2018
DOI: 10.1007/s00033-018-0938-5
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Global, finite energy, weak solutions for the NLS with rough, time-dependent magnetic potentials

Abstract: We prove the existence of weak solutions in the space of energy for a class of non-linear Schrödinger equations in the presence of a external, rough, time-dependent magnetic potential. Under our assumptions it is not possible to study the problem by means of usual arguments like resolvent techniques or Fourier integral operators, for example. We use a parabolic regularisation and we solve the approximating Cauchy problem. This is achieved by obtaining suitable smoothing estimates for the dissipative evolution.… Show more

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Cited by 5 publications
(3 citation statements)
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References 43 publications
(75 reference statements)
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“…3 is a weak solution to (1.1). By means of Proposition 3.4, we have also that à ∈ W 1,6 T L 3 . Therefore, after choosing T possibly smaller (depending on R 1 , R 2 ), we have (ũ, Ã) ∈ Z, whence (ũ, Ã) = (u, A).…”
Section: As a Consequence Of Lemma 43 We Can Define Formentioning
confidence: 80%
See 1 more Smart Citation
“…3 is a weak solution to (1.1). By means of Proposition 3.4, we have also that à ∈ W 1,6 T L 3 . Therefore, after choosing T possibly smaller (depending on R 1 , R 2 ), we have (ũ, Ã) ∈ Z, whence (ũ, Ã) = (u, A).…”
Section: As a Consequence Of Lemma 43 We Can Define Formentioning
confidence: 80%
“…Altough magnetic Strichartz estimates are well understood for time independent potentials [13,14,15,16,17] (see also [37] and references therein), in the time dependent case much less is known, and the only results available require the smallness of suitable scale invariant space-time norms [19,48]. In particular, even for a non-linear Schrödinger equation with a given external time dependent magnetic potential, the well-posedness in the energy space is in general an open question (global existence of weak solutions can be proved using the method of parabolic regularization [6]). Concerning the Maxwell-Schrödinger system with focusing non-linearities, one can also study the existence and stability of standing waves, see for instance [12] and references therein.…”
Section: Introductionmentioning
confidence: 99%
“…Our second main focus concerns the local and global well-posedness of (1.12) in the energy space. This field is under a comprehensive and well-established control in the classical, unperturbed case α = ∞, including also when (1.12) contains much more singular and non-symmetric convolution potentials, together with electric and magnetic potentials, possibly depending on time (see, e.g., [21,45,12] and the references therein).…”
Section: Strictly Positive and Strictly Radially Decreasing;mentioning
confidence: 99%