Este volumen Ω nace como una síntesis estructural de todo el camino recorrido por la hipótesis HDC-CBC. No pretende reescribir los siete volúmenes previos, sino condensar su contenido en una forma operativa, comprensible y contrastable para cualquier lector que quiera poner a prueba el modelo.
\nEl objetivo es doble. Por un lado, ofrecer una visión de conjunto clara del marco correlacional: qué es exactamente el HDC-CBC, cuáles son sus ecuaciones fundamentales y cómo se articula con la Relatividad General y la física cuántica. Por otro lado, mostrar de manera ordenada qué consigue el modelo ya con su formulación clásica de C fija: qué tensiones cosmológicas alivia, qué observables respeta y qué predicciones fuertes pone sobre la mesa.
\nEn esta fase, Ω no introduce aún parámetros libres adicionales ni versiones “flexibilizadas” del modelo. Al contrario: se apoya en la versión más restrictiva del HDC-CBC, la que trabaja con un conjunto fijo de parámetros y con una correlación basal C que no se ajusta a posteriori. Esa fue la filosofía de QRPTON: comprobar hasta qué punto la hipótesis se sostiene cuando se le niega la tentación del fine-tuning y se la obliga a vivir bajo el criterio de máxima rigidez.
\nEl resultado de ese ejercicio es importante: incluso con C fija, el HDC-CBC reproduce con gran precisión la historia de expansión tipo ΛCDM, ofrece una interpretación geométrica y correlacional unificada, y proporciona un patrón muy concreto de predicciones:
\nLa única tensión mayor que queda claramente abierta en este escenario rígido es la discrepancia fina en H\u2080 entre reconstrucciones de universo temprano (tipo Planck) y medidas locales (tipo SH0ES). HDC-CBC, con C rígida, se sitúa de forma natural en un valor intermedio elevado pero no extremo; no fuerza la reconciliación total, pero sí sugiere hacia qué región del espacio de parámetros debería converger la solución.
\nΩ parte de esta constatación: antes incluso de introducir C\u209c, el modelo ya estaba haciendo un trabajo notable. La extensión con C\u209c variable aparece más tarde, no como excusa para salvar un fracaso, sino como una consecuencia casi inevitable de tomarse en serio la información que el propio HDC-CBC estaba devolviendo al compararlo con los datos.
\nEste volumen, por tanto, se organiza en dos etapas:
\nEl lector encontrará, en cada capítulo, no solo una narración conceptual, sino también un resumen operativo de las fórmulas clave: las suficientes para que alguien con formación en cosmología pueda implementar numéricamente el modelo, contrastarlo con datos o falsarlo. Las derivaciones detalladas y los desarrollos técnicos completos permanecen en los volúmenes originales; aquí se ofrece el mapa para recorrerlos con sentido.
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All types of scholarly material are welcome: preprints, papers, presentations, data, simulations, commentaries, reviews, videos, or conference proceedings, as long as they relate to the core theme of non-standard cosmology and astrophysics.
Who can contribute?
This community is open to independent researchers, interdisciplinary thinkers, and academic scientists alike. We value intellectual curiosity, open inquiry, and respectful dialogue across backgrounds and disciplines.
Open Science, Open Review
In the spirit of open science, no moderation or gatekeeping is applied to submissions, unless if they seem to fall outside the scope of this community. For all submissions, community commenting, open peer review, and critical discussion are encouraged to promote transparency, collaboration, and constructive engagement.
This community brings together research that explores and challenges the assumptions, theories, and interpretations of standard cosmology and astrophysics.
\nWe welcome all contributions that lie outside or question the mainstream paradigms, including alternative cosmological models, alternative solar models, reinterpretations of astrophysical data, and critical examinations of foundational concepts such as the cosmic microwave background, redshift, galactic rotation curves, general relativity, and more. If your work addresses what doesn’t quite “fit” in the standard models, whether theoretically, observationally, or methodologically, it belongs here.
\nOrigin
This community was initiated following DemystiCon 2025: Beyond the Big Bang, a conference on non-standard cosmology and astrophysics organized by DemystifySci and held in June 2025 in Sesimbra, Portugal. The first contribution is the Book of Abstracts from this event, and we warmly invite others working in related areas to share their research here.
Let this be a space for bold ideas, careful questioning, and fresh perspectives on the cosmos.
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