Exploring Quark Matter under Extreme Scenarios of Temperature and Density

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "High Energy Nuclear and Particle Physics".

Deadline for manuscript submissions: 30 April 2024 | Viewed by 1334

Special Issue Editors


E-Mail Website
Guest Editor
Institute of Nuclear Physics (Instytut Fizyki Jądrowej Akademii Nauk), Walerego Eljasza-Radzikowskiego 152, 31-342 Kraków, Poland
Interests: heavy ion collisions; jet quenching; parton showers

E-Mail Website
Guest Editor
Department of Physical Sciences, IISER Berhampur, IISER Berhampur Transit Campus (Govt. ITI Building) Engg. School Junction, Berhampur Odisha 760010, India
Interests: phenomenology of relativistic heavy ion collisions

E-Mail Website
Guest Editor
Department of Basic Sciences, Mukesh Patel School of Technology Management and Engineering, NMIMS University, Mumbai 400056, India
Interests: phenomenology of relativistic heavy ion collisions; neutron stars

Special Issue Information

Dear Colleagues,

RHIC and LHC programs aim to explore and potentially discover a critical point or a first-order phase transition in the quantum chromodynamics (QCD) phase diagram. The significance of such a discovery lies in its implications for our understanding of QCD as it would signify a clear distinction between quark–gluon plasma (QGP) and hadronic matter. Collisions at very high energies explore a regime akin to that of the early universe, i.e., characterized by high temperature and low baryon chemical potential. On the other hand, collisions at low energies create systems that closely resemble those found in neutron star mergers, featuring low temperature and high baryon chemical potential. Numerous intriguing questions arise from these collision regimes. Addressing these questions through dedicated studies will foster fruitful work in the fluid dynamics and transport theories of both heavy-ion physics and neutron stars.

The objective of this Special Issue is to compile a comprehensive assortment of both comprehensive reviews and novel research articles that describe nuclear theory and experiments in the context of heavy-ion collisions and mergers of two or more neutron stars. The topics in heavy-ion collisions encompass many-body theory and chiral effective field theory, perturbative QCD, transport coefficients, relativistic viscous fluid dynamics, jets, electromagnetic probes, collective dynamics, early time electromagnetic fields, baryon stopping and dynamics of conserved charges, polarization, and spin alignment. Additionally, from the realm of neutron star mergers, the addressed subjects include the examination of phase transition signatures, chemical equilibration and the role of magnetic fields. We cordially invite contributions from both the theoretical and experimental domains.

Points: jets; collective dynamics; electromagnetic probes; equation of state; transport coefficients in merger; phase transition; magnetic evolution; electromagnetic fields in heavy ion collisions and neutron star mergers; polarisation and spin alignment; conserved charge dynamics

Dr. Souvik Priyam Adhya
Dr. Sandeep Chatterjee
Dr. Sreemoyee Sarkar
Guest Editors

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.

Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Universe is an international peer-reviewed open access monthly journal published by MDPI.

Please visit the Instructions for Authors page before submitting a manuscript. Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.

Keywords

  • heavy ion collisions
  • quark–gluon plasma
  • hard probes
  • collective dynamics
  • saturation
  • neutron star mergers
  • equation of state
  • transport coefficients
  • electromagnetic probes
  • chirality
  • small systems

Published Papers (1 paper)

Order results
Result details
Select all
Export citation of selected articles as:

Review

54 pages, 757 KiB  
Review
Transport Coefficients of Relativistic Matter: A Detailed Formalism with a Gross Knowledge of Their Magnitude
by Ashutosh Dwibedi, Nandita Padhan, Arghya Chatterjee and Sabyasachi Ghosh
Universe 2024, 10(3), 132; https://doi.org/10.3390/universe10030132 - 07 Mar 2024
Viewed by 941
Abstract
The present review article has attempted a compact formalism description of transport coefficient calculations for relativistic fluid, which is expected in heavy ion collision experiments. Here, we first address the macroscopic description of relativistic fluid dynamics and then its microscopic description based on [...] Read more.
The present review article has attempted a compact formalism description of transport coefficient calculations for relativistic fluid, which is expected in heavy ion collision experiments. Here, we first address the macroscopic description of relativistic fluid dynamics and then its microscopic description based on the kinetic theory framework. We also address different relaxation time approximation-based models in Boltzmann transport equations, which make a sandwich between Macro and Micro frameworks of relativistic fluid dynamics and finally provide different microscopic expressions of transport coefficients like the fluid’s shear viscosity and bulk viscosity. In the numeric part of this review article, we put stress on the two gross components of transport coefficient expressions: relaxation time and thermodynamic phase-space part. Then, we try to tune the relaxation time component to cover earlier theoretical estimations and experimental data-driven estimations for RHIC and LHC matter. By this way of numerical understanding, we provide the final comments on the values of transport coefficients and relaxation time in the context of the (nearly) perfect fluid nature of the RHIC or LHC matter. Full article
Show Figures

Figure 1

Back to TopTop