2018
DOI: 10.1007/s00220-018-3099-7
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Scattering in the Energy Space for Boussinesq Equations

Abstract: In this note we show that all small solutions in the energy space of the generalized 1D Boussinesq equation must decay to zero as time tends to infinity, strongly on slightly proper subsets of the space-time light cone. Our result does not require any assumption on the power of the nonlinearity, working even for the supercritical range of scattering. For the proof, we use two new Virial identities in the spirit of works [10,11]. No parity assumption on the initial data is needed.

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Cited by 15 publications
(18 citation statements)
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“…Consider now the weight function φ(x) := sech 6 x in (4.9). Then, (4.10) leads to the estimate (see [34] for similar results)…”
Section: )mentioning
confidence: 66%
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“…Consider now the weight function φ(x) := sech 6 x in (4.9). Then, (4.10) leads to the estimate (see [34] for similar results)…”
Section: )mentioning
confidence: 66%
“…We conjecture that decay to zero in the energy space should hold in any compact set. See also the works [5,34,26,21] for decay in extended regions of space which profit of internal directions for decay.…”
Section: )mentioning
confidence: 99%
See 1 more Smart Citation
“…The second problem for which interesting conclusions can be stated is a classic one-wave fluid model. In [41], the authors considered extending the previous results to the case of the good Boussinesq model in 1+1 dimensions,…”
Section: Introduction and Main Resultsmentioning
confidence: 99%
“…Note however that u seems not locally L 2 integrable in time. However, (1.14) shows that this norm indeed decays to zero in time (even if it is not integrable in time The techniques that we use to prove Theorem 1.2 are not new, and have been used to show decay for the Born-Infeld equation [2], the good Boussinesq system [24], the Benjamin-Bona-Mahony (BBM) equation [12], and more recently in the more complex abcd Boussinesq system [14,13]. In all these works, suitable virial functionals were constructed to show decay to zero in compact/not compact regions of space.…”
Section: 2mentioning
confidence: 99%