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University of Cambridge > Talks.cam > Isaac Newton Institute Seminar Series > Essential spectra and black hole modes for inhomogeneous, anisotropic dissipative Maxwell and Drude-Lorentz systems
Essential spectra and black hole modes for inhomogeneous, anisotropic dissipative Maxwell and Drude-Lorentz systemsAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact nobody. RNTW04 - Synergistic workshop on Rich and Nonlinear tomography aimed at drawing together all strands of both methods and applications with new insights The methods required to study spectral pollution for dissipative Maxwell and Drude-Lorentz systems turn out to be closely connected to the methods required to study the essential spectrum for such systems and are very different from the methods used for Schroedinger equations. The presence of dissipation, e.g. in the form of conductivity, means that the essential spectrum can be changed by changing the coefficients in the system on any arbitrarily small, non-empty open set. The proof of this result consists of a reduction of the system to a triangular block operator matrix, together with an analysis of quasi-modes associated with one of the diagonal blocks. In the case of conductivity discontinuous across an interface, additional modes arise whose rapid exponential decay away from the interface makes them effectively invisible at a distance – hence the name `black hole modes’. These modes have previously been observed by various authors for \div(p \grad) operators with sign-changing p, and may also occur in transmission eigenvalue problems. This talk describes joint work with various co-authors including Giovanni Alberti, Sabine Boegli, Francesco Ferraresso, Christiane Tretter, Ian Wood and the late Malcolm Brown. This talk is part of the Isaac Newton Institute Seminar Series series. This talk is included in these lists:
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