Lecture 16, 18.376, Tue Apr 11, 2023. Summary % Continue with Quasi-Modes; and finish section 3 "Wave equation in an interval: Dirichlet/Radiation BC (example 3)" of the notes: Examples of pde with the Laplace Transform. Point out how the poles of the Green's function that give rise to the "spectral decomposition" obtained in these notes [i.e.: equations (3.14) and (3.15)] are only accessible because we are looking at the problem in 0 < x < 1, with a radiation BC at x = 1. If the full 0 < x < infty interval is considered, the Green's function ceases to make sense for re(s) < 0 [same phenomena explained in prior lecture], and the poles cannot be accessed. Mention other similar examples, like quasi-modes in the atmosphere, if a radiation BC is imposed at the tropo-pause [much harder problem, but same mechanics]. At the lecture's end a question was asked about equations (3.14) and (3.15). Equations seem puzzling, since the alpha_n depend only on alpha = u(x, 0) and the beta_n only on beta = u_t(x, 0) yet u(x, t) depends on both ... even at t = 0. % % ========================================================================== NOTE: Here #nnn are references to the Lecture Points file. [PSQ] means Problem Set Question. The "lecture summaries and points" are NOT intended as study materials. The points purpose is explained in the "lecture points" file. The summaries are brief descriptions each lecture, used by the instructor to keep track of the material covered. They ARE *NOT* "lecture notes" to be used to study and/or replace attending the lectures, etc. They are provided for your convenience, as a help to organize your own notes. % ========================================================================== % EOF