Inverse Construction of Coherential Backgrounds Compatible with Tachyonic Stability

This work is a toy inverse-construction benchmark, not an astrophysical background. We introduce an inverse methodology for generating one-dimensional coherential profiles C_0(y) compatible with tachyonic stability (T3) under the D6-F operational combination of Radial Coherential Dynamics (RCD), within a previously ghost/gradient-controlled extended regime (LB-04 with decoupling limit, quasi-static approximation, Brown-Schutz dust, |xi|<1, Z_0>0). Forward attempts with Gaussian-bump and tanh-wall profiles produce structural failures driven by the sign of the kinetic-geometric functional Phi[C_0] = 2(C_0')^2 + (1-C_0)C_0'', not by matter or coupling parameters. Imposing Phi[C_0] >= 0 as a design constraint and integrating, we obtain a closed-form first integral (u')^2 = epsilon_0/2 + C_1 u^4 with u = 1-C_0. The saturation branch (Phi = 0) yields a non-viable hyperbolic profile; the simplest strict-positivity branch (Phi = epsilon_0 > 0, C_1 = 0) yields a linear bank with a closed-form upper bound rho_max(m, alpha, mu) = 4m^2 / [alpha * sqrt(1 + (m^2/mu^4)/(1+alpha))] on the dimensionless matter density. For representative parameters (m, alpha, mu) = (0.4, 1e-4, 1) this gives rho_max ~ 5.94 x 10^3, a four-order margin against natural values. The linear bank is shown to be optimal within its family: the non-linear branch C_1 > 0 preserves Phi exactly but strictly degrades the matter margin and contracts the domain length. The result is offered as a methodological contribution: a viable inverse-construction route exists for T3 in D6-F, with the linear bank as its first closed example, not its final destination. Scope is explicitly bounded: the result is a toy bank, not an astrophysical background; T1 and T2 are inherited from previous D6-F analysis and not rederived here; no claim is made about global RCD stability or about deriving the program's parameter alpha. The note includes an appendix with a self-contained derivation of the master bound V_0^max from the D6-F action in the LB-04 extended regime, two figures (forward vs. inverse methodology; profile and kinetic-geometric functional across three banks), and explicit references to the EFT-for-dark-energy framework of Frusciante et al. (2016, 2017, 2019) and to the Brown-Schutz matter action (Brown 1993; Sorkin 1997). Draft v1, May 2026. Internal Panel Cerezo review applied. Symbolic verifications with SymPy and numerical evaluations with SciPy fully reproducible from the equations as stated.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-05-18
DOI
https://doi.org/10.5281/zenodo.20262975
Primary Topic
Cosmology and Gravitation Theories
Type
preprint
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preprint

Inverse Construction of Coherential Backgrounds Compatible with Tachyonic Stability

Arturo Cerezo
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
preprint

Inverse Construction of Coherential Backgrounds Compatible with Tachyonic Stability

Arturo Cerezo
preprint en

Abstract

This work is a toy inverse-construction benchmark, not an astrophysical background. We introduce an inverse methodology for generating one-dimensional coherential profiles C_0(y) compatible with tachyonic stability (T3) under the D6-F operational combination of Radial Coherential Dynamics (RCD), within a previously ghost/gradient-controlled extended regime (LB-04 with decoupling limit, quasi-static approximation, Brown-Schutz dust, |xi|<1, Z_0>0). Forward attempts with Gaussian-bump and tanh-wall profiles produce structural failures driven by the sign of the kinetic-geometric functional Phi[C_0] = 2(C_0')^2 + (1-C_0)C_0'', not by matter or coupling parameters. Imposing Phi[C_0] >= 0 as a design constraint and integrating, we obtain a closed-form first integral (u')^2 = epsilon_0/2 + C_1 u^4 with u = 1-C_0. The saturation branch (Phi = 0) yields a non-viable hyperbolic profile; the simplest strict-positivity branch (Phi = epsilon_0 > 0, C_1 = 0) yields a linear bank with a closed-form upper bound rho_max(m, alpha, mu) = 4m^2 / [alpha * sqrt(1 + (m^2/mu^4)/(1+alpha))] on the dimensionless matter density. For representative parameters (m, alpha, mu) = (0.4, 1e-4, 1) this gives rho_max ~ 5.94 x 10^3, a four-order margin against natural values. The linear bank is shown to be optimal within its family: the non-linear branch C_1 > 0 preserves Phi exactly but strictly degrades the matter margin and contracts the domain length. The result is offered as a methodological contribution: a viable inverse-construction route exists for T3 in D6-F, with the linear bank as its first closed example, not its final destination. Scope is explicitly bounded: the result is a toy bank, not an astrophysical background; T1 and T2 are inherited from previous D6-F analysis and not rederived here; no claim is made about global RCD stability or about deriving the program's parameter alpha. The note includes an appendix with a self-contained derivation of the master bound V_0^max from the D6-F action in the LB-04 extended regime, two figures (forward vs. inverse methodology; profile and kinetic-geometric functional across three banks), and explicit references to the EFT-for-dark-energy framework of Frusciante et al. (2016, 2017, 2019) and to the Brown-Schutz matter action (Brown 1993; Sorkin 1997). Draft v1, May 2026. Internal Panel Cerezo review applied. Symbolic verifications with SymPy and numerical evaluations with SciPy fully reproducible from the equations as stated.

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