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. Author manuscript; available in PMC: 2021 Sep 28.
Published in final edited form as: Phys Rev D. 2018 Nov 12;98(10):103008. doi: 10.1103/physrevd.98.103008

TABLE II.

Grid structure for all cases listed in Table I. The computational mesh consists of one set of j-nested AMR grids centered at the start, in which equatorial symmetry is imposed. Here j = 5, …, levelmax denotes the number of AMR grids during a given evolution epoch, and levelmax is the maximum number of AMR grids at the end of the simulations. Each case begins with a set of j = 5-AMR grids, and we add a new refinement level every time the maximum value of the rest-mass density increases by a factor of three. The finest level for a given set of j-nested grids is denoted by Δxmin. The grid spacing of all other levels is 2l−1Δxmin, where l = 1, …, j, is the level number such that l = 1 corresponds to the coarsest level. The half-side length of the outermost AMR boundary is given by the first number in the grid hierarchy.

Case Δxmin levelmax Grid hierarchy
n3-HYD 1.36M/2j−5 10 1312M/2l−1
n3-INT 1.36M/2j−5 11 1312M/2l−1
n3-EXTINT 1.36M/2j−5 11 1312M/2l−1
n295-EXTINT 0.4M/2j−5 9 728M/2l−1
n29-HYD 0.48M/2j−5 9 454M/2l−1
n29-INT 0.48M/2j−5 9 454M/2l−1
n29-EXTINT 0.48M/2j−5 9 454M/2l−1
n29-EXTINT-0.75SPIN 0.48M/2j−5 9 458M/2l−1
n29-EXTINT-DIFF 0.40M/2j−5 9 515M/2l−1