TQNT-V5.9 — Gravitational waves from χ-field transverse-traceless modes (GW150914 chirp)

TQNT-V5.9 shows that the transverse-traceless (TT) modes of the V5 χ-field reproduce the standard general-relativistic gravitational wave equation in the long-wavelength limit, with propagation speed c and quadrupolar polarisation content (h+, h×). The leading-order inspiral chirp of GW150914 is recovered exactly within the precision of the V5-derived G inherited from V5.8. No new parameter is introduced relative to V5.7-V5.8. Complements the V5 monograph (10.5281/zenodo.19131538).

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-06-12
DOI
https://doi.org/10.5281/zenodo.20656825
Primary Topic
Pulsars and Gravitational Waves Research
Type
preprint
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preprint

TQNT-V5.9 — Gravitational waves from χ-field transverse-traceless modes (GW150914 chirp)

Lilian Cariou
Zenodo (CERN European Organization for Nuclear Research)
Pulsars and Gravitational Waves Research
preprint

TQNT-V5.9 — Gravitational waves from χ-field transverse-traceless modes (GW150914 chirp)

Lilian Cariou
preprint en

Abstract

TQNT-V5.9 shows that the transverse-traceless (TT) modes of the V5 χ-field reproduce the standard general-relativistic gravitational wave equation in the long-wavelength limit, with propagation speed c and quadrupolar polarisation content (h+, h×). The leading-order inspiral chirp of GW150914 is recovered exactly within the precision of the V5-derived G inherited from V5.8. No new parameter is introduced relative to V5.7-V5.8. Complements the V5 monograph (10.5281/zenodo.19131538).

Zenodo (CERN European Organization for Nuclear Research)
Systématique, adaptation, évolution (FR)
Pulsars and Gravitational Waves Research
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