity, initial state percolation temperature and
energy density. The CSPM results are then compared with different theoretical
calculations from the JET collaboration those incorporate particle energy loss
in the medium. A good agreement is found between CSPM results and the JET
collaboration calculations.Comment: 8 pages and 7 figures, Submitted for publicatio
Diffusion and fluctuations of open charmed hadrons in an interacting hadronic medium
Heavy quarks are excellent probes to understand the hot and dense medium
formed in ultra-relativistic collisions. In a hadronic medium, studying the
transport properties, e.g. the drag (), momentum diffusion (),
and spatial diffusion () coefficients of open charmed hadrons can
provide useful information about the medium. Moreover, the fluctuations of
charmed hadrons can help us to locate the onset of their deconfinement. In this
work, we incorporate attractive and repulsive interactions in the
well-established van der Waals hadron resonance gas model (VDWHRG) and study
the diffusion and fluctuations of charmed hadrons. This study helps us
understand the importance of interactions in the system, which significantly
affect both the diffusion and fluctuations of charmed hadrons.Comment: 11 pages and 8 captioned figures. Submitted for publicatio
Formation of a Perfect Fluid in , -Pb, Xe-Xe and Pb-Pb Collisions at the Large Hadron Collider Energies
Isothermal compressibility () is an important thermodynamic
observable which gives information about the deviation of a fluid from a
perfect fluid. In this work, for the first time we have estimated the
isothermal compressibility of QCD matter formed in high energy hadronic and
nuclear collisions using color string percolation model (CSPM), where we
investigate the change in as a function of final state charged
particle multiplicity across various collision species. We have also estimated
the initial percolation temperature for different collision systems at
different collision energies, which helps us to have a better understanding of
the system at the initial phase of evolution. The comparison of the CSPM
results for isothermal compressibility with that for the well known fluids,
indicates that the matter formed in heavy-ion collisions might be the {\it
closest perfect fluid} found in nature. This estimation complements the
well-known observation of minimum shear viscosity to entropy density ratio for
a possible QGP medium created in heavy-ion collision experiments. Also, a
threshold of pseudorapidity density of charged particles, is found for a possible QGP formation at the LHC energies.Comment: Xe-Xe data are added to this versio
Thermodynamics of a rotating hadron resonance gas with van der Waals interaction
Studying the thermodynamics of the systems produced in ultra-relativistic
heavy-ion collisions is crucial in understanding the QCD phase diagram.
Recently, a new avenue has opened regarding the implications of large initial
angular momentum and subsequent vorticity in the medium evolution in
high-energy collisions. This adds a new type of chemical potential into the
partonic and hadronic systems, called the rotational chemical potential. We
study the thermodynamics of an interacting hadronic matter under rotation,
formed in an ultra-relativistic collision. We introduce attractive and
repulsive interactions through the van der Waals equation of state.
Thermodynamic properties like the pressure (), energy density
(), entropy density (), trace anomaly (), specific heat () and squared speed of sound () are studied as functions of temperature () for zero and finite
rotation chemical potential. The charge fluctuations, which can be quantified
by their respective susceptibilities, are also studied. The rotational (spin)
density corresponding to the rotational chemical potential is explored. In
addition, we explore the possible liquid-gas phase transition in the hadron gas
with van der Waals interaction in the -- phase space.Comment: 11 pages and 6 captioned figures. Submitted for publicatio
Proton number cumulants in a modified van der Waals hadron resonance gas
An estimate of the proton number cumulants in the hadronic matter is
presented considering a van der Waals-type interaction between the constituent
particles. We argue that the attractive and repulsive parameters in the VDW
hadron resonance gas (VDWHRG) model change as functions of baryochemical
potential () and temperature (). This, in turn, affects the
estimation of thermodynamic properties and, consequently, the conserved charge
fluctuations. We employ a simple parametrization to bring in the center-of-mass
energy () dependence on temperature and baryochemical
potential and then estimate the proton number cumulants with the modified
approach. The modified van der Waals hadron resonance gas model (MVDWHRG)
explains the existing experimental data very well.Comment: 9-pages and 6-captioned figures, Submitted for publicatio
Effect of magnetic field on the optical and thermodynamic properties of a high-temperature hadron resonance gas with van der Waals interactions
We study the behavior of a hadronic matter in the presence of an external
magnetic field within the van der Waals hadron resonance gas (VDWHRG) model,
considering both attractive and repulsive interactions among the hadrons.
Various thermodynamic quantities like pressure (), energy density
(), magnetization (), entropy density (), squared
speed of sound (), specific heat capacity at constant volume
() are calculated as functions of temperature () and static finite
magnetic field (). We also consider the effect of baryochemical potential
() on the above-mentioned thermodynamic observables in the presence of
a magnetic field. Further, we estimate the magnetic susceptibility (), relative permeability (), and electrical susceptibility
() which can help us to understand the system better. With
the information of and dielectric constant (), we
enumerate the refractive index () of the system under consideration.
Through this model, we quantify a liquid-gas phase transition in the
T-eB- phase space.Comment: 18 pages and 5-captioned figures. Submitted for publicatio
and (2S) polarization in proton-proton collisions at the LHC energies using PYTHIA8
The production mechanisms of charmonium states in both hadronic and heavy-ion
collisions hold great significance for investigating the hot and dense QCD
matter. Studying charmonium polarization in ultra-relativistic collisions can
also provide insights into the underlying production mechanisms. With this
motivation, we explore the and (2S) polarization in
proton+proton collisions at = 7, 8, and 13 TeV using a pQCD-inspired
Monte-Carlo event generator called PYTHIA8. This work considers reconstructed
quarkonia through their dimuons decay channel in the ALICE forward rapidity
acceptance range of . Further, we calculate the
polarization parameters , , from the polar and azimuthal angular distributions of the dimuons in
helicity and Collins-Soper frames. This study presents a comprehensive
measurement of the polarization parameters as a function of transverse
momentum, charged-particle multiplicity, and rapidity at the LHC energies. Our
findings of charmonium polarization are in qualitative agreement with the
corresponding experimental data.Comment: 10 pages and 5-captioned figures. Submitted for publicatio
Impact of vorticity and viscosity on the hydrodynamic evolution of hot QCD medium
The strongly interacting transient quark-gluon plasma (QGP) medium created in
ultra-relativistic collisions survive for a duration of a few fm/c. The
spacetime evolution of QGP crucially depends on the equation of state (EoS),
vorticity, viscosity, magnetic field, etc. In the present study, we obtain the
QGP lifetime considering it as a 1+1-dimensionally (1+1) D expanding fluid by
using second-order viscous hydrodynamics. We observe that the coupling of
vorticity and viscosity significantly increases the lifetime of rotating QGP.
Incorporating a static magnetic field along with vorticity and viscosity makes
the evolution slower. However, for a non-rotating medium, the static magnetic
field slightly decreases the QGP lifetime by accelerating the evolution
process. We also report the rate of change of vorticity in the QGP medium,
which can be helpful in studying the medium behavior in detail.Comment: 16 pages and 20 captioned figures. Submitted for publicatio
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