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Published byKatrina Nicholson Modified over 8 years ago
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1+log slicing in gravitational collapse
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Ingredients of successful binary black hole simulations Pretorius Generalized harmonic coordinates Excision ____________________________ Campanelli et al and Baker et al BSSN 1+log slicing Gamma freezing shift Moving punctures
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Why do these approaches work? BSSN and Harmonic because they make Einstein’s equation look like the wave equation Excision because it gets rid of “grid stretching” 1+log slicing ??? Gamma freezing shift ??? Moving punctures ???
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Look at one ingredient at a time 1+log slicing It has been suggested by Rezzolla et al that 1+log slicing and Gamma freezing shift be used in collapse simulations The slicing doesn’t commit you to a particular form of Einstein’s equations
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Look at the ingredient in a simple context Spherically symmetric gravitational collapse Scalar field matter Radial length as the spatial coordinate
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Maximal slicing Lapse should be small in the middle and approach 1 on the outside to avoid the singularity K=0 D a D a =[ ]
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Maximal slicing lapse length
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Maximal slicing area radius r length
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1+log slicing Elliptic equations take too long to solve, Try something else t – i i = - 2 K This should make small if K is positive But what if K is negative?
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1+log slicing lapse length
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1+log slicing K K length
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1+log slicing lapse with excision length
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1+log slicing K with excision K length
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Conclusions 1+log slicing is dangerous, use with caution. Use it only with excision 1+log slicing works with moving punctures because moving punctures are “excision without excision”
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