Local simulations of the magnetized Kelvin-Helmholtz instability in neutron-star mergers

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Table A.7:

Same as Table A.6 but for the 3D merger-motivated models simulated on grids of 128³ and 256³ zones, respectively.
b₀^x [10¹³ G]	$\mathsf{M}= 1$		$\mathsf{M}= 4$
	128³	256³	128³	256³
5	$\surd$	$\surd$
$\pm 5$	$\surd$	$\surd$
10	$\surd$	$\surd$	$\surd$	$\surd$
$\pm 10$	$\surd$	$\surd$	$\surd$	$\surd$
20	$\surd$	$\surd$	$\surd$	$\surd$
$\pm 20$	$\surd$	$\surd$	$\surd$	$\surd$
40		$\surd$	$\surd$	$\surd$
$\pm 40$		$\surd$	$\surd$	$\surd$

Source LaTeX | All tables | In the text

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