Stable characteristic evolution of generic three-dimensional single-black-hole spacetimes

Binary Black Hole Grand Challenge Alliance

doi:10.1103/PhysRevLett.80.3915

Stable characteristic evolution of generic three-dimensional single-black-hole spacetimes

Binary Black Hole Grand Challenge Alliance

Physics

Research output: Contribution to journal › Article › peer-review

87 Scopus citations

Abstract

We report new results which establish that the accurate three-dimensional numerical simulation of generic single-black-hole spacetimes has been achieved by characteristic evolution with unlimited long term stability. Our results include distorted, moving, and spinning single black holes, with evolution times up to 60000M.

Original language	English (US)
Pages (from-to)	3915-3918
Number of pages	4
Journal	Physical review letters
Volume	80
Issue number	18
DOIs	https://doi.org/10.1103/PhysRevLett.80.3915
State	Published - 1998

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

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10.1103/PhysRevLett.80.3915

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@article{890420ebeff94cbc8e1b20f68460f4eb,

title = "Stable characteristic evolution of generic three-dimensional single-black-hole spacetimes",

abstract = "We report new results which establish that the accurate three-dimensional numerical simulation of generic single-black-hole spacetimes has been achieved by characteristic evolution with unlimited long term stability. Our results include distorted, moving, and spinning single black holes, with evolution times up to 60000M.",

author = "\{Binary Black Hole Grand Challenge Alliance\} and R. G{\'o}mez and L. Lehner and Marsa, \{R. L.\} and J. Winicour and Abrahams, \{A. M.\} and A. Anderson and P. Anninos and Baumgarte, \{T. W.\} and Bishop, \{N. T.\} and Brandt, \{S. R.\} and Browne, \{J. C.\} and K. Camarda and Choptuik, \{M. W.\} and Cook, \{G. B.\} and R. Correll and Evans, \{C. R.\} and Finn, \{L. S.\} and Fox, \{G. C.\} and T. Haupt and Huq, \{M. F.\} and Kidder, \{L. E.\} and Klasky, \{S. A.\} and P. Laguna and W. Landry and J. Lenaghan and J. Masso and Matzner, \{R. A.\} and S. Mitra and P. Papadopoulos and M. Parashar and L. Rezzolla and Rupright, \{M. E.\} and F. Saied and Saylor, \{P. E.\} and Scheel, \{M. A.\} and E. Seidel and Shapiro, \{S. L.\} and D. Shoemaker and L. Smarr and B. Szil{\'a}gyi and Teukolsky, \{S. A.\} and \{Van Putten\}, \{M. H.P.M.\} and P. Walker and York, \{J. W.\}",

year = "1998",

doi = "10.1103/PhysRevLett.80.3915",

language = "English (US)",

volume = "80",

pages = "3915--3918",

journal = "Physical review letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "18",

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TY - JOUR

T1 - Stable characteristic evolution of generic three-dimensional single-black-hole spacetimes

AU - Binary Black Hole Grand Challenge Alliance

AU - Gómez, R.

AU - Lehner, L.

AU - Marsa, R. L.

AU - Winicour, J.

AU - Abrahams, A. M.

AU - Anderson, A.

AU - Anninos, P.

AU - Baumgarte, T. W.

AU - Bishop, N. T.

AU - Brandt, S. R.

AU - Browne, J. C.

AU - Camarda, K.

AU - Choptuik, M. W.

AU - Cook, G. B.

AU - Correll, R.

AU - Evans, C. R.

AU - Finn, L. S.

AU - Fox, G. C.

AU - Haupt, T.

AU - Huq, M. F.

AU - Kidder, L. E.

AU - Klasky, S. A.

AU - Laguna, P.

AU - Landry, W.

AU - Lenaghan, J.

AU - Masso, J.

AU - Matzner, R. A.

AU - Mitra, S.

AU - Papadopoulos, P.

AU - Parashar, M.

AU - Rezzolla, L.

AU - Rupright, M. E.

AU - Saied, F.

AU - Saylor, P. E.

AU - Scheel, M. A.

AU - Seidel, E.

AU - Shapiro, S. L.

AU - Shoemaker, D.

AU - Smarr, L.

AU - Szilágyi, B.

AU - Teukolsky, S. A.

AU - Van Putten, M. H.P.M.

AU - Walker, P.

AU - York, J. W.

PY - 1998

Y1 - 1998

N2 - We report new results which establish that the accurate three-dimensional numerical simulation of generic single-black-hole spacetimes has been achieved by characteristic evolution with unlimited long term stability. Our results include distorted, moving, and spinning single black holes, with evolution times up to 60000M.

AB - We report new results which establish that the accurate three-dimensional numerical simulation of generic single-black-hole spacetimes has been achieved by characteristic evolution with unlimited long term stability. Our results include distorted, moving, and spinning single black holes, with evolution times up to 60000M.

UR - https://www.scopus.com/pages/publications/4243654605

UR - https://www.scopus.com/pages/publications/4243654605#tab=citedBy

U2 - 10.1103/PhysRevLett.80.3915

DO - 10.1103/PhysRevLett.80.3915

M3 - Article

AN - SCOPUS:4243654605

SN - 0031-9007

VL - 80

SP - 3915

EP - 3918

JO - Physical review letters

JF - Physical review letters

IS - 18

ER -

Stable characteristic evolution of generic three-dimensional single-black-hole spacetimes

Abstract

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