Dynamics of spinning particles around the loop quantum black hole

In this work, we investigated the motion of spinning test particles in the spacetime of a Loop Quantum Black Hole. The dynamics of the spinning particles were formulated using the Mathisson–Papapetrou–Dixon equations, from which the effective potential was derived and analyzed with respect to the parameters of the LQBH metric. We examined how the particle’s spin influences the innermost stable circular orbit, as well as the corresponding specific angular momentum and energy, for various values of the black hole parameters. In addition, we determined the critical spin parameter s , beyond which time-like trajectories transition to non-physical, space-like motion, and analyzed its dependence on the deformation parameters α and β . Finally, we studied the center-of-mass energy resulting from the collision of two spinning particles near the event horizon, highlighting how spin and quantum corrections jointly affect high-energy processes in Loop Quantum Black Hole spacetimes.

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Publication Details

Journal
Nuclear Physics B
Published
2026-02-14
DOI
https://doi.org/10.1016/j.nuclphysb.2026.117353
Primary Topic
Noncommutative and Quantum Gravity Theories
Type
article
Field-Weighted Citation Impact
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article

Dynamics of spinning particles around the loop quantum black hole

Ahmadjon Abdujabbarov, Gulnisa Abdukayumova, G. Mustafa, Phongpichit Channuie et al.
Nuclear Physics B
Noncommutative and Quantum Gravity Theories
article

Dynamics of spinning particles around the loop quantum black hole

Ahmadjon Abdujabbarov, Gulnisa Abdukayumova, G. Mustafa, Phongpichit Channuie, Farruh Atamurotov
article en

Abstract

In this work, we investigated the motion of spinning test particles in the spacetime of a Loop Quantum Black Hole. The dynamics of the spinning particles were formulated using the Mathisson–Papapetrou–Dixon equations, from which the effective potential was derived and analyzed with respect to the parameters of the LQBH metric. We examined how the particle’s spin influences the innermost stable circular orbit, as well as the corresponding specific angular momentum and energy, for various values of the black hole parameters. In addition, we determined the critical spin parameter s , beyond which time-like trajectories transition to non-physical, space-like motion, and analyzed its dependence on the deformation parameters α and β . Finally, we studied the center-of-mass energy resulting from the collision of two spinning particles near the event horizon, highlighting how spin and quantum corrections jointly affect high-energy processes in Loop Quantum Black Hole spacetimes.

Nuclear Physics BVol. 1024
Khazar University (AZ), Zhejiang Normal University (CN), Urgench State University (UZ), Harbin Institute of Technology (CN), Tashkent State Technical University named after Islam Karimov (UZ), Tashkent Institute of Irrigation and Agricultural Mechanization Engineers (UZ), Westminster International University in Tashkent (UZ), Walailak University (TH)
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Openalex Percentile: Top 53%
Noncommutative and Quantum Gravity Theories
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