Add to ORKGWe perform an analytic late time analysis for maximal slicing of the Reissner-Nordstr\"om black hole spacetime. In particular, we discuss the collapse of the lapse in terms of its late time behavior at the throat and at the event horizon for the even and the puncture lapse. In the latter case we also determine the value of the lapse at the puncture. Furthermore, in the limit of late times slice stretching effects are studied as they arise for maximal slicing of puncture evolutions. We perform numerical experiments for a Schwarzschild black hole with puncture lapse and find agreement with the analytical results
We expand upon our previous analysis of numerical moving-puncture simulations of the Schwarzschild s...
The strong-field region inside a black hole needs special attention during numerical simulation. One...
We review, without assuming symmetry, why time-independent endstates can be reached in black hole an...
We perform an analytic late time analysis for maximal slicing of the Reissner-Nordstr\"om black hole...
We prove by explicit construction that there exists a maximal slicing of the Schwarzschild spacetime...
A time-symmetric Cauchy slice of the extended Schwarzschild spacetime can evolve into a foliation of...
Slice stretching effects such as slice sucking and slice wrapping arise when foliating the extended ...
Currently the most popular method to evolve black-hole binaries is the ``moving puncture'' method. I...
Slice stretching effects are discussed as they arise at the event horizon when geodesically slicing ...
Numerical relativity has faced the problem that standard 3+1 simulations of black hole spacetimes wi...
The ``moving puncture'' technique has led to dramatic advancements in the numerical simulations of b...
In this brief note, we revisit the study of the leading order late time decay tails of massless scal...
We apply a new analytic scheme, developed in a preceding paper, in order to calculate the late time ...
The moving-puncture technique has led to dramatic advancements in the numerical simulations of bin...
We present a new analytic approach for the study of late time evolution of linear test-fields, propa...
We expand upon our previous analysis of numerical moving-puncture simulations of the Schwarzschild s...
The strong-field region inside a black hole needs special attention during numerical simulation. One...
We review, without assuming symmetry, why time-independent endstates can be reached in black hole an...
We perform an analytic late time analysis for maximal slicing of the Reissner-Nordstr\"om black hole...
We prove by explicit construction that there exists a maximal slicing of the Schwarzschild spacetime...
A time-symmetric Cauchy slice of the extended Schwarzschild spacetime can evolve into a foliation of...
Slice stretching effects such as slice sucking and slice wrapping arise when foliating the extended ...
Currently the most popular method to evolve black-hole binaries is the ``moving puncture'' method. I...
Slice stretching effects are discussed as they arise at the event horizon when geodesically slicing ...
Numerical relativity has faced the problem that standard 3+1 simulations of black hole spacetimes wi...
The ``moving puncture'' technique has led to dramatic advancements in the numerical simulations of b...
In this brief note, we revisit the study of the leading order late time decay tails of massless scal...
We apply a new analytic scheme, developed in a preceding paper, in order to calculate the late time ...
The moving-puncture technique has led to dramatic advancements in the numerical simulations of bin...
We present a new analytic approach for the study of late time evolution of linear test-fields, propa...
We expand upon our previous analysis of numerical moving-puncture simulations of the Schwarzschild s...
The strong-field region inside a black hole needs special attention during numerical simulation. One...
We review, without assuming symmetry, why time-independent endstates can be reached in black hole an...