2004
DOI: 10.1103/physrevc.70.024906
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Constrained molecular dynamics simulation of the quark-gluon plasma

Abstract: We calculate the Equation of State of a quark system interacting through a phenomenological potential: the Richardson's potential, at finite baryon density and zero temperature. In particular we study three different cases with different quark masses(u and d), and different assumptions for the potential at large distances. We solve molecular dynamics with a constraint due to Pauli blocking and find evidencies of a phase transition from "nuclear" to "quark matter", which is analyzed also through the behaviour o… Show more

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Cited by 17 publications
(6 citation statements)
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“…When considering the interaction of nucleons at short enough distances, the point particle assumption is not proper and the size of the nucleon should be taken into account. In CoMD [8,9,10,11,12,13,14], the nucleons are assumed to have a Gaussian distribution with width σ r…”
Section: Folding For Comdmentioning
confidence: 99%
See 1 more Smart Citation
“…When considering the interaction of nucleons at short enough distances, the point particle assumption is not proper and the size of the nucleon should be taken into account. In CoMD [8,9,10,11,12,13,14], the nucleons are assumed to have a Gaussian distribution with width σ r…”
Section: Folding For Comdmentioning
confidence: 99%
“…In this first paper we only discuss the perturbative effect on the energy. We will introduce the correction into the microscopic model Constrained Molecular Dynamics (CoMD) [8,9,10,11,12,13,14], and in following research we will discuss actual production. The structure of this paper is as follows.…”
Section: Introductionmentioning
confidence: 99%
“…In contrast, the field of computational plasma physics has traditionally relied on hydrodynamics [5,6] and kinetic [7,8] codes because the temporal and spatial scales of interest are much too large for MD to be tractable; moreover, the detailed description of discrete particles is less important and instead macroscopic field variables are computed. However, MD plays a central role in a diverse set of plasma subfields concerned with understanding microscopic particles such as astrophysical systems [9,10], dusty plasmas [11,12], ultracold neutral plasmas [13,14], dense plasmas [15,16], low temperature plasmas [17,18], plasma beams [19,20], quark-gluon plasmas [21,22], etc.…”
Section: Introductionmentioning
confidence: 99%
“…One possibility to avoid this problem is, instead of using the Pauli potential, to maintain the Pauli principle of the system by stochastic rearrangements of particle momenta [25]. This model was originally developed for nucleon systems and was applied also to the quark system very recently [26].…”
Section: Pauli Potentialmentioning
confidence: 99%