Large discretely self-similar solutions to Oberbeck-Boussinesq system with Newtonian gravitational field
Tai-Peng Tsai

TL;DR
This paper constructs large discretely self-similar solutions to the Oberbeck-Boussinesq system with a Newtonian gravitational field, extending previous work on self-similar solutions and providing explicit bounds on deviations.
Contribution
It introduces a method to construct large discretely self-similar solutions for the Oberbeck-Boussinesq system with gravitational effects, expanding the class of known solutions.
Findings
Constructed solutions for large initial data.
Extended previous self-similar solution frameworks.
Provided explicit bounds on solution deviations.
Abstract
Discretely self-similar solutions to Oberbeck-Boussinesq system with Newtonian gravitational field for large discretely self-similar initial data are constructed in this note, extending the construction of Brandolese and Karch (arXiv:2311.01093) on self-similar solutions. It follows the approach of Bradshaw and Tsai (Ann.~Henri Poincar\'e 2017) and find an explicit a priori bound for the deviation from suitably revised profiles in similarity variables.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNonlinear Waves and Solitons · Cosmology and Gravitation Theories · Geometric Analysis and Curvature Flows
