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A spinor model for quantum cosmology

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A spinor model for quantum cosmology. / Dereli, Tekin; Önder, M.; Tucker, Robin.
In: Physics Letters B, Vol. 324, No. 2, 31.03.1994, p. 134-140.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Dereli, T, Önder, M & Tucker, R 1994, 'A spinor model for quantum cosmology', Physics Letters B, vol. 324, no. 2, pp. 134-140. https://doi.org/10.1016/0370-2693(94)90399-9

APA

Dereli, T., Önder, M., & Tucker, R. (1994). A spinor model for quantum cosmology. Physics Letters B, 324(2), 134-140. https://doi.org/10.1016/0370-2693(94)90399-9

Vancouver

Dereli T, Önder M, Tucker R. A spinor model for quantum cosmology. Physics Letters B. 1994 Mar 31;324(2):134-140. doi: 10.1016/0370-2693(94)90399-9

Author

Dereli, Tekin ; Önder, M. ; Tucker, Robin. / A spinor model for quantum cosmology. In: Physics Letters B. 1994 ; Vol. 324, No. 2. pp. 134-140.

Bibtex

@article{5091eb901a99466287a382e2f6145a06,
title = "A spinor model for quantum cosmology",
abstract = "The question of the interpretation of Wheeler-DeWitt solutions in the context of cosmological models is addressed by implementing the Hamiltonian constraint as a spinor wave equation in minisuperspace. We offer a relative probability interpretation based on a non-closed vector current in this space and a prescription for a parametrisation of classical solutions in terms of classical time. Such a prescription can accommodate classically degenerate metrics describing manifolds with signature change. The relative probability density, defined in terms of a Killing vector of the DeWitt metric on minisuperspace, should permit one to identify classical loci corresponding to geometries for a classical manifold. This interpretation is illustrated in the context of a quantum cosmology model for two-dimensional dilaton gravity.",
author = "Tekin Dereli and M. {\"O}nder and Robin Tucker",
year = "1994",
month = mar,
day = "31",
doi = "10.1016/0370-2693(94)90399-9",
language = "English",
volume = "324",
pages = "134--140",
journal = "Physics Letters B",
issn = "0370-2693",
publisher = "ELSEVIER SCIENCE BV",
number = "2",

}

RIS

TY - JOUR

T1 - A spinor model for quantum cosmology

AU - Dereli, Tekin

AU - Önder, M.

AU - Tucker, Robin

PY - 1994/3/31

Y1 - 1994/3/31

N2 - The question of the interpretation of Wheeler-DeWitt solutions in the context of cosmological models is addressed by implementing the Hamiltonian constraint as a spinor wave equation in minisuperspace. We offer a relative probability interpretation based on a non-closed vector current in this space and a prescription for a parametrisation of classical solutions in terms of classical time. Such a prescription can accommodate classically degenerate metrics describing manifolds with signature change. The relative probability density, defined in terms of a Killing vector of the DeWitt metric on minisuperspace, should permit one to identify classical loci corresponding to geometries for a classical manifold. This interpretation is illustrated in the context of a quantum cosmology model for two-dimensional dilaton gravity.

AB - The question of the interpretation of Wheeler-DeWitt solutions in the context of cosmological models is addressed by implementing the Hamiltonian constraint as a spinor wave equation in minisuperspace. We offer a relative probability interpretation based on a non-closed vector current in this space and a prescription for a parametrisation of classical solutions in terms of classical time. Such a prescription can accommodate classically degenerate metrics describing manifolds with signature change. The relative probability density, defined in terms of a Killing vector of the DeWitt metric on minisuperspace, should permit one to identify classical loci corresponding to geometries for a classical manifold. This interpretation is illustrated in the context of a quantum cosmology model for two-dimensional dilaton gravity.

U2 - 10.1016/0370-2693(94)90399-9

DO - 10.1016/0370-2693(94)90399-9

M3 - Journal article

VL - 324

SP - 134

EP - 140

JO - Physics Letters B

JF - Physics Letters B

SN - 0370-2693

IS - 2

ER -