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6
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85033963465
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See also, Ref. 2
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For example, http://lisa.jpl.nasa.gov/. See also, Ref. 2).
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7
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0003447159
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ed. J.-P. Lasota and J.-A. Marck Cambridge University Press, Cambridge, see also references cited therein
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For example, L. Blanchet, in Relativistic gravitation and gravitational radiation, ed. J.-P. Lasota and J.-A. Marck (Cambridge University Press, Cambridge, 1997), see also references cited therein.
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(1997)
Relativistic Gravitation and Gravitational Radiation
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Blanchet, L.1
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8
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0001085269
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ed. J.-P. Lasota and J.-A. Marck Cambridge University Press, Cambridge
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For example, see K. Oohara and T. Nakamura, in Relativistic gravitation and gravitational radiation, ed. J.-P. Lasota and J.-A. Marck (Cambridge University Press, Cambridge, 1997), p. 309. As for a USA project, see, http://www.npac.syr.edu/projects/bh.
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(1997)
Relativistic Gravitation and Gravitational Radiation
, pp. 309
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Oohara, K.1
Nakamura, T.2
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15
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0000000886
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For example, M. Shibata, Phys. Rev. D55 (1997), 6019. M. Shibata, K. Oohara and T. Nakamura, Prog. Theor. Phys. 98 (1997), 1081. M. Shibata, T. W. Baumgarte and S. L. Shapiro, Phys. Rev. D58 (1998), 023002.
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(1997)
Phys. Rev.
, vol.D55
, pp. 6019
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Shibata, M.1
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16
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0031322483
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For example, M. Shibata, Phys. Rev. D55 (1997), 6019. M. Shibata, K. Oohara and T. Nakamura, Prog. Theor. Phys. 98 (1997), 1081. M. Shibata, T. W. Baumgarte and S. L. Shapiro, Phys. Rev. D58 (1998), 023002.
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(1997)
Prog. Theor. Phys.
, vol.98
, pp. 1081
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Shibata, M.1
Oohara, K.2
Nakamura, T.3
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17
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0001968284
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For example, M. Shibata, Phys. Rev. D55 (1997), 6019. M. Shibata, K. Oohara and T. Nakamura, Prog. Theor. Phys. 98 (1997), 1081. M. Shibata, T. W. Baumgarte and S. L. Shapiro, Phys. Rev. D58 (1998), 023002.
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(1998)
Phys. Rev.
, vol.D58
, pp. 023002
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Shibata, M.1
Baumgarte, T.W.2
Shapiro, S.L.3
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18
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85033965900
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note
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i are actually the second and first post-Newtonian order. This fact can be found by performing a post-Newtonian analysis in the (3+1) formalism as we have done in the next reference 17).
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20
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0002051709
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The Moncrief variables are defined in a Schwarzschild spacetime. In this paper, we use them by simply setting the gravitational mass to be zero in order to consider the gauge invariant quantities in the flat spacetime
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V. Moncrief, Ann. of Phys. 88 (1974), 323. The Moncrief variables are defined in a Schwarzschild spacetime. In this paper, we use them by simply setting the gravitational mass to be zero in order to consider the gauge invariant quantities in the flat spacetime.
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(1974)
Ann. of Phys.
, vol.88
, pp. 323
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Moncrief, V.1
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21
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0003513781
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New York, Wiley, chapter 16
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For example, S. L. Shapiro and S. A. Teukolsky, Black Holes, White Dwarfs, and Neutron Stars (New York, Wiley, 1983), chapter 16.
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(1983)
Black Holes, White Dwarfs, and Neutron Stars
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Shapiro, S.L.1
Teukolsky, S.A.2
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22
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4243561411
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This feature has been already found by the following authors in a semi-analytical study of the Oppenheimer-Snyder collapse in the MD gauge and maximal slice conditions. L. I. Petrich, S. L. Shapiro and S. A. Teukolsky, Phys. Rev. D31 (1985), 2459, see Fig. 2 in this paper.
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(1985)
Phys. Rev.
, vol.D31
, pp. 2459
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Petrich, L.I.1
Shapiro, S.L.2
Teukolsky, S.A.3
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24
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85033963199
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in preparation
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M. Shibata, in preparation.
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Shibata, M.1
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