Abstract
Metallic films much thinner than the skin depth can support surface plasmon modes whose dispersion approaches the plasma frequency, giving rise to the so-called epsilon-near-zero mode. We analyse its features and observation conditions. © 2015 OSA.
| Original language | English |
|---|---|
| Title of host publication | Integrated Photonics Research, Silicon and Nanophotonics, IPRSN 2015 |
| Pages | 371p |
| Number of pages | 1 |
| DOIs | |
| State | Published - Jan 1 2015 |
| Externally published | Yes |
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