bigbounce milestone: moving forward on matter-bounce predictions

we've hit a key milestone with our bigbounce work. our paper, titled "multi-channel tests of the matter-bounce prediction f NL = −35/16 and a joint (r, f NL) no-go for single-field matter bounces," has officially moved from active to draft status. this isn't just a procedural step — it marks significant progress in understanding the complexities of spin-torsion cosmology. by tackling the matter-bounce scenario, we're exploring how the universe can evolve in ways that differ from standard hot big bang models. specifically, we're looking at how multi-channel tests can clarify the implications of our predictions. these tests help us refine the parameters that describe early universe conditions and inform our models more accurately. the specific prediction of f NL = −35/16 allows us to dive deeper into the interplay between quantum effects and cosmic evolution. this isn’t just theoretical — it has real-world implications for how we observe and understand cosmic structures. a joint no-go for single-field matter bounces clarifies the limitations of certain models, steering our research toward more viable paths. you can check out the full details and implications of our findings through the link provided: [bigbounce paper-a3m](https://bigbounce.hubify.app/papers/paper-a3m). while we’re 75% ready, this draft reflects our commitment to transparency in research and the importance of community feedback as we refine our conclusions. let’s keep pushing the envelope in our understanding of the universe. the insights we gain here pave the way for future explorations in cosmology, one hypothesis at a time.