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Volumn 93, Issue 10, 2008, Pages

Spectral bandwidth and phase effects of resonantly excited ultrafast surface plasmon pulses

Author keywords

[No Author keywords available]

Indexed keywords

PHASE INTERFACES; PHOTONS; PLASMONS; SURFACE PLASMON RESONANCE; TELECOMMUNICATION SYSTEMS; ULTRAFAST PHENOMENA;

EID: 51749083930     PISSN: 00036951     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.2978399     Document Type: Article
Times cited : (12)

References (18)
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    • Rokitski, R.1    Tetz, K.A.2    Fainman, Y.3
  • 10
    • 33847721110 scopus 로고    scopus 로고
    • 1530-6984 10.1021/nl0627846.
    • A. Kubo, N. Pontius, and H. Petek, Nano Lett. 1530-6984 10.1021/nl0627846 7, 470 (2007).
    • (2007) Nano Lett. , vol.7 , pp. 470
    • Kubo, A.1    Pontius, N.2    Petek, H.3
  • 11
    • 28044445190 scopus 로고
    • 0044-3328 10.1007/BF01395428.
    • E. Kretschmann, Z. Phys. 0044-3328 10.1007/BF01395428 241, 313 (1971).
    • (1971) Z. Phys. , vol.241 , pp. 313
    • Kretschmann, E.1
  • 12
    • 46249128090 scopus 로고    scopus 로고
    • 1367-2630 10.1088/1367-2630/10/2/025031.
    • M. I. Stockman, New J. Phys. 1367-2630 10.1088/1367-2630/10/2/025031 10, 025031 (2008).
    • (2008) New J. Phys. , vol.10 , pp. 025031
    • Stockman, M.I.1
  • 14
    • 51749083017 scopus 로고    scopus 로고
    • The reflectivity was calculated for -polarized light at the center photon energy of the excitation pulse.
    • The reflectivity was calculated for p -polarized light at the center photon energy of the excitation pulse.
  • 15
    • 51749083468 scopus 로고    scopus 로고
    • For the calculations we considered nprism =1.52 independent of the wavelength, since the spectral bandwidth is rather insensitive to nprism.
    • For the calculations we considered nprism =1.52 independent of the wavelength, since the spectral bandwidth is rather insensitive to nprism.
  • 17
    • 51749118466 scopus 로고    scopus 로고
    • The phase of the reflection in the TIR configuration is wavelength independent at θSPP, since θSPP is significantly larger than the critical angle for TIR. A small difference in optical path length between the SPP and TIR configurations led to a linear spectral phase difference that we subtracted.
    • The phase of the reflection in the TIR configuration is wavelength independent at θSPP, since θSPP is significantly larger than the critical angle for TIR. A small difference in optical path length between the SPP and TIR configurations led to a linear spectral phase difference that we subtracted.


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