Slice stretching effects such as slice sucking and slice wrapping arise when foliating the extended Schwarzschild spacetime with maximal slices. For arbitrary spatial coordinates these effects are quantified here in the context of boundary conditions where the lapse arises as a linear combination of odd and even lapse. Favourable boundary conditions are then derived which make the overall slice stretching occur late in numerical simulations. Allowing the lapse to become negative, this requirement leads to lapse functions which approach at late times the odd lapse corresponding to the static Schwarzschild metric. Demanding, however, that a numerically favourable lapse remains non-negative, as a result the average of odd and even lapse is obt...
We present long-term stable and second-order convergent evolutions of an excised wobbling black hole...
The strong-field region inside a black hole needs special attention during numerical simulation. One...
We expand upon our previous analysis of numerical moving-puncture simulations of the Schwarzschild s...
Slice stretching effects such as slice sucking and slice wrapping arise when foliating the extended ...
Slice stretching effects are discussed as they arise at the event horizon when geodesically slicing ...
We prove by explicit construction that there exists a maximal slicing of the Schwarzschild spacetime...
Numerical relativity has faced the problem that standard 3+1 simulations of black hole spacetimes wi...
We perform an analytic late time analysis for maximal slicing of the Reissner-Nordstr\"om black hole...
A time-symmetric Cauchy slice of the extended Schwarzschild spacetime can evolve into a foliation of...
Currently the most popular method to evolve black-hole binaries is the "moving puncture" method. It ...
The ``moving puncture'' technique has led to dramatic advancements in the numerical simulations of b...
We analyze stationary slicings of the Schwarzschild spacetime defined by members of the Bona-Masso f...
We give a detailed description of the constant mean curvature foliations in Schwarzschild spacetime,...
We consider a family of spherical three-dimensional spacelike slices embedded in the Schwarzschild s...
The moving-puncture technique has led to dramatic advancements in the numerical simulations of bin...
We present long-term stable and second-order convergent evolutions of an excised wobbling black hole...
The strong-field region inside a black hole needs special attention during numerical simulation. One...
We expand upon our previous analysis of numerical moving-puncture simulations of the Schwarzschild s...
Slice stretching effects such as slice sucking and slice wrapping arise when foliating the extended ...
Slice stretching effects are discussed as they arise at the event horizon when geodesically slicing ...
We prove by explicit construction that there exists a maximal slicing of the Schwarzschild spacetime...
Numerical relativity has faced the problem that standard 3+1 simulations of black hole spacetimes wi...
We perform an analytic late time analysis for maximal slicing of the Reissner-Nordstr\"om black hole...
A time-symmetric Cauchy slice of the extended Schwarzschild spacetime can evolve into a foliation of...
Currently the most popular method to evolve black-hole binaries is the "moving puncture" method. It ...
The ``moving puncture'' technique has led to dramatic advancements in the numerical simulations of b...
We analyze stationary slicings of the Schwarzschild spacetime defined by members of the Bona-Masso f...
We give a detailed description of the constant mean curvature foliations in Schwarzschild spacetime,...
We consider a family of spherical three-dimensional spacelike slices embedded in the Schwarzschild s...
The moving-puncture technique has led to dramatic advancements in the numerical simulations of bin...
We present long-term stable and second-order convergent evolutions of an excised wobbling black hole...
The strong-field region inside a black hole needs special attention during numerical simulation. One...
We expand upon our previous analysis of numerical moving-puncture simulations of the Schwarzschild s...