Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals
gr-qc, astro-ph.HE, hep-th
Submitted: 2026-06-25
Updated: 2026-10-07
Comments: 24 pages, 9 figures, 4 tables
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
- Tests of General Relativity with GW170817
- GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
- Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors
- Testing General Relativity with Present and Future Astrophysical Observations
- Research Update on Extreme-Mass-Ratio Inspirals
- Testing gravity with Extreme-Mass-Ratio Inspirals
- Testing the nature of dark compact objects: a status report
- Waveform Modelling for the Laser Interferometer Space Antenna
- Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals
- Laser Interferometer Space Antenna
- New Horizons for Fundamental Physics with LISA
- LISA Definition Study Report
- TianQin: a space-borne gravitational wave detector
- The TianQin project: current progress on science and technology
- Taiji Program: Gravitational-Wave Sources
- Possibility of Direct Measurement of the Acceleration of the Universe Using 0.1 Hz Band Laser Interferometer Gravitational Wave Antenna in Space
- Current status of space gravitational wave antenna DECIGO and B-DECIGO
- Constructing EOB dynamics with numerical energy flux for intermediate-mass-ratio inspirals
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