Geodesics and scalar perturbations of Schwarzschild black holes embedded in a Dehnen-type dark matter halo with quintessence
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F62690094%3A18470%2F25%3A50022986" target="_blank" >RIV/62690094:18470/25:50022986 - isvavai.cz</a>
Výsledek na webu
<a href="http://dx.doi.org/10.1088/1402-4896/ae0ed7" target="_blank" >http://dx.doi.org/10.1088/1402-4896/ae0ed7</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/1402-4896/ae0ed7" target="_blank" >10.1088/1402-4896/ae0ed7</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Geodesics and scalar perturbations of Schwarzschild black holes embedded in a Dehnen-type dark matter halo with quintessence
Popis výsledku v původním jazyce
We present a comprehensive analysis of a Schwarzschild black hole embedded in a Dehnen-type dark-matter halo and surrounded by a quintessence field. We construct the composite spacetime metric and analyze its geometric properties, including horizon structure and curvature invariants. We find that increasing both the dark-matter core density rho s and the quintessence normalization parameter c enlarges the event horizon while reducing the cosmological horizon. We analyze timelike and null geodesics to determine the innermost stable circular orbits, photon-sphere radii, and shadow properties. Using the Gauss-Bonnet theorem, we compute weak-deflection angles and demonstrate that gravitational lensing intensifies as rho s and rs increase. Scalar perturbations are examined using the sixth-order WKB method and Pad & eacute; approximants, supported by time-domain checks. We observe that the quasinormal modes are suppressed as the dark-matter density increases. Greybody factors and the sparsity of Hawking radiation are also computed, revealing that increased halo density enhances transmission and modifies their deviation from blackbody emission. Our results highlight the observable signatures of dark matter and quintessence in black-hole phenomenology, with testable implications for Event Horizon Telescope imaging and gravitational-wave spectroscopy.
Název v anglickém jazyce
Geodesics and scalar perturbations of Schwarzschild black holes embedded in a Dehnen-type dark matter halo with quintessence
Popis výsledku anglicky
We present a comprehensive analysis of a Schwarzschild black hole embedded in a Dehnen-type dark-matter halo and surrounded by a quintessence field. We construct the composite spacetime metric and analyze its geometric properties, including horizon structure and curvature invariants. We find that increasing both the dark-matter core density rho s and the quintessence normalization parameter c enlarges the event horizon while reducing the cosmological horizon. We analyze timelike and null geodesics to determine the innermost stable circular orbits, photon-sphere radii, and shadow properties. Using the Gauss-Bonnet theorem, we compute weak-deflection angles and demonstrate that gravitational lensing intensifies as rho s and rs increase. Scalar perturbations are examined using the sixth-order WKB method and Pad & eacute; approximants, supported by time-domain checks. We observe that the quasinormal modes are suppressed as the dark-matter density increases. Greybody factors and the sparsity of Hawking radiation are also computed, revealing that increased halo density enhances transmission and modifies their deviation from blackbody emission. Our results highlight the observable signatures of dark matter and quintessence in black-hole phenomenology, with testable implications for Event Horizon Telescope imaging and gravitational-wave spectroscopy.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10303 - Particles and field physics
Návaznosti výsledku
Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2025
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Physica scripta
ISSN
0031-8949
e-ISSN
1402-4896
Svazek periodika
100
Číslo periodika v rámci svazku
10
Stát vydavatele periodika
GB - Spojené království Velké Británie a Severního Irska
Počet stran výsledku
22
Strana od-do
"Article number: 105008"
Kód UT WoS článku
001592108600001
EID výsledku v databázi Scopus
2-s2.0-105018858312