Editing Relativistic Euler equations (section)

{{More citations needed|date=April 2020}}
In [[fluid mechanics]] and [[astrophysics]], the '''relativistic Euler equations''' are a generalization of the [[Euler equations (fluid dynamics)|Euler equations]] that account for the effects of [[general relativity]]. They have applications in [[high-energy astrophysics]] and [[numerical relativity]], where they are commonly used for describing phenomena such as [[gamma-ray burst]]s, [[Accretion disk|accretion phenomena]], and [[neutron star]]s, often with the addition of a [[Magnetohydrodynamics|magnetic field]].<ref name=":0">{{Cite book|last=Rezzolla, L. (Luciano)|title=Relativistic hydrodynamics|others=Zanotti, Olindo|date=14 June 2018|isbn=978-0-19-880759-9|location=Oxford|oclc=1044938862}}</ref> ''Note: for consistency with the literature, this article makes use of [[natural units]], namely the speed of light'' <math>c=1</math> ''and the [[Einstein notation|Einstein summation convention]].''