Weak solutions for Euler systems with non-local interactions
We consider several modifications of the Euler system of fluid dynamics, including its pressureless variant driven by non-local interaction repulsive-attractive and alignment forces in the space dimension N = 2, 3. These models arise in the study of self-organization in collective behavior modeling...
Main Authors: | , , , |
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Format: | Journal article |
Language: | English |
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Wiley
2017
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author | Carrillo De La Plata, J Feireisl, E Gwiazda, P Swierczewska-Gwiazda, A |
author_facet | Carrillo De La Plata, J Feireisl, E Gwiazda, P Swierczewska-Gwiazda, A |
author_sort | Carrillo De La Plata, J |
collection | OXFORD |
description | We consider several modifications of the Euler system of fluid dynamics, including its pressureless variant driven by non-local interaction repulsive-attractive and alignment forces in the space dimension N = 2, 3. These models arise in the study of self-organization in collective behavior modeling of animals and crowds. We adapt the method of convex integration to show the existence of infinitely many global-in-Time weak solutions for any bounded initial data. Then we consider the class of dissipative solutions satisfying, in addition, the associated global energy balance (inequality).We identify a large set of initial data for which the problem admits infinitely many dissipative weak solutions. Finally, we establish a weak-strong uniqueness principle for the pressure-driven Euler system with non-local interaction terms as well as for the pressurelesssystem with Newtonian interaction. |
first_indexed | 2024-03-06T21:31:12Z |
format | Journal article |
id | oxford-uuid:44bc74c1-6b0d-433a-a01e-6a0f1e4499ad |
institution | University of Oxford |
language | English |
last_indexed | 2024-03-06T21:31:12Z |
publishDate | 2017 |
publisher | Wiley |
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spelling | oxford-uuid:44bc74c1-6b0d-433a-a01e-6a0f1e4499ad2022-03-26T15:03:33ZWeak solutions for Euler systems with non-local interactionsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:44bc74c1-6b0d-433a-a01e-6a0f1e4499adEnglishSymplectic ElementsWiley2017Carrillo De La Plata, JFeireisl, EGwiazda, PSwierczewska-Gwiazda, AWe consider several modifications of the Euler system of fluid dynamics, including its pressureless variant driven by non-local interaction repulsive-attractive and alignment forces in the space dimension N = 2, 3. These models arise in the study of self-organization in collective behavior modeling of animals and crowds. We adapt the method of convex integration to show the existence of infinitely many global-in-Time weak solutions for any bounded initial data. Then we consider the class of dissipative solutions satisfying, in addition, the associated global energy balance (inequality).We identify a large set of initial data for which the problem admits infinitely many dissipative weak solutions. Finally, we establish a weak-strong uniqueness principle for the pressure-driven Euler system with non-local interaction terms as well as for the pressurelesssystem with Newtonian interaction. |
spellingShingle | Carrillo De La Plata, J Feireisl, E Gwiazda, P Swierczewska-Gwiazda, A Weak solutions for Euler systems with non-local interactions |
title | Weak solutions for Euler systems with non-local interactions |
title_full | Weak solutions for Euler systems with non-local interactions |
title_fullStr | Weak solutions for Euler systems with non-local interactions |
title_full_unstemmed | Weak solutions for Euler systems with non-local interactions |
title_short | Weak solutions for Euler systems with non-local interactions |
title_sort | weak solutions for euler systems with non local interactions |
work_keys_str_mv | AT carrillodelaplataj weaksolutionsforeulersystemswithnonlocalinteractions AT feireisle weaksolutionsforeulersystemswithnonlocalinteractions AT gwiazdap weaksolutionsforeulersystemswithnonlocalinteractions AT swierczewskagwiazdaa weaksolutionsforeulersystemswithnonlocalinteractions |