AdS Black String in a Cosmic Web: Geodesics, Shadows, and Thermodynamics

TL;DR

This paper analyzes how surrounding clouds of strings and quintessence fields affect the properties of AdS black strings, including geodesics, shadows, and thermodynamics, with implications for astronomical observations.

Contribution

It provides a comprehensive analysis of cylindrically symmetric AdS black strings surrounded by clouds of strings and quintessence fields, revealing their effects on geodesic, shadow, and thermodynamic properties.

Findings

CS and QF reduce photon orbit radius and shadow size

Higher CS and QF parameters increase particle energy

C-energy decreases with radius but varies with parameters

Abstract

In a recent article (Ref. \cite{AOP}), the authors obtained a static, cylindrically symmetric Anti-de Sitter (AdS) black string (BS) solutions, which are cylindrical generalizations of black holes (BHs), surrounded by a cloud of strings (CS) and the quintessence field (QF), and discussed its properties. In the present study, we present a comprehensive analysis of cylindrically symmetric AdS BSs surrounded by CS and QF. Our analysis yields several significant results. We demonstrate that the presence of CS (parameter $\alpha$) and QF (parameters $c$ and $w$) reduces the radius of circular photon orbits (CPO) and BH shadow size, with measurements constrained by Event Horizon Telescope (EHT) observations of Sagittarius A*. We find that time-like particle orbits show increased energy with higher $\alpha$ and $c$ values. We calculate that C-energy, representing gravitational energy within cylindrical radius, decreases with radial distance but exhibits distinct responses to CS and QF parameters. We observe that scalar perturbation potential increases $r$ for specific $\alpha$ and $c$ values, indicating stronger field-spacetime interactions away from the BS. We determine that Hawking temperature increases linearly with Schwarzschild radius, with parameter-dependent behavior varying based on QF state parameter $w$. These results demonstrate how CS and QF significantly modify the geodesic, perturbative, and thermodynamic properties of AdS BS, with potential observational implications for gravitational lensing, accretion disk dynamics, and BH evaporation signatures in future astronomical observations.