dc.contributor.author | Horsley, SAR | |
dc.date.accessioned | 2019-12-02T15:17:52Z | |
dc.date.issued | 2019-11-11 | |
dc.description.abstract | At zero energy the difference in the number of spin-up and spin-down modes of the Dirac equation is determined by the topology of both space and the gauge field in which the system sits. Writing Maxwell's equations in a Dirac-like form, we identify cases where a combination of material parameters plays the role of "energy." At zero energy we thus find electromagnetic modes that are indifferent to local changes in the material parameters, with a dispersion relation depending only on the asymptotic values of the material parameters at infinity. We give several examples and show that this theory has implications for non-Hermitian media, where it can be used to construct permittivity profiles that are either reflectionless or act as coherent perfect absorbers or lasers. | en_GB |
dc.description.sponsorship | Royal Society (Charity) | en_GB |
dc.identifier.citation | Vol. 100; 053819 | en_GB |
dc.identifier.doi | 10.1103/PhysRevA.100.053819 | |
dc.identifier.uri | http://hdl.handle.net/10871/39911 | |
dc.language.iso | en | en_GB |
dc.publisher | American Physical Society | en_GB |
dc.title | Indifferent electromagnetic modes: Bound states and topology | en_GB |
dc.type | Article | en_GB |
dc.date.available | 2019-12-02T15:17:52Z | |
dc.identifier.issn | 2469-9926 | |
dc.description | This is the author accepted manuscript. The final version is available from the publisher via the DOI in this record | en_GB |
dc.identifier.journal | Physical Review A | en_GB |
dc.rights.uri | http://www.rioxx.net/licenses/all-rights-reserved | en_GB |
dcterms.dateAccepted | 2019-06-10 | |
exeter.funder | ::Royal Society (Charity) | en_GB |
rioxxterms.version | AM | en_GB |
rioxxterms.licenseref.startdate | 2019-11-11 | |
rioxxterms.type | Journal Article/Review | en_GB |
refterms.dateFCD | 2019-12-02T15:10:14Z | |
refterms.versionFCD | AM | |
refterms.dateFOA | 2019-12-02T15:17:55Z | |
refterms.panel | B | en_GB |