About the work
\begin{abstract}
The Stochastic Gravitational Wave Background (SGWB) is an astrophysical and cosmological relic that encodes valuable information about the early universe and the nature of fundamental interactions. While standard General Relativity (GR) predicts the SGWB spectrum based on well-known sources such as inflation, cosmic strings, and mergers of compact objects, the Emergent Quantum Fields and Adaptive Gravity Theory (CCEGA) introduces an adaptive curvature parameter $R_c$ that dynamically modifies spacetime geometry. This adaptation leads to distinct corrections in the SGWB energy density spectrum $\Omega_{GW}(f)$, alters the angular power spectrum $C_\ell$, and results in a scale-dependent speed of gravitational waves. We analyze how $R_c$ impacts the propagation and anisotropies of the SGWB, providing predictions that differ from GR. Observations from upcoming experiments such as LISA, CMB-S4, and the Einstein Telescope will be crucial to test these predictions. This work highlights how CCEGA moves beyond conceptual unification by offering specific observational signatures in the stochastic gravitational wave background, establishing a concrete path to empirically validate the framework.
\end{abstract}
\begin{abstract}
The Stochastic Gravitational Wave Background (SGWB) is an astrophysical and cosmological relic that encodes valuable information about the early universe and the nature of fundamental interactions. While standard General Relativity (GR) predicts the SGWB spectrum based on well-known sources such as inflation, cosmic strings, and mergers of compact objects, the Emergent Quantum Fields and Adaptive Gravity Theory (CCEGA) introduces an adaptive curvature parameter $R_c$ that dynamically modifies spacetime geometry. This adaptation leads to distinct corrections in the SGWB energy density spectrum $\Omega_{GW}(f)$, alters the angular power spectrum $C_\ell$, and results in a scale-dependent speed of gravitational waves. We analyze how $R_c$ impacts the propagation and anisotropies of the SGWB, providing predictions that differ from GR. Observations from upcoming experiments such as LISA, CMB-S4, and the Einstein Telescope will be crucial to test these predictions. This work highlights how CCEGA moves beyond conceptual unification by offering specific observational signatures in the stochastic gravitational wave background, establishing a concrete path to empirically validate the framework.
\end{abstract}
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Title \documentclass[12pt]{article} \usepackage[utf8]{inputenc} \usepackage[T1]{fontenc} \usepackage[english]{babel} \usepackage{amsmath,amssymb,physics} \usepackage{graphicx} \usepackage{hyperref} \usepackage{booktabs} \usepackage{geometry} \usepackage{xcolor}
\begin{abstract}
The Stochastic Gravitational Wave Background (SGWB) is an astrophysical and cosmological relic that encodes valuable information about the early universe and the nature of fundamental interactions. While standard General Relativity (GR) predicts the SGWB spectrum based on well-known sources such as inflation, cosmic strings, and mergers of compact objects, the Emergent Quantum Fields and Adaptive Gravity Theory (CCEGA) introduces an adaptive curvature parameter $R_c$ that dynamically modifies spacetime geometry. This adaptation leads to distinct corrections in the SGWB energy density spectrum $\Omega_{GW}(f)$, alters the angular power spectrum $C_\ell$, and results in a scale-dependent speed of gravitational waves. We analyze how $R_c$ impacts the propagation and anisotropies of the SGWB, providing predictions that differ from GR. Observations from upcoming experiments such as LISA, CMB-S4, and the Einstein Telescope will be crucial to test these predictions. This work highlights how CCEGA moves beyond conceptual unification by offering specific observational signatures in the stochastic gravitational wave background, establishing a concrete path to empirically validate the framework.
\end{abstract}
\begin{abstract}
The Stochastic Gravitational Wave Background (SGWB) is an astrophysical and cosmological relic that encodes valuable information about the early universe and the nature of fundamental interactions. While standard General Relativity (GR) predicts the SGWB spectrum based on well-known sources such as inflation, cosmic strings, and mergers of compact objects, the Emergent Quantum Fields and Adaptive Gravity Theory (CCEGA) introduces an adaptive curvature parameter $R_c$ that dynamically modifies spacetime geometry. This adaptation leads to distinct corrections in the SGWB energy density spectrum $\Omega_{GW}(f)$, alters the angular power spectrum $C_\ell$, and results in a scale-dependent speed of gravitational waves. We analyze how $R_c$ impacts the propagation and anisotropies of the SGWB, providing predictions that differ from GR. Observations from upcoming experiments such as LISA, CMB-S4, and the Einstein Telescope will be crucial to test these predictions. This work highlights how CCEGA moves beyond conceptual unification by offering specific observational signatures in the stochastic gravitational wave background, establishing a concrete path to empirically validate the framework.
\end{abstract}
Work type Technical
Tags black hole information, neurophysics, consciousness, curvature, information dynamics, ccega, emergent gravity, geometría adaptativa, quantum gravity, φ field, quantum field, non-biologiquantum entanglement, teoría de todo, multiverso, quantum field memory, adaptive geometryemergent time, emergent field theory, nonlocal structure, ccega campo φ, gravedad cuántica
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Identifier 2506302332439
Entry date Jun 30, 2025, 1:44 AM UTC
License Creative Commons Attribution-NonCommercial-ShareAlike 4.0
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Author 100.00 %. Holder MARC LOPEZ SANCHEZ. Date Jun 30, 2025.
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