Observation of Gravitational Waves from a Binary Black Hole Merger

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• Book V — Categorical Macrocosm Part 2
  Chapter Linear τ-Einstein: Weak-Field Regime and Classical Tests

  GW150914: Binary black hole merger. The first direct detection of gravitational waves (2015) was a binary black hole merger with chirp mass M ≈ 28.3 M_ at luminosity distance ∼ 410 Mpc

• Book V — Categorical Macrocosm Part 5
  Chapter Binary Mergers and Gravitational-Wave Readout

  Binary Mergers and Gravitational-Wave Readout On September 14, 2015, the Laser Interferometer Gravitational-Wave Observatory (LIGO) detected the gravitational-wave signal GW150914: the merger of two black holes with masses 36 M_ and 29 M_ at a distance of ∼ 410 Mpc, releasing ∼ 3 M_ c^2 of energy in gravitational radiation over a fraction of a second

• Book V — Categorical Macrocosm Part 7
  Chapter The Correspondence Map: τ³ leftrightarrow Orthodox Physics

  Gravitational dynamics (Schwarzschild , Kerr , gravitational waves ), since the τ-Einstein identity reduces to the Einstein field equation in the chart limit

• Book V — Categorical Macrocosm Part 7
  Chapter General Relativity as Emergent Geometry

  Modern confirmations. enumi4 Gravitational waves (LIGO, 2015) : the binary black hole merger GW150914 matched the GR waveform template to within calibration uncertainties

• Book V — Categorical Macrocosm Part 7
  Chapter The Dark Sector Dissolved

  Modern confirmations. enumi4 Gravitational waves (LIGO, 2015) : GW150914 matched the GR waveform template

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