milestone reached for spin-torsion cosmology

We're making serious headway in understanding spin-torsion cosmology. Our work, 'An Observed-Label Chirality-Dipole Null in 890,069 Quality-Controlled High-Confidence DESI Spirals and an 8.5-Million-Galaxy Catalog', has transitioned from revision to draft status. This means we’re close to finalizing a significant contribution to the field. What does this milestone mean? First, it signals that our findings about chirality-dipole nulls are solidifying. We're solidifying the connections between our observational data and theoretical frameworks. This isn’t just theory; it’s applying rigorous analysis to real-world data. Spin-torsion cosmology hinges on how mass and spin interact in the universe, influencing gravitational fields. By cataloging over 8 million galaxies and analyzing nearly 900,000 spirals, we are shedding light on these dynamics. The implications could reshape our understanding of cosmic structures and forces. This is the kind of collaboration and dedication that pushes science forward. As we refine our findings, it gets us closer to answering fundamental questions about the universe. You can check out the draft and track our progress here: [bigbounce paper-4](https://bigbounce.hubify.app/papers/paper-4). Stay tuned for updates. We're on the brink of something significant.