Motti Intermediate Physics — HAL: Laboratory Measurement of G, Cosmic String GW, and Primordial Nucleosynthesis

Three HAL results: (1) Lab measurements of G measure G_eff = G_N/C0; G_N = C0 x G_CODATA is a HAL prediction unobservable by measuring G alone. (2) Cosmic string GW: h^HAL = h^GR/C0 (-0.73%), opposite to merger GW. (3) BBN: H^HAL = H^GR exactly, all abundances unchanged.

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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.20935191
Primary Topic
Gamma-ray bursts and supernovae
Type
preprint
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preprint

Motti Intermediate Physics — HAL: Laboratory Measurement of G, Cosmic String GW, and Primordial Nucleosynthesis

Mordecai Gavila Alvarez
Zenodo (CERN European Organization for Nuclear Research)
Gamma-ray bursts and supernovae
preprint

Motti Intermediate Physics — HAL: Laboratory Measurement of G, Cosmic String GW, and Primordial Nucleosynthesis

Mordecai Gavila Alvarez
preprint en

Abstract

Three HAL results: (1) Lab measurements of G measure G_eff = G_N/C0; G_N = C0 x G_CODATA is a HAL prediction unobservable by measuring G alone. (2) Cosmic string GW: h^HAL = h^GR/C0 (-0.73%), opposite to merger GW. (3) BBN: H^HAL = H^GR exactly, all abundances unchanged.

Zenodo (CERN European Organization for Nuclear Research)
Valencia Catholic University Saint Vincent Martyr (ES)
Gamma-ray bursts and supernovae
DOIOpen Access PDFOpenAlex
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Motti Intermediate Physics — HAL: Laboratory Measurement of G, Cosmic String GW, and Primordial Nucleosynthesis — Mordecai Gavila Alvarez · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS