English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We quantize a closed homogeneous and isotropic universe in the modifiedteleparallel gravity, wherein a scalar field is non-minimally coupled to boththe torsion and a boundary term. In this regard, we study exact solutions atboth the classical and quantum frameworks by utilizing the correspondingWheeler-DeWitt (WDW) equation of the model. To correspond to the comprehensiveclassical and quantum levels, we propose an appropriate initial condition forthe wave packets and observe that they closely adhere to the classicaltrajectories and reach their peak. We quantify this correspondence using thede-Broglie Bohm interpretation of quantum mechanics. According to thisproposal, the classical and Bohmian trajectories coincide when the quantumpotential vanishes along the Bohmian paths. Furthermore, we apply thede-parameterization technique to our model in the realm of the problem of timein quantum cosmological models based on the WDW equation, utilizing the globalinternal time denoted as $\chi$, which represents a scalar field.

Quantum Cosmology of scalar-tensor teleparallel gravity with a boundary term