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Refractive index sensing based on surface plasmon-coupled emission excited by reverse Kretschmann or Tamm structure

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Abstract

Surface plasmon coupled emission (SPCE) is the directional emission of surface plasmon polaritons (SPPs) through the reverse channels of focused surface plasmon excitation to the far field, which has shown significant possibilities in bioanalysis, medical diagnosis, and so on. We carried out a theoretical study of SPCE to analyze its mechanisms and proposed a new structure to improve the emission intensity of SPCE. We proposed a method for refractive index sensing based on SPCE, consisting of a reverse Kretschmann (RK) or a Tamm structure for the first time, to the best of our knowledge. The corresponding sensing sensitivity reaches 87.61 deg/RIU and 67.44 deg/RIU, respectively. Compared with that in the RK, the far-field radiation intensity of SPCE in the Tamm structure is enhanced by two orders of magnitude. Furthermore, compared with surface plasmon resonance (SPR) sensing, SPCE sensing can improve the signal-to-noise ratio (SNR) and excitation efficiency. Our structures enable refractive index sensing with a high SNR, high spatial resolution, and without the requirement of angular alignment using complex mechanics, which are suitable for practical applications such as quantitative biomolecular detection and medical diagnosis.

© 2022 Optica Publishing Group

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Supplementary Material (5)

NameDescription
Supplement 1       The content of this document includes the use of practical light sources such as focused radially, linearly, and circularly beams to simulate the excitation process of SPCE.
Visualization 1       The emission process of SPCE under reverse Kretschmann structure when the time changes from 0 to 11 seconds
Visualization 2       At the bottom of the reverse Kretschmann structure, the SPCE bright ring slowly grows larger when the refractive index changes from 1 to 1.1
Visualization 3       The emission process of SPCE under Tamm structure when the time changes from 0 to 11 seconds
Visualization 4       At the bottom of the Tamm structure, the SPCE bright ring slowly grows larger when the refractive index changes from 1 to 1.1

Data availability

Data underlying the results presented in this paper are not publicly available at this time but may be obtained from the authors upon reasonable request.

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