We present Asymmetric Bounce-Loop Theory (ABLT), a novel theoretical framework in cyclic cosmology that resolves classical gravitational singularities, information destruction, and thermodynamic entropy degradation across successive cosmic cycles. By integrating Loop Quantum Cosmology (LQC) holonomy corrections with an asymmetric Eddington-Finkelstein metric inversion, we demonstrate how a collapsing universe transitions through a Planck-density quantum bounce into an expanding white-hole phase without encountering a physical singularity. Furthermore, we establish the thermodynamic mechanism by which metric expansion and spatial dilution reset local entropy density relative to the comoving volume, resolving Tolman’s entropy paradox. Observational signatures in the cosmic microwave background (CMB) non-Gaussianity and primordial gravitational wave power spectra are proposed as empirical tests for the ABLT framework.
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Aditya Vikram Gupta (2026) studied this question.
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