Plummer Dark Matter Black Hole with Topological Defects: Shadow, Greybody Factors, Quasinormal Modes, and Thermodynamics
Ahmad Al-Badawi, Faizuddin Ahmed, and \.Izzet Sakall{\i}

TL;DR
This paper constructs a black hole model embedded in a dark matter halo and a cloud of strings, analyzing its shadow, perturbations, and thermodynamics, revealing the dominant role of string tension in observable modifications.
Contribution
It introduces a novel black hole solution incorporating a Plummer dark matter halo and a string cloud, and systematically studies its optical, perturbative, and thermodynamic properties.
Findings
The black hole admits a single event horizon for certain parameters.
The string tension parameter significantly influences all observable features.
The heat capacity is always negative, indicating no phase transitions.
Abstract
We construct a static, spherically symmetric black hole (BH) solution embedded in a cored Plummer dark matter (DM) halo and a Letelier cloud of strings (CoS). Starting from the Plummer-Schwarzschild metric of Senjaya et al.~\cite{Senjaya2026}, we incorporate the string-cloud tension parameter into the lapse function, obtaining . The resulting spacetime admits a single, non-degenerate event horizon (EH) for and a naked singularity for . We determine the photon sphere (PS) and BH shadow radii, compute the weak deflection angle via the Gauss-Bonnet theorem (GBT), and analyze the innermost stable circular orbit (ISCO). Scalar perturbations are studied through the effective potential, greybody factor (GF) bounds obtained from the Boonserm-Visser method, the Hawking emission spectrum, and quasinormal mode (QNM)…
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