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Extreme mass-ratio inspirals as probes of scalar fields: inclined circular orbits around Kerr black holes

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arxiv 2401.09542 v1 pith:UO6DKZKF submitted 2024-01-17 gr-qc

Extreme mass-ratio inspirals as probes of scalar fields: inclined circular orbits around Kerr black holes

classification gr-qc
keywords scalarorbitsextremefieldfieldsinclinedinspiralslisa
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Extreme mass-ratio inspirals, a target source for the space-based gravitational wave detector LISA, are a sensitive probe of fundamental scalar fields coupled to gravity. We assess the capability of LISA to detect whether the secondary compact object is endowed with a scalar field, in the case of inclined orbits. We show that the imprint of the scalar field depends on the orbital inclination, and is significantly larger for prograde orbits.

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Forward citations

Cited by 3 Pith papers

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

  1. The significance of first post-adiabatic contributions for scalar charge measurements with intermediate and extreme mass ratio inspirals

    gr-qc 2026-07 accept novelty 6.5

    Neglecting 1PA gravitational self-force biases intrinsic EMRI parameters while scalar-charge inference remains robust; pure-GR templates produce large biases and underestimated errors on charged signals.

  2. Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals

    gr-qc 2026-06 unverdicted novelty 5.0

    Computes scalar and tensor fluxes for eccentric EMRIs with massive scalars, quantifies dephasing, and shows via Fisher matrix that LISA can constrain scalar charge and mass.

  3. Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals

    gr-qc 2026-04 unverdicted novelty 5.0

    LISA EMRIs can constrain deviations from Kerr equatorial symmetry to 10^{-2} and axial symmetry to 10^{-3} using Analytic Kludge waveforms and Fisher analysis.