Uniqueness Result

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Norbert Van Den Bergh - One of the best experts on this subject based on the ideXlab platform.

  • petrov type i silent universes with g3 isometry group the Uniqueness Result recovered
    Classical and Quantum Gravity, 2006
    Co-Authors: Lode Wylleman, Norbert Van Den Bergh
    Abstract:

    Irrotational dust spacetimes with vanishing magnetic Weyl curvature are called silent universes (Matarrese et al 1994 Phys. Rev. D 72 320). The silent universe conjecture (Sopuerta 1997 Phys. Rev. D 55 5936, van Elst et al 1997 Class. Quantum Grav. 14 1151) states that the only algebraically general silent universes are the orthogonally spatially homogeneous Bianchi I models. In the same paper by Sopuerta, this was confirmed for the subcase where the spacetime also admits a group G3 of isometries. However, the proof contains a conceptual mistake. We recover the Result in a different way.

  • petrov type i silent universes with g3 isometry group the Uniqueness Result recovered
    arXiv: General Relativity and Quantum Cosmology, 2005
    Co-Authors: Lode Wylleman, Norbert Van Den Bergh
    Abstract:

    The \emph{silent universe conjecture} (Sopuerta 1997, van Elst et al. 1997) states that the only algebraically general silent universes are the orthogonally spatially homogeneous Bianchi I models. In the same paper by Sopuerta this was confirmed for the subcase where the spacetime also admits a group G3 of isometries. However the proof contains a conceptual mistake. We recover the Result in a different way.

Farid Bozorgnia - One of the best experts on this subject based on the ideXlab platform.

Lode Wylleman - One of the best experts on this subject based on the ideXlab platform.

  • petrov type i silent universes with g3 isometry group the Uniqueness Result recovered
    Classical and Quantum Gravity, 2006
    Co-Authors: Lode Wylleman, Norbert Van Den Bergh
    Abstract:

    Irrotational dust spacetimes with vanishing magnetic Weyl curvature are called silent universes (Matarrese et al 1994 Phys. Rev. D 72 320). The silent universe conjecture (Sopuerta 1997 Phys. Rev. D 55 5936, van Elst et al 1997 Class. Quantum Grav. 14 1151) states that the only algebraically general silent universes are the orthogonally spatially homogeneous Bianchi I models. In the same paper by Sopuerta, this was confirmed for the subcase where the spacetime also admits a group G3 of isometries. However, the proof contains a conceptual mistake. We recover the Result in a different way.

  • petrov type i silent universes with g3 isometry group the Uniqueness Result recovered
    arXiv: General Relativity and Quantum Cosmology, 2005
    Co-Authors: Lode Wylleman, Norbert Van Den Bergh
    Abstract:

    The \emph{silent universe conjecture} (Sopuerta 1997, van Elst et al. 1997) states that the only algebraically general silent universes are the orthogonally spatially homogeneous Bianchi I models. In the same paper by Sopuerta this was confirmed for the subcase where the spacetime also admits a group G3 of isometries. However the proof contains a conceptual mistake. We recover the Result in a different way.

Jose M Velhinho - One of the best experts on this subject based on the ideXlab platform.

  • quantum gowdy t3 model a Uniqueness Result
    Classical and Quantum Gravity, 2006
    Co-Authors: Alejandro Corichi, J Cortez, Guillermo Mena A Marugan, Jose M Velhinho
    Abstract:

    Modulo a homogeneous degree of freedom and a global constraint, the linearly polarized Gowdy T 3 cosmologies are equivalent to a free scalar field propagating in a fixed nonstationary background. Recently, a new field parametrization was proposed for the metric of the Gowdy spacetimes such that the associatedscalarfieldevolves in a flat background in (1+1) dimensions with the spatial topology of S 1 , although subject to a time-dependent potential. Introducing a suitable Fock quantization for this scalar field, a quantum theory was constructed for the Gowdy model in which the dynamics is implemented as a unitary transformation. A question that was left open is whether one might adopt a different, nonequivalent Fock representation by selecting a distinct complex structure. The present work proves that the chosen Fock quantization is in fact unique (up to unitary equivalence) if one demands unitary implementation of the dynamics and invariance under the group of S translations. These translations are precisely those generated by the global constraint that remains on the Gowdy model. It is also shown that the proof of Uniqueness in the choice of the complex structure can be applied to more general field dynamics than that corresponding to the Gowdy cosmologies.

  • quantum gowdy t 3 model a Uniqueness Result
    arXiv: General Relativity and Quantum Cosmology, 2006
    Co-Authors: Alejandro Corichi, J Cortez, Guillermo Mena A Marugan, Jose M Velhinho
    Abstract:

    Modulo a homogeneous degree of freedom and a global constraint, the linearly polarised Gowdy $T^3$ cosmologies are equivalent to a free scalar field propagating in a fixed nonstationary background. Recently, a new field parameterisation was proposed for the metric of the Gowdy spacetimes such that the associated scalar field evolves in a flat background in 1+1 dimensions with the spatial topology of $S^1$, although subject to a time dependent potential. Introducing a suitable Fock quantisation for this scalar field, a quantum theory was constructed for the Gowdy model in which the dynamics is implemented as a unitary transformation. A question that was left open is whether one might adopt a different, nonequivalent Fock representation by selecting a distinct complex structure. The present work proves that the chosen Fock quantisation is in fact unique (up to unitary equivalence) if one demands unitary implementation of the dynamics and invariance under the group of constant $S^1$ translations. These translations are precisely those generated by the global constraint that remains on the Gowdy model. It is also shown that the proof of Uniqueness in the choice of complex structure can be applied to more general field dynamics than that corresponding to the Gowdy cosmologies.

Alejandro Corichi - One of the best experts on this subject based on the ideXlab platform.

  • quantum gowdy t3 model a Uniqueness Result
    Classical and Quantum Gravity, 2006
    Co-Authors: Alejandro Corichi, J Cortez, Guillermo Mena A Marugan, Jose M Velhinho
    Abstract:

    Modulo a homogeneous degree of freedom and a global constraint, the linearly polarized Gowdy T 3 cosmologies are equivalent to a free scalar field propagating in a fixed nonstationary background. Recently, a new field parametrization was proposed for the metric of the Gowdy spacetimes such that the associatedscalarfieldevolves in a flat background in (1+1) dimensions with the spatial topology of S 1 , although subject to a time-dependent potential. Introducing a suitable Fock quantization for this scalar field, a quantum theory was constructed for the Gowdy model in which the dynamics is implemented as a unitary transformation. A question that was left open is whether one might adopt a different, nonequivalent Fock representation by selecting a distinct complex structure. The present work proves that the chosen Fock quantization is in fact unique (up to unitary equivalence) if one demands unitary implementation of the dynamics and invariance under the group of S translations. These translations are precisely those generated by the global constraint that remains on the Gowdy model. It is also shown that the proof of Uniqueness in the choice of the complex structure can be applied to more general field dynamics than that corresponding to the Gowdy cosmologies.

  • quantum gowdy t 3 model a Uniqueness Result
    arXiv: General Relativity and Quantum Cosmology, 2006
    Co-Authors: Alejandro Corichi, J Cortez, Guillermo Mena A Marugan, Jose M Velhinho
    Abstract:

    Modulo a homogeneous degree of freedom and a global constraint, the linearly polarised Gowdy $T^3$ cosmologies are equivalent to a free scalar field propagating in a fixed nonstationary background. Recently, a new field parameterisation was proposed for the metric of the Gowdy spacetimes such that the associated scalar field evolves in a flat background in 1+1 dimensions with the spatial topology of $S^1$, although subject to a time dependent potential. Introducing a suitable Fock quantisation for this scalar field, a quantum theory was constructed for the Gowdy model in which the dynamics is implemented as a unitary transformation. A question that was left open is whether one might adopt a different, nonequivalent Fock representation by selecting a distinct complex structure. The present work proves that the chosen Fock quantisation is in fact unique (up to unitary equivalence) if one demands unitary implementation of the dynamics and invariance under the group of constant $S^1$ translations. These translations are precisely those generated by the global constraint that remains on the Gowdy model. It is also shown that the proof of Uniqueness in the choice of complex structure can be applied to more general field dynamics than that corresponding to the Gowdy cosmologies.