Gravitational waveforms from periodic orbits around a Schwarzschild black hole embedded in a Dehnen-type dark matter halo

Abstract In this paper, we study the periodic orbits, characterized by zoom-whirl behavior, around a Schwarzschild-like black hole (BH) embedded within a Dehnen-type dark matter (DM) halo. We demonstrate how the DM halo modifies the gravitational dynamics of the black hole, influencing the energy an...

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Main Authors: Mirzabek Alloqulov, Tursunali Xamidov, Sanjar Shaymatov, Bobomurat Ahmedov
Format: Article
Language:English
Published: SpringerOpen 2025-07-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-025-14529-8
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author Mirzabek Alloqulov
Tursunali Xamidov
Sanjar Shaymatov
Bobomurat Ahmedov
author_facet Mirzabek Alloqulov
Tursunali Xamidov
Sanjar Shaymatov
Bobomurat Ahmedov
author_sort Mirzabek Alloqulov
collection DOAJ
description Abstract In this paper, we study the periodic orbits, characterized by zoom-whirl behavior, around a Schwarzschild-like black hole (BH) embedded within a Dehnen-type dark matter (DM) halo. We demonstrate how the DM halo modifies the gravitational dynamics of the black hole, influencing the energy and angular momentum of timelike particle geodesics and enhancing their interaction with the BH. We determine the radii of the marginally bound orbits (MBOs) and innermost stable circular orbits (ISCOs), showing that the DM halo increases both. This provides a deeper understanding of how the DM alters the behavior, energy, and angular momentum of timelike particle geodesics. Furthermore, we explore the gravitational waveforms emitted by a timelike particle in periodic orbits around a supermassive black hole (SMBH) within this BH-DM system. Using a semi-analytical approach, we calculate particle trajectories and derive the corresponding waveforms, demonstrating that the DM halo modifies the zoom-whirl orbital behavior, leading to distinct changes in the waveform structure. Our findings suggest that future gravitational wave (GW) observations could constrain the properties of DM halos surrounding BHs, providing new insights into the gravitational wave signatures arising from the interaction between BH gravity and DM.
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institution Kabale University
issn 1434-6052
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publishDate 2025-07-01
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series European Physical Journal C: Particles and Fields
spelling doaj-art-6347e20ef7c248bfa7946f089af6bb5f2025-08-20T04:02:56ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522025-07-0185711410.1140/epjc/s10052-025-14529-8Gravitational waveforms from periodic orbits around a Schwarzschild black hole embedded in a Dehnen-type dark matter haloMirzabek Alloqulov0Tursunali Xamidov1Sanjar Shaymatov2Bobomurat Ahmedov3School of Physics, Harbin Institute of TechnologyInstitute of Fundamental and Applied Research, National Research University TIIAMEInstitute of Fundamental and Applied Research, National Research University TIIAMESchool of Physics, Harbin Institute of TechnologyAbstract In this paper, we study the periodic orbits, characterized by zoom-whirl behavior, around a Schwarzschild-like black hole (BH) embedded within a Dehnen-type dark matter (DM) halo. We demonstrate how the DM halo modifies the gravitational dynamics of the black hole, influencing the energy and angular momentum of timelike particle geodesics and enhancing their interaction with the BH. We determine the radii of the marginally bound orbits (MBOs) and innermost stable circular orbits (ISCOs), showing that the DM halo increases both. This provides a deeper understanding of how the DM alters the behavior, energy, and angular momentum of timelike particle geodesics. Furthermore, we explore the gravitational waveforms emitted by a timelike particle in periodic orbits around a supermassive black hole (SMBH) within this BH-DM system. Using a semi-analytical approach, we calculate particle trajectories and derive the corresponding waveforms, demonstrating that the DM halo modifies the zoom-whirl orbital behavior, leading to distinct changes in the waveform structure. Our findings suggest that future gravitational wave (GW) observations could constrain the properties of DM halos surrounding BHs, providing new insights into the gravitational wave signatures arising from the interaction between BH gravity and DM.https://doi.org/10.1140/epjc/s10052-025-14529-8
spellingShingle Mirzabek Alloqulov
Tursunali Xamidov
Sanjar Shaymatov
Bobomurat Ahmedov
Gravitational waveforms from periodic orbits around a Schwarzschild black hole embedded in a Dehnen-type dark matter halo
European Physical Journal C: Particles and Fields
title Gravitational waveforms from periodic orbits around a Schwarzschild black hole embedded in a Dehnen-type dark matter halo
title_full Gravitational waveforms from periodic orbits around a Schwarzschild black hole embedded in a Dehnen-type dark matter halo
title_fullStr Gravitational waveforms from periodic orbits around a Schwarzschild black hole embedded in a Dehnen-type dark matter halo
title_full_unstemmed Gravitational waveforms from periodic orbits around a Schwarzschild black hole embedded in a Dehnen-type dark matter halo
title_short Gravitational waveforms from periodic orbits around a Schwarzschild black hole embedded in a Dehnen-type dark matter halo
title_sort gravitational waveforms from periodic orbits around a schwarzschild black hole embedded in a dehnen type dark matter halo
url https://doi.org/10.1140/epjc/s10052-025-14529-8
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AT sanjarshaymatov gravitationalwaveformsfromperiodicorbitsaroundaschwarzschildblackholeembeddedinadehnentypedarkmatterhalo
AT bobomuratahmedov gravitationalwaveformsfromperiodicorbitsaroundaschwarzschildblackholeembeddedinadehnentypedarkmatterhalo