Electromagnetic Waves in Cosmological Space-Time II. Luminosity Distance
Denitsa Staicova, Michail Stoilov

TL;DR
This paper derives explicit solutions for electromagnetic wave propagation in expanding cosmological spacetime, revealing potential modifications to luminosity distance calculations and implications for cosmological parameters, fitting supernova data without a cosmological constant.
Contribution
It provides explicit solutions for electromagnetic waves in expanding spacetime, offering an alternative to geometric optics and null geodesics in cosmological models.
Findings
Alternative model fits supernova data without cosmological constant
Proposes modifications to standard luminosity distance formula
Suggests a universe with stiff or ultra-stiff matter instead of dark energy
Abstract
In this article, we continue our investigation on how the electromagnetic waves propagate in the Friedman-Lemaitre-Robertson-Walker spacetime. Unlike the standard approach, which relies on null geodesics and geometric optics approximation, we derive explicit solutions for electromagnetic waves in expanding spacetime and examine their implications for cosmological observations. In particular, our analysis reveals potential modifications to the standard luminosity distance formula. Its effect on other cosmological parameters, e.g., the amount of cold dust matter in the Universe, is considered and estimated from Type Ia supernovae data. We see that this alternative model is able to fit the supernova data, but it gives a qualitatively different Universe without a cosmological constant but with stiff or ultra-stiff matter.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
