(3+1)-dimensional relativistic hydrodynamical expansion of hot and dense matter in ultra-relativistic nuclear collision

Chiho Nonaka; Eiji Honda; Shin Muroya

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(3+1)-dimensional relativistic hydrodynamical expansion of hot and dense matter in ultra-relativistic nuclear collision

Chiho Nonaka, Eiji Honda, Shin Muroya

High Energy Physics - Phenomenology · Submitted 18 Jul 2000

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim Applying hydrodynamical calculations to the deformed uranium collisions at AGS energy region, we discuss the nature of space-time structure and particle distributions in detail.

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arXiv IDhep-ph/0007187 (version 2)

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CitationChiho Nonaka, Eiji Honda, Shin Muroya. "(3+1)-dimensional relativistic hydrodynamical expansion of hot and dense matter in ultra-relativistic nuclear collision." arXiv:hep-ph/0007187 (2000). https://pith.science/paper/SEL2UTW4

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What the abstract itself states, as probabilities: claims first 0.07 · states limitation 0.07 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.04 · compares with prior results 0.07 · mentions code or data availability 0.02.

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arXiv listing abstract v2. Results and the main claim are underlined; show every role.

A full (3+1)-dimensional calculation using the Lagrangian hydrodynamics is proposed for relativistic nuclear collisions. The calculation enables us to evaluate anisotropic flow of hadronic matter which appears in non-central and/or asymmetrical relativistic nuclear collisions. Applying hydrodynamical calculations to the deformed uranium collisions at AGS energy region, we discuss the nature of space-time structure and particle distributions in detail.

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#	sentence	role	the authors' own work	states the main conclusion	strength
s0	A full (3+1)-dimensional calculation using the Lagrangian hydrodynamics is proposed for relativistic nuclear collisions.	method 0.51	0.61	0.08	asserted 0.83
s1	The calculation enables us to evaluate anisotropic flow of hadronic matter which appears in non-central and/or asymmetrical relativistic nuclear collisions.	contribution 0.73	0.48	0.14	asserted 0.83
s2	Applying hydrodynamical calculations to the deformed uranium collisions at AGS energy region, we discuss the nature of space-time structure and particle distributions in detail.	contribution 0.73	0.88	0.21	asserted 0.91

What kind of paper the classifier reports this is: method or tool 0.53 · evidence from simulation or computation 1.00.

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arXiv listing abstract v2

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figures and tables
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Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper

Original abstract

A full (3+1)-dimensional calculation using the Lagrangian hydrodynamics is proposed for relativistic nuclear collisions. The calculation enables us to evaluate anisotropic flow of hadronic matter which appears in non-central and/or asymmetrical relativistic nuclear collisions. Applying hydrodynamical calculations to the deformed uranium collisions at AGS energy region, we discuss the nature of space-time structure and particle distributions in detail.

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References

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6 arXiv papers cite this in 6 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 2 sentences without a confident label

Uses its method or tool 1 paper

For our purpose, we have to infer parton and hadron number density from the energy density or temperature provided by the hydrodynamic solution, which uses a Bag model for the equation of state (EOS) [ref] .

Bulk matter evolution and extraction of jet transport parameter in heavy-ion collisions at RHIC · (1+3)d Ideal Hydrodynamical Expansion · 0.81

Cites it as background 3 papers

Nowadays, the relativistic hydrodynamics is regarded as the best theoretical framework for description of the spacetime evolution of strongly interacting matter produced in ultra-relativistic heavy-ion collisions [ref] , for a recent review see [ref] .

Hydrodynamic description of particle production in relativistic heavy-ion collisions · Introduction · 0.90
The hadronic phase is described using a resonance gas and the QGP phase using a parton gas with a bag constant [ref] .

QCD Equation of State at Finite Chemical Potentials for Relativistic Nuclear Collisions · From bag model to lattice QCD · 0.93
Historically, the first hydrodynamic models of heavy-ion collisions were developed with an emphasis on the fluid dynamics of QGP [ref] .

Comparisons and Predictions for Collisions of deformed $^{238}$U nuclei at $\sqrt{s_{NN}} = 193$ GeV · IP-Glasma · 1.00

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