TY  - JOUR
AU  - Heidari, N.
AU  - Hassanabadi, H.
AU  - Araujo Filho, A. A.
AU  - Kriz, J.
AU  - Zare, S.
AU  - Porfirio, P. J.
PY  - 2024
DA  - 2024//
TI  - Gravitational signatures of a non-commutative stable black hole
T2  - Phys. Dark Universe
JO  - Physics of the Dark Universe
SP  - 101382
EP  - 13pp
VL  - 43
PB  - Elsevier
KW  - Non-commutativity
KW  - Black hole
KW  - Shadows
KW  - Geodesics
AB  - This work investigates several key aspects of a non-commutative theory with mass deformation. We calculate thermodynamic properties of the system and compare our results with recent literature. We examine the quasinormal modes of massless scalar perturbations using two approaches: the WKB approximation and the Poschl-Teller fitting method. Our results indicate that stronger non-commutative parameters lead to slower damping oscillations of gravitational waves and higher partial absorption cross sections. Furthermore, we study the geodesics of massless and massive particles, highlighting that the non-commutative parameter (R) significantly impacts the paths of light and event horizons. Also, we calculate the shadows, which show that larger values of (R) correspond to larger shadow radii, and provide some constraints on (R) applying the observation of Sgr A* from the Event Horizon Telescope. Finally, we explore the deflection angle in this context.
UR  - https://arxiv.org/abs/2305.06838
UR  - https://doi.org/10.1016/j.dark.2023.101382
DO  - 10.1016/j.dark.2023.101382
LA  - English
N1  - WOS:001126934800001
ID  - Heidari_etal2024
ER  -