1997
DOI: 10.1006/jfan.1997.3131
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Weighted Estimates for the Helmholtz Equation and Some Applications

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Cited by 72 publications
(112 citation statements)
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“…For A = −∆ this is a classical result (see e.g. Agmon [1]); here we shall use a very precise version of the principle, due to Barcelo, Ruiz and Vega [4]. On the other hand, for the Dirac operator only a few results are available, which concern the case with a nonzero mass term (see [28], [42]).…”
Section: The Limiting Absorption Principlementioning
confidence: 99%
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“…For A = −∆ this is a classical result (see e.g. Agmon [1]); here we shall use a very precise version of the principle, due to Barcelo, Ruiz and Vega [4]. On the other hand, for the Dirac operator only a few results are available, which concern the case with a nonzero mass term (see [28], [42]).…”
Section: The Limiting Absorption Principlementioning
confidence: 99%
“…Remark 1.2. As an essential step in the proof of Theorem 1.1, we need to establish the limiting absorption principle (LAP) for the operator H. This is obtained in Section 3 through several steps: starting from the "weak" LAP of [4] for the free resolvent, we first prove a strong version of the LAP for the free operator in the weighted spaces…”
Section: Introductionmentioning
confidence: 99%
“…These three surfaces are model examples of hypersurfaces with curvature 4 , though of course the cone differs from the sphere and paraboloid in that it has one vanishing principal curvature. These three hypersurfaces also enjoy a large group of symmetries (the orthogonal group, the parabolic scaling and Gallilean groups, and the Poincare group, respectively).…”
Section: The Restriction Problemmentioning
confidence: 99%
“…For the PDE applications it is sometimes convenient to think of R n as a spacetime R n−1 × R := {(x, t) : x ∈ R n−1 , t ∈ R} (with the frequency space thus becoming spacetime frequency space {(ξ, τ ) : ξ ∈ R n−1 , τ ∈ R}), but we will avoid doing so here. 4 One could also consider cylinders such as S k−1 × R n−k ⊂ R n , but it turns out that the restriction theory for these surfaces is identical to that of the sphere S k−1 inside R k . 5 Indeed, it suffices for the weak-type estimate from L p (R n ) to L p,∞ (S; dσ) to fail.…”
Section: Restriction Estimates and Extension Estimatesmentioning
confidence: 99%
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