Testing low energy string theory with strong gravitational lensing by black holes and constraints from EHT observations

IF 5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Physics of the Dark Universe Pub Date : 2025-02-01 DOI:10.1016/j.dark.2024.101768
Amna Ali , Shafqat Ul Islam , Sushant G. Ghosh , Ammuthavali Ramasamya
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Abstract

We explore strong-gravitational lensing by spherically symmetric Dyon black holes, characterized by the parameters λ and β, which are releated to the electric and magnetic charges within low-energy string theory. Our study reveals that as the values of λ and β increase, there is a decrease in the photon sphere radius (xm), the critical impact parameter (um), and the angular position (θ). Additionally, the flux ratio (rmag) of the first image to all other images decreases with increasing λ and β. In contrast to Schwarzschild black holes (where λ and β approach 0), these Dyon black holes show a smaller deflection angle (αD), which further decreases as λ and β increase. Furthermore, the time delay for black holes such as Sgr A* and M87* can reach up to approximately 10.011 and 15133.1 min, respectively, deviating from Schwarzschild black holes by about 1.4858 and 2245.8 min. For Sgr A* and M87*, the angular position (θ) is found to be within the range of (13.07–26.50) μas and (10.11–20.51) μas, respectively, with angular separations (s) ranging from (0.017–0.406) μas for Sgr A* and (0.013–0.314) μas for M87*. The Event Horizon Telescope (EHT) constraints on θsh for Sgr A* and M87* within the 1σ region limit the parameters λ and β such that the allowed values of β depend on the parameter λ. For Sgr A* 0.184M2<β<0.508M2 and 0<β<0.138M2 for M87* when λ=0.4M. Our results imply that Dyon black holes, inspired by low-energy string theory, match EHT observations within a specific parameter space, indicating that these black holes could be convincing candidates for astrophysical black holes. We also estimate the parameters λ and β for string-inspired Dyon black holes using EHT observation results for Sgr A* and M87*.
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Physics of the Dark Universe
Physics of the Dark Universe ASTRONOMY & ASTROPHYSICS-
CiteScore
9.60
自引率
7.30%
发文量
118
审稿时长
61 days
期刊介绍: Physics of the Dark Universe is an innovative online-only journal that offers rapid publication of peer-reviewed, original research articles considered of high scientific impact. The journal is focused on the understanding of Dark Matter, Dark Energy, Early Universe, gravitational waves and neutrinos, covering all theoretical, experimental and phenomenological aspects.
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