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

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

Figure 5.2: Coordinate velocity V <strong>of</strong> the fluid defined as the ratio <strong>of</strong> the fluid displacement with respect to the<br />

line <strong>of</strong> constant spatial coordinates to the coordinate time increment dt.<br />

From the very definition <strong>of</strong> the shift vector (cf. Sec. 4.2.2), the drift <strong>of</strong> the coordinate line<br />

x i = const from the Eulerian observer worldline between t <strong>and</strong> t + dt is the vector dt β. Hence<br />

we have (cf. Fig. 5.2)<br />

dℓ = dt β + dx. (5.40)<br />

Dividing this relation by dτ, using Eqs. (5.33), (3.15) <strong>and</strong> (5.37) yields<br />

U = 1<br />

(V + β) . (5.41)<br />

N<br />

On this expression, it is clear that at the Newtonian limit as given by (5.15), U = V .<br />

5.3.2 Baryon number conservation<br />

In addition to ∇ · T = 0, the perfect fluid must obey to the fundamental law <strong>of</strong> baryon number<br />

conservation:<br />

∇ · jB = 0 , (5.42)<br />

where jB is the baryon number 4-current, expressible in terms <strong>of</strong> the fluid 4-velocity <strong>and</strong><br />

the fluid proper baryon number density nB as<br />

jB = nBu . (5.43)<br />

The baryon number density measured by the Eulerian observer is<br />

NB := −jB · n. (5.44)

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