ΔΩc\u209cN V3 is an operational package developed to accompany the HDC–CBC/ΔΩc\u209c framework through a reproducible numerical implementation of trajectory-enabled correlational closure.
\nThe package includes two main versions of the pipeline:
\nDeltaOmegaCtN_V3
A classic terminal-oriented version designed for direct execution, controlled sweeps, reproducible output generation and structural validation of the parameter space.
DeltaOmegaCtN_V3_Chat
A guided conversational version designed to facilitate step-by-step execution through assisted selection of families, anchors, execution depth and historical trajectory parameters.
The purpose of ΔΩc\u209cN V3 is to preserve the benchmark layer inherited from ΩCt/N while adding a dynamical trajectory layer for the correlational index. In this version, users can explore constant configurations, smooth transitions and ΔΩc\u209c trajectories through explicit controls such as the potential model, effective closure strength, dynamical branch, normalization convention and reference correlational value.
\nThe pipeline is intended as a reviewer-ready structural validation environment. It supports reproducible sweeps, trajectory tests, proxy-level observational diagnostics, result classification and identification of the first rupture sector. It is not intended to replace full cosmological codes such as CLASS, CAMB or hi_class, nor does it constitute a final Bayesian inference engine. Its role is to provide a lightweight, transparent and executable tool for evaluating the structural admissibility of correlational trajectories within the HDC–CBC/ΔΩc\u209c framework.
\nThis release also includes the official user manuals in Spanish and English:
\nManual_Oficial_DeltaOmegaCtN_ES_V3
Official Spanish user manual, including installation instructions, execution modes, configuration options, output interpretation, known limitations and recommended usage practices.
Manual_Official_DeltaOmegaCtN_EN_V3
Official English user manual, including installation instructions, execution modes, trajectory controls, output interpretation, known limitations and recommended usage practices.
Version V3 corrects and consolidates the operational implementation with respect to previous transitional versions. It includes full deltaomegact support, bilingual execution aliases, an explicit quartic potential option, operational normalization, proxy-validation policy, declared dependencies and updated launchers.
What can be submitted?
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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