Static dilaton space-time parameters from frequency shifts of photons emitted by geodesic particles
Susana Valdez-Alvarado, Ricardo Becerril, Francisco Astorga

TL;DR
This paper derives the mass parameter of dilaton space-times from the frequency shifts of photons emitted by orbiting particles, providing bounds for observable shifts in specific dilaton metrics.
Contribution
It introduces a method to determine dilaton space-time parameters using photon frequency shifts, focusing on generalized Chatterjee and Gibbons-Maeda metrics.
Findings
Mass parameter expressed via redshift and blueshift.
Bounds on observable frequency shifts for these metrics.
Connection to Schwarzschild black hole in certain limits.
Abstract
The mass parameter of dilaton space-times is obtained as a function of the redshift-blueshift (zred, zblue) of photons emitted by particles orbiting in circular motion around these objects and their corresponding radii. Particularly, we work with the generalized Chatterjee and Gibbons- Maeda space-times. Both of them become the Schwarzschild black hole in certain limit of one of their parameters. Bounds for the values of these frequency shifts, that may be observed for these metrics, are also determined.
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Astrophysics and Cosmic Phenomena
