Stability of three-dimensional relativistic jets: implications for jet collimation

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Table 1:

Parameters of the simulations discussed in this paper.
Model	$\gamma_{\rm j}$	$M_{\rm j}$	$\rho_{\rm j}/\rho_{\rm a}$	$\Gamma$	$\varepsilon_{\rm j} (c^2)$	$\varepsilon_{\rm a}(c^2)$	$c_{\rm sj} (c)$	Resolution (cells/ $R_{\rm j}$ )
B05 (3D)	5.0	13.2	0.1	4/3	0.42	0.042	0.35	32/64^a
B05 (2D)	-	-	-	-	-	-	-	32/ $128\times 256$ ^b
D10 (3D)	10.0	14.2	0.1	4/3	60.0	6.0	0.57	32
B20 (3D)	20.0	54.0	0.1	4/3	0.42	0.042	0.35	32
B20 (2D)	-	-	-	-	-	-	-	32/ $128\times 256$ ^b

Notes. ^(a) This simulation was repeated (in the linear regime only) doubling the resolution. ^(b) The numbers correspond to the axial times radial resolution when it is not the same in all the dimensions.

Source LaTeX | All tables | In the text

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