Threshold Behavior for Nonlinear Wave Equations
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Publication:2732450
DOI10.2991/jnmp.2001.8.s.7zbMath0980.35109OpenAlexW4251537652MaRDI QIDQ2732450
Publication date: 29 October 2001
Published in: Journal of Nonlinear Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.2991/jnmp.2001.8.s.7
Second-order nonlinear hyperbolic equations (35L70) Analyticity in context of PDEs (35A20) Initial value problems for second-order hyperbolic equations (35L15)
Related Items (10)
Dynamics near explicit stationary solutions in similarity variables for solutions of a semilinear wave equation in higher dimensions ⋮ High order variable mesh off-step discretization for the solution of 1-D non-linear hyperbolic equation ⋮ On blowup for the supercritical quadratic wave equation ⋮ Stable blowup for the cubic wave equation in higher dimensions ⋮ The blow-up rate for a non-scaling invariant semilinear wave equations in higher dimensions ⋮ Approximation of nonlinear wave equations with nonstandard anisotropic growth conditions ⋮ The blow-up rate for a non-scaling invariant semilinear wave equations ⋮ On the stability of the notion of non-characteristic point and blow-up profile for semilinear wave equations ⋮ The blow-up rate for strongly perturbed semilinear wave equations in the conformal regime without a radial assumption ⋮ Solution to the semilinear wave equation with a pyramid-shaped blow-up surface
Cites Work
- Blow-up of solutions of nonlinear wave equations in three space dimensions
- The formation of black holes and singularities in spherically symmetric gravitational collapse
- Long‐time behaviour of solutions of a system of nonlinear wave equations
- Weak solutions and development of singularities of the SU(2) σ‐model
- Bounded variation solutions of the spherically symmetric einstein‐scalar field equations
- Dispersion and collapse of wave maps
- Global existence of harmonic maps in minkowski space
- Critical phenomena in gravitational collapse
- Equivariant self-similar wave maps from Minkowski spacetime into 3-sphere
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