Loop Quantum Gravitational Signatures via Love Numbers
Meysam Motaharfar, Parampreet Singh

TL;DR
This paper investigates how loop quantum gravity modifies black hole properties, showing non-zero, negative Love numbers that could serve as observable quantum signatures distinguishing quantum black holes from classical ones.
Contribution
It demonstrates that loop quantum effects induce measurable tidal Love numbers in black holes, providing a potential observational window into quantum gravity.
Findings
Loop quantum black holes have non-zero, negative Love numbers.
Love numbers decrease with increasing black hole mass.
Quantum effects produce detectable 'quantum hair' in black holes.
Abstract
Loop quantum gravitational effects can resolve the central singularity of black holes while potentially leaving tiny traces of quantization in the exterior spacetime. We show the way these residues can, in principle, be explored using tidal Love numbers (TLNs). We consider loop quantized Schwarzschild black hole, in particular the Ashtekar-Olmedo-Singh (AOS) model, and study the static response to external tidal fields of spin zero (scalar field), spin one (vector field), and spin two (axial gravitational field) types. We find that, in contrast to the classical theory, where TLNs vanish, they are non-vanishing and negative for all three responses and for all multipoles. Besides, the magnitude of TLNs decreases as the black hole mass increases, and TLNs, in response to the axial gravitational field, have the largest magnitude among these three responses. Our results show that for black…
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Taxonomy
TopicsQuantum Mechanics and Applications · Noncommutative and Quantum Gravity Theories · Mathematical and Theoretical Analysis
