Bouncing Cosmology in f(Q) Symmetric Teleparallel Gravity - INSPIRE

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Bouncing Cosmology in f(Q) Symmetric Teleparallel Gravity

Francesco Bajardi
(
- Naples U. and
- INFN, Naples
)
,
Daniele Vernieri
(
- Naples U. and
- INFN, Naples
)
,
Salvatore Capozziello
(
- Naples U. and
- INFN, Naples and
- SSM, Naples and
- Tomsk Pedagogical Inst.
)

Nov 2, 2020

11 pages

Published in:

Eur.Phys.J.Plus 135 (2020) 11, 912

Published: Nov 17, 2020

e-Print:

2011.01248 [gr-qc]

DOI:

10.1140/epjp/s13360-020-00918-3

View in:

ADS Abstract Service

reference search146 citations

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Abstract: (arXiv)

We consider f(Q) extended symmetric teleparallel cosmologies, where Q is the non-metricity scalar, and constrain its functional form through the order reduction method. By using this technique, we are able to reduce and integrate the field equations and thus to select the corresponding models giving rise to bouncing cosmology. The selected Lagrangian is then used to develop the Hamiltonian formalism and to obtain the Wave Function of the Universe which suggests that classical observable universes can be recovered according to the Hartle Criterion.

Note:

11 pages, 1 figure, 68 references

cosmological model: bounce
gravitation: teleparallel
Hamiltonian formalism
field equations: solution
wave function
constraint
gravitation: model
quantum cosmology

References(68)

Figures(1)

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