Zobrazeno 1 - 10
of 46
pro vyhledávání: '"Tonini, E. V."'
We examine the gravitational wave recoil waves and the associated net kick velocities in non-axisymmetric Robinson-Trautman spacetimes. We use characteristic initial data for the dynamics corresponding to non-head-on collisions of black holes. We mak
Externí odkaz:
http://arxiv.org/abs/1407.4405
We examine numerically the gravitational wave recoil in non-axisymmetric Robinson-Trautman spacetimes. We construct characteristic initial data for the Robinson-Trautman dynamics which are interpreted as corresponding to the early post-merger state o
Externí odkaz:
http://arxiv.org/abs/1403.4581
We examine numerically the process of gravitational wave recoil in the merger of two black holes in non head-on collision, in the realm of Robinson-Trautman spacetimes. Characteristic initial data for the system are constructed, and the evolution cov
Externí odkaz:
http://arxiv.org/abs/1202.1271
Publikováno v:
Phys. Rev. D 85, 024003 (2012)
We examine numerically the post-merger regime of two Schwarzschild black holes in non head-on collision. Our treatment is made in the realm of non-axisymmetric Robinson-Trautman spacetimes which are appropriate for the description of the system. Char
Externí odkaz:
http://arxiv.org/abs/1111.1223
Publikováno v:
Int.J.Mod.Phys.D17:2049-2064,2008
We examine the efficiency of gravitational bremsstrahlung production in the process of head-on collision of two boosted Schwarzschild black holes. We constructed initial data for the characteristic initial value problem in Robinson-Trautman spacetime
Externí odkaz:
http://arxiv.org/abs/0804.3610
In this paper we explore one of the most important features of the Galerkin method, which is to achieve high accuracy with a relatively modest computational effort, in the dynamics of Robinson-Trautman spacetimes.
Comment: 7 pages, 5 figures
Comment: 7 pages, 5 figures
Externí odkaz:
http://arxiv.org/abs/gr-qc/0703007
Publikováno v:
Phys.Rev. D65 (2002) 083511
The dynamics of a general Bianchi IX model with three scale factors is examined. The matter content of the model is assumed to be comoving dust plus a positive cosmological constant. The model presents a critical point of saddle-center-center type in
Externí odkaz:
http://arxiv.org/abs/gr-qc/0202047
Publikováno v:
Phys.Rev.D60:121301,1999
We describe a new statistical pattern in the chaotic dynamics of closed inflationary cosmologies, associated with the partition of the Hamiltonian rotational motion energy and hyperbolic motion energy pieces, in a linear neighborhood of the saddle-ce
Externí odkaz:
http://arxiv.org/abs/gr-qc/9909042
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