Charged-scalar vacuum polarization makes photon paths timelike and yields frequency-dependent Sachs-Wolfe corrections, giving a CMB mu-distortion and power-spectrum modifications whose size depends on the scalar mass and coupling.
Geometry and Motion in General Relativity
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
A classic problem in general relativity, long studied by both physicists and philosophers of physics, concerns whether the geodesic principle may be derived from other principles of the theory, or must be posited independently. In a recent paper [Geroch & Weatherall, "The Motion of Small Bodies in Space-Time", Comm. Math. Phys. (forthcoming)], Bob Geroch and I have introduced a new approach to this problem, based on a notion we call "tracking". In the present paper, I situate the main results of that paper with respect to two other, related approaches, and then make some preliminary remarks on the interpretational significance of the new approach. My main suggestion is that "tracking" provides the resources for eliminating "point particles"---a problematic notion in general relativity---from the geodesic principle altogether.
citation-role summary
citation-polarity summary
fields
astro-ph.CO 1years
2025 1verdicts
CONDITIONAL 1roles
background 1polarities
unclear 1representative citing papers
citing papers explorer
-
Vacuum Polarization, Geodesic Equation and Sachs-Wolfe Effect
Charged-scalar vacuum polarization makes photon paths timelike and yields frequency-dependent Sachs-Wolfe corrections, giving a CMB mu-distortion and power-spectrum modifications whose size depends on the scalar mass and coupling.