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QUANTUM COSMOLOGY OF MULTIFIELD SCALAR MATTER: SOME EXACT SOLUTIONS. / Andrianov, A.A.; Novikov, O.O.; Chen, L.

в: Theoretical and Mathematical Physics, Том 184, № 3, 2015, стр. 1224-1233.

Результаты исследований: Научные публикации в периодических изданиях › статья

Harvard

Andrianov, AA, Novikov, OO & Chen, L 2015, 'QUANTUM COSMOLOGY OF MULTIFIELD SCALAR MATTER: SOME EXACT SOLUTIONS', Theoretical and Mathematical Physics, Том. 184, № 3, стр. 1224-1233. https://doi.org/10.1007/s11232-015-0328-5

APA

Andrianov, A. A., Novikov, O. O., & Chen, L. (2015). QUANTUM COSMOLOGY OF MULTIFIELD SCALAR MATTER: SOME EXACT SOLUTIONS. Theoretical and Mathematical Physics, 184(3), 1224-1233. https://doi.org/10.1007/s11232-015-0328-5

Vancouver

Andrianov AA, Novikov OO, Chen L. QUANTUM COSMOLOGY OF MULTIFIELD SCALAR MATTER: SOME EXACT SOLUTIONS. Theoretical and Mathematical Physics. 2015;184(3):1224-1233. https://doi.org/10.1007/s11232-015-0328-5

Author

Andrianov, A.A. ; Novikov, O.O. ; Chen, L. / QUANTUM COSMOLOGY OF MULTIFIELD SCALAR MATTER: SOME EXACT SOLUTIONS. в: Theoretical and Mathematical Physics. 2015 ; Том 184, № 3. стр. 1224-1233.

BibTeX

@article{fc0e6ef62c2b453db8dfe9f6df80a0e0,
title = "QUANTUM COSMOLOGY OF MULTIFIELD SCALAR MATTER: SOME EXACT SOLUTIONS",
abstract = "We consider gravity interacting with matter scalar fields and quantized in the superspace approach in which the wave functional is described by the Wheeler–DeWitt equations. Assuming the dominance of the homogeneous and isotropic geometry, we investigate the leading contribution to the wave functional in the minisuperspace approximation with the Friedmann–Robertson–Walker metric and scalar fields depending on the time parameter. We construct a model of several scalar fields with exponential potentials and kinetic terms admitting a special mixing such that it is ultimately possible to separate the variables in the Wheeler–DeWitt equation and find its exact solution in terms of special functions. We study the semiclassical approximation in detail and choose boundary conditions that allow selecting the physical solution selection for classical cosmologies.",
keywords = "quantum cosmology, Wheeler–DeWitt equation, minisuperspace, exponential potential",
author = "A.A. Andrianov and O.O. Novikov and L. Chen",
year = "2015",
doi = "10.1007/s11232-015-0328-5",
language = "English",
volume = "184",
pages = "1224--1233",
journal = "Theoretical and Mathematical Physics (Russian Federation)",
issn = "0040-5779",
publisher = "Springer Nature",
number = "3",

}

RIS

TY - JOUR

T1 - QUANTUM COSMOLOGY OF MULTIFIELD SCALAR MATTER: SOME EXACT SOLUTIONS

AU - Andrianov, A.A.

AU - Novikov, O.O.

AU - Chen, L.

PY - 2015

Y1 - 2015

N2 - We consider gravity interacting with matter scalar fields and quantized in the superspace approach in which the wave functional is described by the Wheeler–DeWitt equations. Assuming the dominance of the homogeneous and isotropic geometry, we investigate the leading contribution to the wave functional in the minisuperspace approximation with the Friedmann–Robertson–Walker metric and scalar fields depending on the time parameter. We construct a model of several scalar fields with exponential potentials and kinetic terms admitting a special mixing such that it is ultimately possible to separate the variables in the Wheeler–DeWitt equation and find its exact solution in terms of special functions. We study the semiclassical approximation in detail and choose boundary conditions that allow selecting the physical solution selection for classical cosmologies.

AB - We consider gravity interacting with matter scalar fields and quantized in the superspace approach in which the wave functional is described by the Wheeler–DeWitt equations. Assuming the dominance of the homogeneous and isotropic geometry, we investigate the leading contribution to the wave functional in the minisuperspace approximation with the Friedmann–Robertson–Walker metric and scalar fields depending on the time parameter. We construct a model of several scalar fields with exponential potentials and kinetic terms admitting a special mixing such that it is ultimately possible to separate the variables in the Wheeler–DeWitt equation and find its exact solution in terms of special functions. We study the semiclassical approximation in detail and choose boundary conditions that allow selecting the physical solution selection for classical cosmologies.

KW - quantum cosmology

KW - Wheeler–DeWitt equation

KW - minisuperspace

KW - exponential potential

U2 - 10.1007/s11232-015-0328-5

DO - 10.1007/s11232-015-0328-5

M3 - Article

VL - 184

SP - 1224

EP - 1233

JO - Theoretical and Mathematical Physics (Russian Federation)

JF - Theoretical and Mathematical Physics (Russian Federation)

SN - 0040-5779

IS - 3

ER -

ID: 3961215