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Enhanced Parameter Estimation for Inspiral Waveforms GWDAW-9, Annecy

Discover the sensitivity range of interferometers for black hole binaries, including mass and event rate comparisons. Explore parameter estimation methods at constant SNR and distance for coalescence time, chirp mass, and mass ratio.

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Enhanced Parameter Estimation for Inspiral Waveforms GWDAW-9, Annecy

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  1. Parameter Estimation Using 3.5 post-Newtonian Inspiral WaveformsGWDAW, December 15-18, 2004, Annecy K. Arun, B.R. Iyer, B.S. Sathyaprakash and P. Sundarajan

  2. Sensitivity of the instruments GWDAW-9, Annecy

  3. Span of the interferometers • Detectors have the best sensitivity to black hole binaries with mass in the range 10-200 M • Initial LIGO and Virgo have similar sensitivities for binaries in the range 10-50 M • Advanced LIGO has a span of 15 times greater than Initial LIGO/VIRGO or an event rate 3000 times larger GWDAW-9, Annecy

  4. Parameter Estimation at Constant SNR: Coalescence Time GWDAW-9, Annecy

  5. Parameter Estimation at Constant SNR: Chirp Mass GWDAW-9, Annecy

  6. Parameter Estimation at Constant SNR: Mass Ratio GWDAW-9, Annecy

  7. Parameter Estimation at Constant Distance: Coalescence Time GWDAW-9, Annecy

  8. Parameter Estimation at Constant Distance: Chirp Mass GWDAW-9, Annecy

  9. Parameter Estimation at Constant Distance: Mass Ratio GWDAW-9, Annecy

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