Non-boost-invariant solution of relativistic hydrodynamics in 1+3 dimensions

Yoshitaka Hatta; Bo Wen Xiao; Di Lun Yang

doi:10.1103/PhysRevD.93.016012

Non-boost-invariant solution of relativistic hydrodynamics in 1+3 dimensions

Yoshitaka Hatta, Bo Wen Xiao, Di Lun Yang

Research output: Contribution to journal › Article › peer-review

5 Citations (Scopus)

Abstract

We present a new solution of relativistic hydrodynamics in 1+3 dimensions which depends on both the transverse coordinate and rapidity. At early times the flow expands dominantly longitudinally in a nonboost-invariant manner, and at late times it expands nearly spherically. These two regimes are shown to be related by symmetry. The effect of viscosity is also discussed.

Original language	English
Article number	016012
Journal	Physical Review D
Volume	93
Issue number	1
DOIs	https://doi.org/10.1103/PhysRevD.93.016012
Publication status	Published - 2016 Jan 27
Externally published	Yes

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.93.016012

Cite this

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title = "Non-boost-invariant solution of relativistic hydrodynamics in 1+3 dimensions",

abstract = "We present a new solution of relativistic hydrodynamics in 1+3 dimensions which depends on both the transverse coordinate and rapidity. At early times the flow expands dominantly longitudinally in a nonboost-invariant manner, and at late times it expands nearly spherically. These two regimes are shown to be related by symmetry. The effect of viscosity is also discussed.",

author = "Yoshitaka Hatta and Xiao, {Bo Wen} and Yang, {Di Lun}",

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N2 - We present a new solution of relativistic hydrodynamics in 1+3 dimensions which depends on both the transverse coordinate and rapidity. At early times the flow expands dominantly longitudinally in a nonboost-invariant manner, and at late times it expands nearly spherically. These two regimes are shown to be related by symmetry. The effect of viscosity is also discussed.

AB - We present a new solution of relativistic hydrodynamics in 1+3 dimensions which depends on both the transverse coordinate and rapidity. At early times the flow expands dominantly longitudinally in a nonboost-invariant manner, and at late times it expands nearly spherically. These two regimes are shown to be related by symmetry. The effect of viscosity is also discussed.

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Non-boost-invariant solution of relativistic hydrodynamics in 1+3 dimensions

Abstract

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