Density and Goldstone emission of an RP³ ≃ SO(3) global-string network relative to U(1), and a massive-bath systematic of the emission estimator

We simulate networks of global Z₂ strings whose vacuum manifold is RP³ ≃ SO(3), produced by a real symmetric-tensor order parameter, and compare them with U(1) axion-string networks evolved in the same code, with the same Goldstone decay constant and core mass, at 576³ (U(1) control also at 768³, where it passes preregistered scaling gates). The string-density ratio is R_ξ ≃ 1.6 for every protocol tested: sparse and dense starts, with and without draining the initial massive radiation, and networks started late and dense that approach the attractor from above, which bracket it to R_ξ ∈ [1.57, 1.68] at ℓ = ln(m_r/H) = 5.61. We identify a systematic of the standard kinetic Goldstone-emission estimator: the conversion of massive radiation left by the initial state into Goldstones is counted as string emission. It is 19% (RP³) and 28% (U(1)) of the measured emission for sparse starts and more than half for dense ones; for U(1) two independent methods, a drain of the massive modes and a direct measurement of the radial-to-Goldstone transfer, agree. With the bath drained, the emission ratio is R_Γ = 1.56 ± 0.09 (stat) ± 0.08 (sampling), independent of the initial density within ≈7%, and the emission per unit string length is within 13% of U(1) from both sides of the attractor. The spectral slope of the RP³ emission at ℓ = 5 is q = 0.87 ± 0.06 with our estimator, but an independent re-implementation shows that the convention used to map the physical fitting window onto lattice momenta shifts it by up to 0.07; we therefore quote q as compatible with 1. All verdict-bearing analyses were preregistered and are reproducible from the released data. Code, network summaries, preregistered specifications, the independent audit and the figure scripts: https://github.com/indigenica/whalefall-rp3-string-networks (code GPL-3.0-or-later; data CC BY-NC 4.0). A script in that repository recomputes every number quoted in the paper from the stored results and checks it against the text.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-10-18
DOI
https://doi.org/10.5281/zenodo.23451009
Primary Topic
Cosmology and Gravitation Theories
Type
preprint
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preprint

Density and Goldstone emission of an RP³ ≃ SO(3) global-string network relative to U(1), and a massive-bath systematic of the emission estimator

Jose Bautista
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
preprint

Density and Goldstone emission of an RP³ ≃ SO(3) global-string network relative to U(1), and a massive-bath systematic of the emission estimator

Jose Bautista
preprint en

Abstract

We simulate networks of global Z₂ strings whose vacuum manifold is RP³ ≃ SO(3), produced by a real symmetric-tensor order parameter, and compare them with U(1) axion-string networks evolved in the same code, with the same Goldstone decay constant and core mass, at 576³ (U(1) control also at 768³, where it passes preregistered scaling gates). The string-density ratio is R_ξ ≃ 1.6 for every protocol tested: sparse and dense starts, with and without draining the initial massive radiation, and networks started late and dense that approach the attractor from above, which bracket it to R_ξ ∈ [1.57, 1.68] at ℓ = ln(m_r/H) = 5.61. We identify a systematic of the standard kinetic Goldstone-emission estimator: the conversion of massive radiation left by the initial state into Goldstones is counted as string emission. It is 19% (RP³) and 28% (U(1)) of the measured emission for sparse starts and more than half for dense ones; for U(1) two independent methods, a drain of the massive modes and a direct measurement of the radial-to-Goldstone transfer, agree. With the bath drained, the emission ratio is R_Γ = 1.56 ± 0.09 (stat) ± 0.08 (sampling), independent of the initial density within ≈7%, and the emission per unit string length is within 13% of U(1) from both sides of the attractor. The spectral slope of the RP³ emission at ℓ = 5 is q = 0.87 ± 0.06 with our estimator, but an independent re-implementation shows that the convention used to map the physical fitting window onto lattice momenta shifts it by up to 0.07; we therefore quote q as compatible with 1. All verdict-bearing analyses were preregistered and are reproducible from the released data. Code, network summaries, preregistered specifications, the independent audit and the figure scripts: https://github.com/indigenica/whalefall-rp3-string-networks (code GPL-3.0-or-later; data CC BY-NC 4.0). A script in that repository recomputes every number quoted in the paper from the stored results and checks it against the text.

Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
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Density and Goldstone emission of an RP³ ≃ SO(3) global-string network relative to U(1), and a massive-bath systematic of the emission estimator — Jose Bautista · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS