dc.creatorBonheure, Denis
dc.creatorCasteras, Jean Baptiste
dc.creatorRoman, Carlos
dc.date.accessioned2024-01-10T13:10:17Z
dc.date.accessioned2024-05-02T20:20:13Z
dc.date.available2024-01-10T13:10:17Z
dc.date.available2024-05-02T20:20:13Z
dc.date.created2024-01-10T13:10:17Z
dc.date.issued2021
dc.identifier10.1007/s00526-021-02081-8
dc.identifier1432-0835
dc.identifier0944-2669
dc.identifierhttps://doi.org/10.1007/s00526-021-02081-8
dc.identifierhttps://repositorio.uc.cl/handle/11534/77823
dc.identifierWOS:000685965500003
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9273940
dc.description.abstractWe consider the boundary value problem
dc.description.abstract{-Delta u + u - lambda e(u) = 0 ,u > 0 in B-1(0)
dc.description.abstractpartial derivative(nu)u = 0 on partial derivative B-1(0),
dc.description.abstractwhose solutions correspond to steady states of the Keller-Segel system for chemotaxis. Here B-1(0) is the unit disk,. the outer normal to partial derivative B-1(0), and lambda > 0 is a parameter. We show that, provided lambda is sufficiently small, there exists a family of radial solutions u(lambda) to this system which blow up at the origin and concentrate on partial derivative B-1(0), as lambda -> 0. These solutions satisfy
dc.description.abstractlim(lambda -> 0) u lambda(0)/vertical bar in lambda vertical bar = 0 and 0 lim(lambda -> 0) 1/vertical bar in lambda vertical bar integral(B1(0)) (lambda eu lambda(x)) dx < infinity,
dc.description.abstracthaving in particular unbounded mass, as lambda -> 0.
dc.languageen
dc.publisherSPRINGER HEIDELBERG
dc.rightsacceso restringido
dc.subjectSTATIONARY SOLUTIONS
dc.subjectSTEADY-STATES
dc.subjectSYSTEM
dc.titleUnbounded mass radial solutions for the Keller-Segel equation in the disk
dc.typeartículo


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