Where do moving punctures go? - INSPIRE

DataBETA

Where do moving punctures go?

Dec, 2006

9 pages

Part of Einstein's legacy: From the theoretical paradise to astrophysical observations

Published in:

J.Phys.Conf.Ser. 66 (2007) 012047

Contribution to:

29th Spanish Relativity Meeting (ERE 2006): Einstein's Legacy: From the Theoretical Paradise to Astrophysical Observation

e-Print:

gr-qc/0612097 [gr-qc]

DOI:

10.1088/1742-6596/66/1/012047

View in:

ADS Abstract Service

reference search60 citations

Citations per year

Abstract: (arXiv)

Currently the most popular method to evolve black-hole binaries is the ``moving puncture'' method. It has recently been shown that when puncture initial data for a Schwarzschild black hole are evolved using this method, the numerical slices quickly lose contact with the second asymptotically flat end, and end instead on a cylinder of finite Schwarzschild coordinate radius. These slices are stationary, meaning that their geometry does not evolve further. We will describe these results in the context of maximal slices, and present time-independent puncture-like data for the Schwarzschild spacetime.

Note:

Proceedings for 29th Spanish Relativity Meeting. Added more details about the time-independent solution, with reference to the analytic result of Baumgarte and Naculich

References(26)

Figures(11)

[1]

Interaction energy in geometrostatics

Dieter R. Brill
(
- Yale U.
)
,
Richard W. Lindquist
(
- Adelphi U.
)

- Phys.Rev. 131 (1963) 471-476
•
DOI:
- 10.1103/PhysRev.131.471

[2]

A Simple construction of initial data for multiple black holes

- Phys.Rev.Lett. 78 (1997) 3606-3609
•
e-Print:
- gr-qc/9703066
•
DOI:
- 10.1103/PhysRevLett.78.3606

[3]

Asymptotically flat and regular Cauchy data

Sergio Dain
(
- Potsdam, Max Planck Inst.
)

- Lect.Notes Phys. 604 (2002) 161-182,
•
e-Print:
- gr-qc/0203021

[4]

Binary black hole mergers in 3-d numerical relativity

Bernd Bruegmann
(
- Potsdam, Max Planck Inst.
)

- Int.J.Mod.Phys.D 8 (1999) 85
•
e-Print:
- gr-qc/9708035
•
DOI:
- 10.1142/S0218271899000080

[5]

The 3-D grazing collision of two black holes

et al.

- Phys.Rev.Lett. 87 (2001) 271103
•
e-Print:
- gr-qc/0012079
•
DOI:
- 10.1103/PhysRevLett.87.271103

[6]

Maximal slicing for puncture evolutions of Schwarzschild and Reissner-Nordstrom black holes

- Phys.Rev.D 69 (2004) 044006
•
e-Print:
- gr-qc/0307036
•
DOI:
- 10.1103/PhysRevD.69.044006

[7]

Late time analysis for maximal slicing of Reissner-Nordstrom puncture evolutions

Bernd Reimann
(
- Potsdam, Max Planck Inst. and
- Mexico U., ICN
)
,
Bernd Bruegmann
(
- Penn State U.
)

- Phys.Rev.D 69 (2004) 124009
•
e-Print:
- gr-qc/0401098
•
DOI:
- 10.1103/PhysRevD.69.124009

[8]

Accurate evolutions of orbiting black-hole binaries without excision

Manuela Campanelli
(
- Texas U., Brownsville and
- Texas U., Brownsville, CGWA
)
,
C.O. Lousto
(
- Texas U., Brownsville and
- Texas U., Brownsville, CGWA
)
,
P. Marronetti
(
- Florida Atlantic U.
)
,
Y. Zlochower
(
- Texas U., Brownsville and
- Texas U., Brownsville, CGWA
)

- Phys.Rev.Lett. 96 (2006) 111101
•
e-Print:
- gr-qc/0511048
•
DOI:
- 10.1103/PhysRevLett.96.111101

[9]

Gravitational wave extraction from an inspiraling configuration of merging black holes

- Phys.Rev.Lett. 96 (2006) 111102
•
e-Print:
- gr-qc/0511103
•
DOI:
- 10.1103/PhysRevLett.96.111102

[10]

Evolution of binary black hole spacetimes

Frans Pretorius
(
- Caltech and
- Alberta U.
)

- Phys.Rev.Lett. 95 (2005) 121101
•
e-Print:
- gr-qc/0507014
•
DOI:
- 10.1103/PhysRevLett.95.121101

[11]

Unequal Mass Binary Black Hole Plunges and Gravitational Recoil

e-Print:
- gr-qc/0601026

[12]

Binary black-hole evolutions of excision and puncture data

Ulrich Sperhake
(
- Jena U., TPI
)

- Phys.Rev.D 76 (2007) 104015
•
e-Print:
- gr-qc/0606079
•
DOI:
- 10.1103/PhysRevD.76.104015

[13]

Solving Einstein's equations with dual coordinate frames

Mark A. Scheel
(
- Caltech
)
,
Harald P. Pfeiffer
(
- Caltech
)
,
Lee Lindblom
(
- Caltech
)
,
Lawrence E. Kidder
(
- Cornell U., Radio. Space Res. Ctr.
)
,
Oliver Rinne
(
- Caltech
)

et al.

- Phys.Rev.D 74 (2006) 104006
•
e-Print:
- gr-qc/0607056
•
DOI:
- 10.1103/PhysRevD.74.104006

[14]

Calibration of Moving Puncture Simulations

Bernd Bruegmann
(
- Jena U.
)
,
Jose A. Gonzalez
(
- Jena U. and
- IFM-UMSNH, Michoacan
)
,
Mark Hannam
(
- Jena U.
)
,
Sascha Husa
(
- Jena U.
)
,
Ulrich Sperhake
(
- Jena U.
)

et al.

- Phys.Rev.D 77 (2008) 024027
•
e-Print:
- gr-qc/0610128
•
DOI:
- 10.1103/PhysRevD.77.024027

[15]

Presented at the New Frontiers in Numerical Relativity meeting, Golm

Pollney D. July

[16]

Geometry and regularity of moving punctures

Mark Hannam
(
- Jena U.
)
,
Sascha Husa
(
- Jena U.
)
,
Denis Pollney
(
- Potsdam, Max Planck Inst.
)
,
Bernd Bruegmann
(
- Jena U.
)
,
Niall O'Murchadha
(
- University Coll., Cork
)

- Phys.Rev.Lett. 99 (2007) 241102
•
e-Print:
- gr-qc/0606099
•
DOI:
- 10.1103/PhysRevLett.99.241102

[17]

in L Witten, ed Gravitation: An introduction to current research (New York: John pp 227-265

Arnowitt R
,
Deser S
,
Misner C. W

[18]

Kinematics and Dynamics of General Relativity

James W. York, Jr.
(
- North Carolina U.
)

[19]

First order hyperbolic formalism for numerical relativity

C. Bona
(
- Balearic Islands U.
)
,
J. Masso
(
- Potsdam, Max Planck Inst. and
- NCSA, Urbana
)
,
E. Seidel
(
- Potsdam, Max Planck Inst. and
- NCSA, Urbana and
- Illinois U., Urbana
)
,
J. Stela
(
- Balearic Islands U.
)

- Phys.Rev.D 56 (1997) 3405-3415
•
e-Print:
- gr-qc/9709016
•
DOI:
- 10.1103/PhysRevD.56.3405

[20]

Gauge conditions for long term numerical black hole evolutions without excision

et al.

- Phys.Rev.D 67 (2003) 084023
•
e-Print:
- gr-qc/0206072
•
DOI:
- 10.1103/PhysRevD.67.084023

[21]

Evolution of three-dimensional gravitational waves: Harmonic slicing case

Masaru Shibata
(
- Osaka U.
)
,
Takashi Nakamura
(
- Kyoto U., FIHS
)

- Phys.Rev.D 52 (1995) 5428-5444
•
DOI:
- 10.1103/PhysRevD.52.5428

[22]

On the numerical integration of Einstein's field equations

- Phys.Rev.D 59 (1998) 024007
•
e-Print:
- gr-qc/9810065
•
DOI:
- 10.1103/PhysRevD.59.024007

[23]

Can a combination of the conformal thin sandwich and puncture methods yield binary black hole solutions in quasiequilibrium?

Mark D. Hannam
(
- North Carolina U.
)
,
Charles R. Evans
(
- North Carolina U.
)
,
Gregory B. Cook
(
- Caltech
)
,
Thomas W. Baumgarte
(
- Bowdoin Coll. and
- Illinois U., Urbana
)

- Phys.Rev.D 68 (2003) 064003
•
e-Print:
- gr-qc/0306028
•
DOI:
- 10.1103/PhysRevD.68.064003

[24]

Maximally slicing a black hole

et al.

- Phys.Rev.D 7 (1973) 2814-2817
•
DOI:
- 10.1103/PhysRevD.7.2814

[25]

Analytical representation of a black hole puncture solution

- Phys.Rev.D 75 (2007) 067502
•
e-Print:
- gr-qc/0701037
•
DOI:
- 10.1103/PhysRevD.75.067502

1-25 of 26
1
2
25 / page