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The Search for Massive Black Hole Binaries with LISA

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arxiv gr-qc/0612091 v3 pith:AC4SJTDR submitted 2006-12-14 gr-qc

classification gr-qc
keywords searchblackbinariesdataholestreamsystemsalgorithm
verification ladder T0 review T1 audit T2 compute T3 formal

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In this work we focus on the search and detection of Massive black hole binary (MBHB) systems, including systems at high redshift. As well as expanding on previous works where we used a variant of Markov Chain Monte Carlo (MCMC), called Metropolis-Hastings Monte Carlo, with simulated annealing, we introduce a new search method based on frequency annealing which leads to a more rapid and robust detection. We compare the two search methods on systems where we do and do not see the merger of the black holes. In the non-merger case, we also examine the posterior distribution exploration using a 7-D MCMC algorithm. We demonstrate that this method is effective in dealing with the high correlations between parameters, has a higher acceptance rate than previously proposed methods and produces posterior distribution functions that are close to the prediction from the Fisher Information matrix. Finally, after carrying out searches where there is only one binary in the data stream, we examine the case where two black hole binaries are present in the same data stream. We demonstrate that our search algorithm can accurately recover both binaries, and more importantly showing that we can safely extract the MBHB sources without contaminating the rest of the data stream.

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Cited by 3 Pith papers

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

  1. Handling Data Gaps for the Next Generation of Gravitational-Wave Observatories

    gr-qc 2025-09 unverdicted novelty 6.0 of 10

    Presents an efficient time-frequency Bayesian gap-filling technique that avoids costly matrix operations and integrates into LISA Global Fit, demonstrated on simulated LISA data.

  2. DeepHMC : a deep-neural-network acclerated Hamiltonian Monte Carlo algorithm for binary neutron star parameter estimation

    gr-qc 2025-05 conditional novelty 6.0 of 10

    A neural-network surrogate for the log-likelihood gradients makes Hamiltonian Monte Carlo trajectories 30 times faster than relative-binning gradients and recovers LVK-consistent posteriors for two binary neutron star...

  3. Detection and parameter estimation of supermassive black hole ringdown signals using a pulsar timing array

    astro-ph.HE 2024-12 conditional novelty 6.0 of 10

    A likelihood-based search with particle swarm optimization can detect and estimate supermassive black hole ringdown signals in simulated pulsar timing array data, reaching 99% detection probability at SNR 10.

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