https://doi.org/10.1140/epjc/s10052-025-14100-5
Regular Article - Theoretical Physics
The constraint on modified black holes with extreme mass ratio inspirals
1
Institute of Fundamental Physics and Quantum Technology, Department of Physics, School of Physical Science and Technology, Ningbo University, 315211, Ningbo, Zhejiang, China
2
School of Physics and Astronomy, Shanghai Jiao Tong University, 800 Dongchuan Rd, 200240, Shanghai, China
Received:
18
December
2024
Accepted:
19
March
2025
Published online:
4
April
2025
The low-energy effective action of String Theory introduces corrections to the dilaton-graviton sector, resulting in deformed black holes beyond general relativity. We analyze extreme mass-ratio inspiral systems (EMRIs), where a stellar-mass object spirals into a slowly rotating supermassive black hole including a distinct deviation parameter. This study examines the effects of this deformation on the rate of change of orbital energy and angular momentum, orbital evolution, and phase dynamics, incorporating leading-order post-Newtonian corrections. The String theory parameter will accelerate the EMRI merger because of the extra energy and angular momentum fluxes carried away by corrections to the dilaton-graviton sector. With 1-year observations of EMRIs, we employ the Fisher information matrix method to evaluate the potential for detecting deviations from general relativity through space-based gravitational wave detectors that utilize time-delay interferometry to suppress laser noise. The constraint on modified black holes,
, is almost the same with and without the time-delay interferometry combination. This analysis enhances our understanding and underscores the crucial role of observations in advancing gravitational phenomena within String Theory.
© The Author(s) 2025
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