Motti Intermediate Physics — HAL: The Stochastic Gravitational Wave Background — Sign-Dependent Corrections and Spectral Ratios

HAL corrections to the stochastic GW background: merger-dominated backgrounds enhanced by C0^2 (+1.46%) because J_total = C0^2 J_GR; rotating NS backgrounds suppressed by 1/C0^2 (-1.44%) because I^HAL = I^GR. Sign depends on whether source is angular momentum (enhanced) or mass quadrupole (suppressed). New prediction: spectral ratio Omega(PTA)/Omega(ET) enhanced by C0^4 (+2.95%) if ET band is NS-rotation dominated. Consistent with NANOGrav 2023.

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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.20934343
Primary Topic
Pulsars and Gravitational Waves Research
Type
preprint
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preprint

Motti Intermediate Physics — HAL: The Stochastic Gravitational Wave Background — Sign-Dependent Corrections and Spectral Ratios

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

Motti Intermediate Physics — HAL: The Stochastic Gravitational Wave Background — Sign-Dependent Corrections and Spectral Ratios

Mordecai Gavila Alvarez
preprint en

Abstract

HAL corrections to the stochastic GW background: merger-dominated backgrounds enhanced by C0^2 (+1.46%) because J_total = C0^2 J_GR; rotating NS backgrounds suppressed by 1/C0^2 (-1.44%) because I^HAL = I^GR. Sign depends on whether source is angular momentum (enhanced) or mass quadrupole (suppressed). New prediction: spectral ratio Omega(PTA)/Omega(ET) enhanced by C0^4 (+2.95%) if ET band is NS-rotation dominated. Consistent with NANOGrav 2023.

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