Authors: Mario Prebježić
We derive quantum corrections to the temporal potential ^ within an effective field theory (EFT) framework and analyze their observational implications using neutron star data. By incorporating one-loop corrections to the metric component , we compute modifications to the gravitational redshift and perform a Bayesian analysis of NICER and XMM-Newton observations of PSR J0740+6620. Our results show that quantum corrections remain negligible (^∼10−38) under EFT assumptions, but systematic discrepancies in observed redshifts suggest the need for beyond-EFT physics. This study provides a methodology for future high-precision tests of quantum gravity effects using next-generation space telescopes.
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