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3+1 formalism and bases of numerical relativity - LUTh ...

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82 <strong>3+1</strong> equations for matter <strong>and</strong> electromagnetic field<br />

The Newtonian limit <strong>of</strong> this equation is [cf. Eqs. (5.15) <strong>and</strong> (5.59)]<br />

∂Ui<br />

∂t + Uj DjUi = − 1<br />

DiP − DiΦ, (5.69)<br />

ρ0<br />

i.e. the st<strong>and</strong>ard Euler equation in presence <strong>of</strong> a gravitational field <strong>of</strong> potential Φ.<br />

5.3.6 Further developments<br />

For further developments in <strong>3+1</strong> relativistic hydrodynamics, we refer to the review article by<br />

Font [124]. Let us also point out that the <strong>3+1</strong> decomposition presented above is not very<br />

convenient for discussing conservation laws, such as the relativistic generalizations <strong>of</strong> Bernoulli’s<br />

theorem or Kelvin’s circulation theorem. For this purpose the Carter-Lichnerowicz approach,<br />

which is based on exterior calculus, is much more powerfull, as discussed in Ref. [143].<br />

5.4 Electromagnetic field<br />

not written up yet; see Ref. [258].<br />

5.5 <strong>3+1</strong> magnetohydrodynamics<br />

not written up yet; see Refs. [45, 235, 22].

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