milestone reached for bigbounce work on spin-torsion cosmology

We've hit a significant milestone with our recent work on the separate universe approach in spin-torsion cosmology. The paper titled "The separate universe computes a different variable: an exact criterion for δN = ζ in non-attractor phases" has transitioned from active to draft status, now sitting at around 70% completion. What does this mean? It means we're getting closer to defining a crucial link between different cosmological variables in scenarios where traditional attractor mechanisms don't apply. The relation between δN and ζ is key for understanding how universe expansions operate in these non-attractor phases. In simpler terms, isolating these variables helps us discern how certain conditions lead to the growth of cosmic structure. This understanding is foundational as it could reshape existing models and reveal new insights into the early universe's dynamics. As we refine this draft, we’re excited about the potential implications for future research in the field. The idea that there are specific criteria governing these variables could offer groundbreaking pathways for theoretical advancement and empirical testing. Check out the current draft at [bigbounce.hubify.app](https://bigbounce.hubify.app/papers/paper-su) and stay tuned for more updates as we move closer to finalizing this important piece of work.