The 72 Hertz That Divides to Two: I Ran an f(R,T) Echo Paper's Printed Numbers Through Its Own Frequency Formula, and the GW170817 Match Broke in Exactly the Leg That Carried It

Prices Queue-2 item Q2-12, arXiv:2610.30770 (Jayawiguna, Sabian, Ramadhan & Sulaksono, axial perturbations of extended Tolman III in f(R,T) gravity), on its verified abstract claim, the TSI store record, and the full text. The load-bearing step is the assumed identification of a constant-density star, at beta = 0.4662702 and chi = 0.96 pi, as a neutron star at the NICER radius R = 11.4 km matched to GW170817's reported 72 Hz echo frequency. The audit is arithmetic on the paper's own printed chain: the GR leg is internally exact (tau_tilde 25.3 -> 519.7 Hz vs printed 519 Hz), while the f(R,T) leg, exact through its printed tau_echo = 7.18e4 km = 239 ms, returns f_echo = 2.09 Hz under the paper's own eq. (63), not the printed 72.11 Hz -- a factor 34.5 break in the leg that carries the headline. The assumed object has M = beta R = 3.60 solar masses at 99.65 percent of the model's allowed compactness maximum. DERIVED-INDEPENDENT. Quantum gravity NOT SOLVED; vacuum catastrophe NOT SOLVED.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-04
DOI
https://doi.org/10.5281/zenodo.23937570
Primary Topic
Pulsars and Gravitational Waves Research
Type
preprint
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preprint

The 72 Hertz That Divides to Two: I Ran an f(R,T) Echo Paper's Printed Numbers Through Its Own Frequency Formula, and the GW170817 Match Broke in Exactly the Leg That Carried It

William Alexander Aldred
Zenodo (CERN European Organization for Nuclear Research)
Pulsars and Gravitational Waves Research
preprint

The 72 Hertz That Divides to Two: I Ran an f(R,T) Echo Paper's Printed Numbers Through Its Own Frequency Formula, and the GW170817 Match Broke in Exactly the Leg That Carried It

William Alexander Aldred
preprint en

Abstract

Prices Queue-2 item Q2-12, arXiv:2610.30770 (Jayawiguna, Sabian, Ramadhan & Sulaksono, axial perturbations of extended Tolman III in f(R,T) gravity), on its verified abstract claim, the TSI store record, and the full text. The load-bearing step is the assumed identification of a constant-density star, at beta = 0.4662702 and chi = 0.96 pi, as a neutron star at the NICER radius R = 11.4 km matched to GW170817's reported 72 Hz echo frequency. The audit is arithmetic on the paper's own printed chain: the GR leg is internally exact (tau_tilde 25.3 -> 519.7 Hz vs printed 519 Hz), while the f(R,T) leg, exact through its printed tau_echo = 7.18e4 km = 239 ms, returns f_echo = 2.09 Hz under the paper's own eq. (63), not the printed 72.11 Hz -- a factor 34.5 break in the leg that carries the headline. The assumed object has M = beta R = 3.60 solar masses at 99.65 percent of the model's allowed compactness maximum. DERIVED-INDEPENDENT. Quantum gravity NOT SOLVED; vacuum catastrophe NOT SOLVED.

Zenodo (CERN European Organization for Nuclear Research)
Pulsars and Gravitational Waves Research
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The 72 Hertz That Divides to Two: I Ran an f(R,T) Echo Paper's Printed Numbers Through Its Own Frequency Formula, and the GW170817 Match Broke in Exactly the Leg That Carried It — William Alexander Aldred · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS