Motti Intermediate Physics - HAL: Observational Consistency - Binary Pulsars, Gravitational Wave Amplitude, and Cosmological Parameters

Key Points

• This research assesses the consistency of HAL predictions with various observational data including binary pulsars and gravitational waves.
• Systematic analysis comparing dPb/dt from HAL and GR for binary pulsars.
• Evaluation of gravitational wave amplitude, correlating HAL predictions with LIGO thresholds.
• Comparison of cosmological parameters including Hubble constant and Omega_Lambda against observational data.
• dPb/dt^HAL matches dPb/dt^GR exactly, supporting ADM protection.
• GW amplitude from HAL is 0.73% above GR, measured below LIGO O3 threshold and at LIGO O5 threshold.
• Cosmological parameters work out to H^HAL = H^GR, with Omega_Lambda at 0.695 as predicted for Euclid 2028.