corner
corner

Phys. Rev. B 78, 035403 (2008) [12 pages]

From slow to superluminal propagation: Dispersive properties of surface plasmon polaritons in linear chains of metallic nanospheroids

Download: PDF (1,111 kB) Buy this article Export: BibTeX or EndNote (RIS)

Alexander A. Govyadinov1,* and Vadim A. Markel2,1,†
1Department of Bioengineering, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
2Department of Radiology, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA

Received 19 July 2007; revised 20 May 2008; published 2 July 2008

We consider propagation of surface plasmon polaritons (SPPs) in linear periodic chains (LPCs) of prolate and oblate metallic spheroids. We show that the SPP group velocity can be efficiently controlled by varying the aspect ratio of the spheroids. For sufficiently small aspect ratios, a gap appears in the first Brillouin zone of the chain lattice in which propagating modes do not exist. Depending on the SPP polarization, the gap extends to certain intervals of the Bloch wave number q. Thus, for transverse polarization, no propagating SPPs exist with wave numbers q such that qc<|q|<π/h, h being the chain period. For longitudinally polarized SPPs, the gap spans the interval |q|<qc. Here qc and qc are different constants, which depend on the chain parameters, spheroid aspect ratio, and its orientation with respect to the chain axis. The dependence of the dispersion curves on the spheroid aspect ratio leads to a number of interesting effects. In particular, bandwidth of SPPs that can propagate in an LPC can be substantially increased by utilizing prolate or oblate spheroids. When q is close to a critical value, so that |qqc|⪡π/h or |qqc|⪡π/h, the decay length of the SPPs is dramatically increased. In addition, the dispersion curves acquire a very large positive or negative slope. This can be used to achieve superluminal group velocity for realistic chain parameters. We demonstrate superluminal propagation of Gaussian wave packets in numerical simulations. Both theory and simulations are based on Maxwell equations with account of retardation and, therefore, are fully relativistic.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.78.035403
DOI:
10.1103/PhysRevB.78.035403
PACS:
73.20.Mf, 71.20.Tx

*algov@seas.upenn.edu

vmarkel@mail.med.upenn.edu.