<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OPJ</journal-id><journal-title-group><journal-title>Optics and Photonics Journal</journal-title></journal-title-group><issn pub-type="epub">2160-8881</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/opj.2017.78B013</article-id><article-id pub-id-type="publisher-id">OPJ-78298</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Chemistry&amp;Materials Science</subject><subject> Engineering</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Ultra-High Specific Absorption of Metallic Binary-Groove Gratings
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yutong</surname><given-names>Li</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yumin</surname><given-names>Liu</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>State Key Laboratory of Information Photonics and Optical Communications, Beijing University of Posts and 
Telecommunications, Beijing, China</addr-line></aff><pub-date pub-type="epub"><day>10</day><month>08</month><year>2017</year></pub-date><volume>07</volume><issue>08</issue><fpage>92</fpage><lpage>98</lpage><history><date date-type="received"><day>June</day>	<month>27,</month>	<year>2017</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>August</month>	<year>7,</year>	</date><date date-type="accepted"><day>August</day>	<month>10,</month>	<year>2017</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  
    A metallic binary-groove gratings, which can be exploited to absorb light at C-band and sense materials with refractive index (1.0 - 1.2), is proposed and investigated numerically. Both ultra-high absorption (99.937%) and sensitivity (1600 nm/RIU) are achieved. 
  
 
</p></abstract><kwd-group><kwd>Surface Plasmon</kwd><kwd> Absorption</kwd><kwd> Gratings</kwd><kwd> Sensing</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The surface plasmon polaritons (SPPs), which is an evanescent wave propagating along metal-insulator interface with extremely confined mode area, can be effectively excited by an applied electromagnetic wave. Recently, a great many of the SPPs-based devices have been extensively designed for applications in nanophotonic circuits, optical communication, solar cells and bio-sensors, etc. The structure for SPPs exciting has been a hot topic in last few decades. Among the investigations, periodic metallic gratings are considered as one of the common structures for transferring the energy of incident wave to SPPs. Much related work has been done to investigate effective index, propagation length and energy absorption [<xref ref-type="bibr" rid="scirp.78298-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.78298-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.78298-ref3">3</xref>]. However, the present results mainly focus on theoretical features rather than practical applications.</p><p>In this paper, a structure of periodic binary grooves is proposed. Due to the coupling of the modes in two grooves, complete absorption peak of an incident wavelength at C-band (1550 nm here) is realized by silver-based structure. The required wavelength can be manipulated by varying optical properties of the structure and materials (silver, gold, aluminum). In addition, the sensing characteristic is also calculated about the proposed structure. We use commercial software COMSOL Multiphysics 5.2.</p></sec><sec id="s2"><title>2. Model Structure</title><p>The resonant absorption behavior is strongly depending on geometric parameters, including width and depth of grooves and spacing distance [<xref ref-type="bibr" rid="scirp.78298-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.78298-ref5">5</xref>]. The two grooves separated from each other with spacing a have and w<sub>2</sub> in width, d<sub>1</sub> and d<sub>2</sub> in depth, respectively. Considering designing a perfect absorber, we set the thickness of Ag as 800 nm that is enough for blocking light transmission. Notice that, the whole structure is considered to be infinite in z-axis and solved by finite element method (FEM) in our simulation. We use metal silver first because of its low optical loss and excellent plasmonic behavior. The electric permittivity of Ag is given by the following (1) Drude model,</p><disp-formula id="scirp.78298-formula71"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/78298x2.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x3.png" xlink:type="simple"/></inline-formula> is the angular frequency, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x4.png" xlink:type="simple"/></inline-formula>is the plasma frequency, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x5.png" xlink:type="simple"/></inline-formula>is a corrective constant that accounts for the background electron screening at high frequency, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x6.png" xlink:type="simple"/></inline-formula> is the electron scattering frequency.</p></sec><sec id="s3"><title>3. Simulation Results</title><p><xref ref-type="fig" rid="fig2">Figure 2</xref> shows the calculated spectral properties of reflectance, transmittance and absorbance for the AS structure. In addition, perfect narrow band absorption occurs at 1550 nm. The two grooves in one period are designed with different values of depth, so that two different cavity modes can be created for coupling. The absorbance is defined as</p><disp-formula id="scirp.78298-formula72"><graphic  xlink:href="http://html.scirp.org/file/78298x7.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x8.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x9.png" xlink:type="simple"/></inline-formula> are transmittance and reflectance, respectively. The distributions of normalized electric field and power flow obtained by silver-based gratings are shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>(b). As we can see, the strongest localized field appears at the outer edge corners and their spacing region. The incident TM-polarized wave is efficiently coupled into both grooves.</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> The schematic diagram of the proposed binary grooves-based metallic gratings</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/78298x10.png"/></fig><fig-group id="fig2"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> (a) Calculated reflectivity, transmission and absorption spectra of the AS struc- ture; (b) The normalized electric field and power flow of the metallic gratings.</title></caption><fig id ="fig2_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/78298x11.png"/></fig><fig id ="fig2_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/78298x12.png"/></fig></fig-group><p>Except for the C-band absorber at 1550 nm, another application of the proposed structure is sensing refractive index of material under detecting. As is shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>(a), five resonant peaks are presented with refractive index changing from 1.0 to 1.2 (an increment of 0.05). Notice that, the materials are filled in the whole region except metal. After calculation, the sensitivity about 1600 nm/RIU is achieved.</p><p>As it depicts in <xref ref-type="fig" rid="fig3">Figure 3</xref>(b), with the refractive index changed from 1.1 to 1.2, the peak has a red shift from about 1550 nm to 1870 nm. The metallic binary- groove structure has a favored linear characteristic. The full wave at half maximum (FWHM) of the peaks are getting wider with the increasing refractive index which can be seen in <xref ref-type="fig" rid="fig3">Figure 3</xref>(c).</p><fig-group id="fig3"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> (a) The reflectance spectrum versus incident wavelength for refractive index varying from 1.00 to 1.20; (b) The linear relation of peak position; (c) The FWHM versus refractive index.</title></caption><fig id ="fig3_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/78298x13.png"/></fig><fig id ="fig3_2"><label>(c)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/78298x14.png"/></fig><fig id ="fig3_3"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/78298x15.png"/></fig></fig-group></sec><sec id="s4"><title>4. Analysis and Applications</title><p>The study on the optical properties of the absorber is investigated. The reflectance dip varied with different w which means the best absorber can be fixed at a value of 1111. The depths of two grooves have effect on the interaction which finally influence the absorption rate at a certain wavelength, such as 1550 nm. Besides, the absorber should work over a wide range of incident angle for practical application. The absorption property of our plasmonic absorber with the same geometric parameters as <xref ref-type="fig" rid="fig3">Figure 3</xref> in terms of the indent angle ranging from 0˚ to 40˚ for TM polarization was investigated by utilizing FEM, and the corresponding absorption spectra was illustrated in <xref ref-type="fig" rid="fig4">Figure 4</xref>. It is found that the absorption spectrum is nearly insensitive to the change of the incident angle. This can be explained in this way: for the TM polarization, the magnetic field of the incident light is always perpendicular to the incident plane with various incident angles and it can efficiently drive the circulating currents at large angles of incidence. Therefore, the absorption peak is nearly independent of the incident angle and it keeps more than 97% even at 40˚. In addition, the comparison of different metals is necessary in practical application. Firstly, metals can give rise to different absorption behaviors of the structures due to their different relative dielectric constants [<xref ref-type="bibr" rid="scirp.78298-ref6">6</xref>]. Secondly, the fabrication cost of metal is another important factor should be taken into consideration. Therefore, metals of silver, gold and aluminum are compared when we trying to obtain the reflectance dip (minimum) at wavelength 1550 nm. In order to ensure full absorption at 1550 nm under these kinds of metal, corresponding structural parameters (a, d and w) are optimized.</p><p>The reflectance spectrums obtained by the silver, gold and aluminum-based structure are shown in Figures 5(a)-(c), respectively. As it can be seen clearly, both silver and gold ensure a precise reflectance minimum of 0.08 and 0.063 at</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> The absorption property of our plasmonic absorber as a function of wavelength for various incident angles for TM polarization. The geometric parameters are the same as those in <xref ref-type="fig" rid="fig1">Figure 1</xref></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/78298x16.png"/></fig><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> The reflectance of the structure with different type of metal. (a) silver; (b) gold and (c) aluminum. The electric field of the structure when the metal is silver. (a) <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x18.png" xlink:type="simple"/></inline-formula>= 200 nm, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x19.png" xlink:type="simple"/></inline-formula>= 170 nm, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x20.png" xlink:type="simple"/></inline-formula>= 60 nm; a = 9.25 nm; (b) <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x21.png" xlink:type="simple"/></inline-formula>= 200 nm, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x22.png" xlink:type="simple"/></inline-formula>= 130 nm, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x23.png" xlink:type="simple"/></inline-formula>= 60 nm; a = 6.05 nm; (c) <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x24.png" xlink:type="simple"/></inline-formula>= 240 nm, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x25.png" xlink:type="simple"/></inline-formula>= 160 nm, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/78298x26.png" xlink:type="simple"/></inline-formula>= 60 nm; a = 4.9 nm</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/78298x17.png"/></fig><p>1550 nm, respectively. When the metal of aluminum is used, a reflectance minimum of 0.0845 is obtained. In the meantime, another minimum of 0.078 is obtained at 1539 nm. In general, a reflectance minimum of 0.063, or an absorption maximum of 99.937%, obtained by gold is the most desired value, despite the metal fabrication cost.</p><p>Based on the above analysis, the structures made by gold and aluminum show better robustness than by silver. Regardless of the fabrication cost in practical, gold is the first choice. However, aluminum becomes an alternative for its low production cost.</p></sec><sec id="s5"><title>5. Conclusion</title><p>In a summary, we propose and investigate metallic binary-groove gratings, which can achieve ultra-high absorption at C-band with silver, gold and aluminum and is nearly independent of the incident angle. As the most commonly used operating wavelength in optical communication, 1550 nm is captured more precisely by the gold gratings. Besides, the robustness of our structure is analyzed by calculating the error tolerance rate. At last, another application acting as a refractive index sensor is proposed and analyzed.</p></sec><sec id="s6"><title>Acknowledgements</title><p>This work was supported by the national natural science foundation of China (Grants No. 61275201 and No. 61372037).</p></sec><sec id="s7"><title>Cite this paper</title><p>Li, Y.T. and Liu, Y.M. (2017) Ultra-High Specific Absorption of Metallic Binary-Groove Gratings. Optics and Photonics Journal, 7, 92-98. https://doi.org/10.4236/opj.2017.78B013</p></sec></body><back><ref-list><title>References</title><ref id="scirp.78298-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Bozhevolnyi, S.I., Volkov, V.S., Devaux, E. and Ebbesen, T.W. (2005) Channel Plasmon-Polariton Guiding by Subwavelength Metal Grooves. 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