Quantum Gravity signatures in late time Universe
Ankit Dhanuka, Kinjalk Lochan

TL;DR
This paper shows that quantum gravitational effects, usually considered negligible after the early universe, can cause observable phenomena in the late universe, especially after the Last Scattering Surface, due to diverging quantum graviton correlators in matter-dominated eras.
Contribution
It demonstrates that quantum gravitons have significant observable effects in the late universe, challenging the assumption that quantum gravity effects fade after the early universe.
Findings
Quantum graviton correlators grow divergently in matter-dominated era.
Post-LSS atoms can be excited by graviton vacuum fluctuations.
Quantum processes influence late-time cosmological evolution.
Abstract
In the cosmological settings, Quantum Gravity effects are typically understood to be limited towards very early phase of the universe, namely in the pre-inflationary era, with limited signatures spilling over into the succeeding inflationary era which gradually fade away as the universe transits into the subsequent radiation and matter driven expansion. In general scenarios as well, the imprints of possible quantum character of gravitons are typically so feeble that they are expected to remain buried under overwhelming noise from other stronger processes. In this work, we demonstrate that quantized gravitational perturbations cause strong observable effects in cosmological settings post the Last Scattering Surface (LSS) more prominently than any other classical or quantum processes. This counter-intuitive effect is facilitated by the fact that the quantum correlators of the gravitons…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Geophysics and Gravity Measurements
