Single-harmonic search for extreme mass-ratio inspirals

Extreme mass-ratio inspirals (EMRIs) are one of the key sources of gravitational waves for space-based detectors such as LISA. However, their detection remains a major data analysis challenge due to the signals' complexity and length. We present a semi-coherent, time-frequency search strategy for detecting EMRI harmonics without relying on full waveform templates. We perform an injection and search campaign of single mildly-eccentric equatorial EMRIs in stationary Gaussian noise. The detection statistic is constructed solely from the EMRI frequency evolution, which is modeled phenomenologically using a Singular Value Decomposition basis. The pipeline and the detection statistic are implemented in time-frequency, enabling efficient searches over one year of data in approximately one hour on a single GPU. The search pipeline achieves 94% detection probability at $\mathrm{SNR} = 30$ for a false-alarm probability of $10^{-2}$, recovering the frequency evolution of the dominant harmonic to 1% relative error. By mapping the EMRI parameters consistent with the recovered frequency evolution, we show that the semi-coherent detection statistic enables a sub-percent precision estimation of the EMRI intrinsic parameters. These results establish a computationally efficient framework for constructing EMRI proposals for the LISA global fit.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2026-01-05
DOI
https://doi.org/10.1103/dh3j-ksfl
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
0.00
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article

Single-harmonic search for extreme mass-ratio inspirals

Christian E. A. Chapman-Bird, Lorenzo Speri, Davide Gerosa, R. Tenorio
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
article

Single-harmonic search for extreme mass-ratio inspirals

Christian E. A. Chapman-Bird, Lorenzo Speri, Davide Gerosa, R. Tenorio
article en

Abstract

Extreme mass-ratio inspirals (EMRIs) are one of the key sources of gravitational waves for space-based detectors such as LISA. However, their detection remains a major data analysis challenge due to the signals' complexity and length. We present a semi-coherent, time-frequency search strategy for detecting EMRI harmonics without relying on full waveform templates. We perform an injection and search campaign of single mildly-eccentric equatorial EMRIs in stationary Gaussian noise. The detection statistic is constructed solely from the EMRI frequency evolution, which is modeled phenomenologically using a Singular Value Decomposition basis. The pipeline and the detection statistic are implemented in time-frequency, enabling efficient searches over one year of data in approximately one hour on a single GPU. The search pipeline achieves 94% detection probability at $\mathrm{SNR} = 30$ for a false-alarm probability of $10^{-2}$, recovering the frequency evolution of the dominant harmonic to 1% relative error. By mapping the EMRI parameters consistent with the recovered frequency evolution, we show that the semi-coherent detection statistic enables a sub-percent precision estimation of the EMRI intrinsic parameters. These results establish a computationally efficient framework for constructing EMRI proposals for the LISA global fit.

Physical review. D/Physical review. D.Vol. 113(2)
Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca (IT), European Space Research and Technology Centre (NL), University of Milano-Bicocca (IT), University of Birmingham (GB)
Openalex Percentile: Top 98%
Pulsars and Gravitational Waves Research
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Single-harmonic search for extreme mass-ratio inspirals — Christian E. A. Chapman-Bird, Lorenzo Speri, et al. · Physical review. D/Physical review. D. (2026) | TGRS Research Map | TGRS