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Quantum cosmological intertwining: Factor ordering and boundary conditions from hidden symmetries

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arxiv 1507.04212 v1 pith:NKWPGEBJ submitted 2015-07-15 gr-qc math-phmath.MP

classification gr-qcmath-phmath.MP
keywords hiddensymmetriesboundaryconditionscosmologicalquantumbargmannfactor
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abstract

We explore the implications of hidden symmetries present in a particular quantum cosmological setting, extending the results reported in \cite{10,11}. In more detail, our case study is constituted by a spatially closed Friedmann-Lema\^{\i}tre-Robertson-Walker universe, in the presence of a conformally coupled scalar field. The $su(1,1)$ hidden symmetries of this model, together with the Hamiltonian constraint, lead to the gauge invariance of its corresponding Bargmann indices. We subsequently show that some factor-ordering choices can be related to the allowed spectrum of Bargmann indices and hence, to the hidden symmetries. Moreover, the presence of those hidden symmetries also implies a set of appropriate boundary conditions to choose from. In summary, our results suggest that factor ordering and boundary conditions can be intertwined when a quantum cosmological model has hidden symmetries.

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  1. Gauge vs (hidden) physical symmetries of FLRW cosmologies

    gr-qc 2026-07 conditional novelty 6.0 of 10

    For flat FLRW with n free massless scalars, the physical symmetry algebra of the minisuperspace is conf(n,1), and the Schrödinger algebra seen in the Eisenhart-Duval lift is gauge-dependent except for the single-field case.

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