Abstract
Clearly, a lot can still be explored further already in what I have presented so far. But I have also explored two other paths, constituting two important generalizations: (i) cylindrical geometry in order to explore the stability of cosmic filaments and (ii) taking buoyancy fully into account in order to explore the importance of this physical process, which is paramount in stellar dynamics. After presenting them, I will finally mention key interrogations brought by the experience gained through the above analysis and that must be tackled to go further to optimize the approach.
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Notes
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More precisely, the only non zero derivatives are \(\partial _\theta \hat{R} = \hat{\theta }\) and \(\partial _\theta \hat{\theta } = - \hat{R}\).
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Durrive, JB. (2017). Further Ongoing Works. In: Baryonic Processes in the Large-Scale Structuring of the Universe. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-61881-4_9
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