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dc.contributor.authorHorsley, SAR
dc.contributor.authorLonghi, S
dc.date.accessioned2017-08-29T11:52:17Z
dc.date.issued2017-08-17
dc.description.abstractReflectionless potentials for classical or matter waves represent an important class of scatteringless systems encountered in different areas of physics. Here we mathematically demonstrate that there is a family of non-Hermitian potentials that, in contrast to their Hermitian counterparts, remain reflectionless even when deformed in space or time. These are the profiles that satisfy the spatial Kramers-Kronig relations. We start by considering scattering of matter waves for the Schrödinger equation with an external field, where a moving potential is observed in the Kramers-Henneberger reference frame. We then generalize this result to the case of electromagnetic waves, by considering a slab of reflectionless material that both is scaled and has its center displaced as an arbitrary function of position. We analytically and numerically demonstrate that the backscattering from these profiles remains zero, even for extreme deformations. Our results indicate the supremacy of non-Hermitian Kramers-Kronig potentials over reflectionless Hermitian potentials in keeping their reflectionless property under deformation and could find applications to, e.g., reflectionless optical coatings of highly deformed surfaces based on perfect absorption.en_GB
dc.description.sponsorshipS.A.R.H. acknowledges financial support through a Royal Society TATA University Research Fellowship (Grant No. RPG-2016-186).en_GB
dc.identifier.citationVol. 96, article 023841en_GB
dc.identifier.doi10.1103/PhysRevA.96.023841
dc.identifier.urihttp://hdl.handle.net/10871/29098
dc.language.isoenen_GB
dc.publisherAmerican Physical Societyen_GB
dc.rights© 2017 American Physical Society
dc.titleSpatiotemporal deformations of reflectionless potentialsen_GB
dc.typeArticleen_GB
dc.date.available2017-08-29T11:52:17Z
dc.identifier.issn1050-2947
dc.descriptionThis is the author accepted manuscript. The final version is available from American Physical Society via the DOI in this record.en_GB
dc.identifier.journalPhysical Review Aen_GB


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