Black Hole Hunting with LISA
arXiv:2005.03610 · doi:10.1103/PhysRevD.101.124008
Abstract
The Laser Interferometer Space Antenna (LISA) will be able to detect massive black hole mergers throughout the visible Universe. These observations will provide unique information about black hole formation and growth, and the role black holes play in galaxy evolution. Here we develop several key building blocks for detecting and characterizing black hole binary mergers with LISA, including fast heterodyned likelihood evaluations, and efficient stochastic search techniques.
11 pages, 11 figures
References in corpus (9)
- Reconstructing the massive black hole cosmic history through gravitational waves
- The Mock LISA Data Challenges: from Challenge 3 to Challenge 4
- Accelerated gravitational-wave parameter estimation with reduced order modeling
- The Mock LISA Data Challenges: from Challenge 1B to Challenge 3
- The Effect of Higher Harmonic Corrections on the Detection of massive black hole binaries with LISA
- MCMC Exploration of Supermassive Black Hole Binary Inspirals
- Catching Super Massive Black Hole Binaries Without a Net
- Searching for Massive Black Hole Binaries in the first Mock LISA Data Challenge
- Inference on inspiral signals using LISA MLDC data
Cited by in corpus (4)
- Modeling compact binary signals and instrumental glitches in gravitational wave data
- Computational Techniques for Parameter Estimation of Gravitational Wave Signals
- Tracing Astrophysical Black Hole Seeds and Primordial Black Holes with LISA-Taiji Network
- LISA Gravitational Wave Sources in A Time-Varying Galactic Stochastic Background