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

Systematic consistency check of HAL against all observational data. Binary pulsars: dPb/dt^HAL = dPb/dt^GR exactly (ADM protection). GW amplitude: h^HAL = C0 h^GR (+0.73%), below LIGO O3 threshold, at LIGO O5 threshold with 200 events and 0.5 percent calibration. Cosmology: H^HAL = H^GR (BBN, CMB, BAO identical). Omega_Lambda = 0.695 (Euclid 2028). sigma_8 partially alleviated. Hubble tension unresolved. Programme ready for experimental verdict.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-06-26
DOI
https://doi.org/10.5281/zenodo.20937309
Primary Topic
Pulsars and Gravitational Waves Research
Type
preprint
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preprint

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

Mordecai Gavila Alvarez
Zenodo (CERN European Organization for Nuclear Research)
Pulsars and Gravitational Waves Research
preprint

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

Mordecai Gavila Alvarez
preprint en

Abstract

Systematic consistency check of HAL against all observational data. Binary pulsars: dPb/dt^HAL = dPb/dt^GR exactly (ADM protection). GW amplitude: h^HAL = C0 h^GR (+0.73%), below LIGO O3 threshold, at LIGO O5 threshold with 200 events and 0.5 percent calibration. Cosmology: H^HAL = H^GR (BBN, CMB, BAO identical). Omega_Lambda = 0.695 (Euclid 2028). sigma_8 partially alleviated. Hubble tension unresolved. Programme ready for experimental verdict.

Zenodo (CERN European Organization for Nuclear Research)
Valencia Catholic University Saint Vincent Martyr (ES)
Pulsars and Gravitational Waves Research
DOIOpen Access PDFOpenAlex
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