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Gravitational waves for eccentric extreme mass ratio inspirals of self-dual spacetime

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arxiv 2404.08454 v1 pith:NYDBAEMS submitted 2024-04-12 gr-qc astro-ph.HE

Yunlong Liu , Xiangdong Zhang This is my paper · ORCID
classification gr-qcastro-ph.HE
keywords eccentricextremefluxgravitationalimprovedinspiralsloopmass
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abstract

In this paper, we calculate the frequencies of geodesic orbits in self-dual spacetime on the equatorial plane and obtain the leading-order effects of loop quantum parameters $P$ on the energy flux and angular momentum flux in eccentric extreme mass ratio inspirals. The gravitational waveform under different eccentricity is carried out by improved "analytic-kludge" method. Through the calculation of waveform mismatches for the LISA detector, the constraints on loop quantum parameters will be improved by 1 to 2 orders of magnitude, compared to the weak field experiments in the solar system, and can reach the level of $10^{-8}$.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Constraining polymerized black holes with quasi-circular extreme mass-ratio inspirals

    gr-qc 2024-12 conditional novelty 6.0 of 10

    A future LISA observation of an extreme-mass-ratio inspiral around a polymerized black hole could constrain the quantum parameter k-hat to about 0.003, roughly two orders of magnitude tighter than current black hole s...

  2. Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves

    gr-qc 2025-06 conditional novelty 4.0 of 10

    Gravitational-wave strains from analytic-kludge EMRI models can distinguish scale-dependent Planck stars from renormalization-group improved Schwarzschild black holes, at least for the chosen orbit parameters.

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