Constraining fractionality using some observational tests

TL;DR

This paper investigates a fractional-fractal generalization of the Schwarzschild black hole by analyzing observational phenomena such as lensing and orbital precession, and compares predictions with data to assess its viability.

Contribution

It introduces and tests a fractional black hole model against observational data, highlighting its potential and the need for further study of fractional spacetimes.

Findings

Fractional black hole model can fit solar-system observational data

Analysis shows potential of fractional spacetimes in astrophysics

Further research needed for fractional black hole implications

Abstract

Recently, a fractional version of the Schwarzschild-Tangherlini black hole with a fractal horizon has been introduced. Motivated by the key role of the Schwarzschild solution in gravitational and astrophysical studies, some consequences of this fractional-fractal generalization of the Schwarzschild black hole have been investigated. In this line, the corresponding i) Shapiro and Sagnac time delays, ii) shadow, iii) orbital precession, and iv) gravitational lensing are studied and confronted with observational data. MCMC analysis also unveils i) the potential of this metric in dealing with the solar-system tests and ii) the necessity of studying fractional spacetimes and objects.