journal article·2018-02Open access

Optical Detection and Spatial Modulation of Mid‐Infrared Surface Plasmon Polaritons in a Highly Doped Semiconductor

Davide Maria Di Paola, Anton V. Velichko, Mario Bomers, Nilanthy Balakrishnan, Oleg Makarovsky, Mario Capizzi, Laurent Cerutti, Alexei N. Baranov, Manoj Kesaria, Anthony Krier, Thierry Taliercio, Amalia Patanè

Advanced Optical Materials· Volume 6· Issue 3

Abstract

Abstract Highly doped semiconductors (HDSCs) are promising candidates for plasmonic applications in the mid‐infrared (MIR) spectral range. This work examines a recent addition to the HDSC family, the dilute nitride alloy In(AsN). Postgrowth hydrogenation of In(AsN) creates a highly conducting channel near the surface and a surface plasmon polariton detected by attenuated total reflection techniques. The suppression of plasmonic effects following a photoannealing of the semiconductor is attributed to the dissociation of the NH bond. This offers new routes for direct patterning of MIR plasmonic structures by laser writing.
Source: crossref · Quality: baseline

Research context

OpenAlex topics: Plasmonic and Surface Plasmon Research · Gold and Silver Nanoparticles Synthesis and Applications · Thermal Radiation and Cooling Technologies

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

School of Physics and Astronomy The University of Nottingham Nottingham NG7 2RD UK

IES l'institut d'électronique Univ. Montpellier and CNRS UMR 5214 F‐34000 Montpellier France

Dipartimento di Fisica Sapienza Università di Roma Piazzale A. Moro 2 00185 Roma Italy

Physics Department Lancaster University Lancaster LA1 4YB UK

Funding

Engineering and Physical Sciences Research Council · H2020 European Research Council · Agence Nationale de la Recherche

References (45)

Show source-provided references
1. 10.1002/adma.20120507610.1002/adma.201205076 ↗
2. 10.1002/lpor.20090005510.1002/lpor.200900055 ↗
3. 10.1140/epjb/e2013-40039-x10.1140/epjb/e2013-40039-x ↗
4. Henini M. · 2002
5. 10.1063/1.494566710.1063/1.4945667 ↗
6. 10.1088/0957-4484/27/42/42520110.1088/0957-4484/27/42/425201 ↗
7. 10.1364/OE.19.01459410.1364/OE.19.014594 ↗
8. 10.1364/OE.24.01617510.1364/OE.24.016175 ↗
9. 10.1017/CBO978051159982810.1017/CBO9780511599828 ↗
10. 10.1088/0953-8984/14/34/20110.1088/0953-8984/14/34/201 ↗
11. 10.1063/1.8828810.1063/1.88288 ↗
12. Luz D. M. · J. Phys. C: Solid State Phys. · 1988 · 21 · 514910.1088/0022-3719/21/29/012 ↗
13. 10.1126/science.119825810.1126/science.1198258 ↗
14. 10.1002/pssr.20100426910.1002/pssr.201004269 ↗
15. 10.1016/j.metmat.2010.11.00110.1016/j.metmat.2010.11.001 ↗
16. 10.1038/nmat420310.1038/nmat4203 ↗
17. 10.1103/PhysRevLett.99.10740110.1103/PhysRevLett.99.107401 ↗
18. 10.1038/nmat203310.1038/nmat2033 ↗
19. 10.1364/OE.22.02429410.1364/OE.22.024294 ↗
20. 10.1117/1.JNP.9.09379110.1117/1.JNP.9.093791 ↗
21. 10.1143/JJAP.29.L69810.1143/JJAP.29.L698 ↗
22. 10.1364/OE.20.01215510.1364/OE.20.012155 ↗
23. 10.1063/1.212611710.1063/1.2126117 ↗
24. 10.1063/1.311723910.1063/1.3117239 ↗
25. 10.1103/PhysRevB.87.16520710.1103/PhysRevB.87.165207 ↗
26. 10.1063/1.490611110.1063/1.4906111 ↗
27. 10.1088/0268-1242/30/10/10503010.1088/0268-1242/30/10/105030 ↗
28. 10.1002/adfm.20110205310.1002/adfm.201102053 ↗
29. Ciatto G. · 201510.1201/b18296 ↗
30. Hamaguchi C. · 2006
31. Patanè A. · Phys. Rev. B · 2009 · 80 · 11520710.1103/PhysRevB.80.115207 ↗
32. Drachenko O. · Appl. Phys. Lett. · 2011 · 98 · 16210910.1063/1.3583378 ↗
33. 10.1007/0-387-37825-110.1007/0-387-37825-1 ↗
34. 10.1063/1.350914910.1063/1.3509149 ↗
35. We estimate the natural tilting of the epilayer by performing the ATR studies for different tilted angles of the sample relative to the horizontal support i.e. φ = 0° ±1° etc. Since in both the φ = 0° and φ = −1° configurations the ATR spectra are the same by taking into account that the Ge prism has a cylindrical symmetry we deduce that the natural tilting of the epilayer isφ*≈ 0.5°. From the diameter of the contact zone of the Ge prism dGe= 100 µm we thus estimate an air gap of up to ≈0.9 µm.
36. 10.1088/0034-4885/33/3/30710.1088/0034-4885/33/3/307 ↗
37. 10.1103/PhysRevLett.10.47110.1103/PhysRevLett.10.471 ↗
38. 10.1103/PhysRevLett.104.25680310.1103/PhysRevLett.104.256803 ↗
39. 10.1103/PhysRevLett.14.54910.1103/PhysRevLett.14.549 ↗
40. 10.1103/PhysRevLett.33.90810.1103/PhysRevLett.33.908 ↗
41. 10.1088/0268-1242/7/9/00210.1088/0268-1242/7/9/002 ↗
42. 10.1063/1.32426510.1063/1.324265 ↗
43. This large increase ofTis reached at relatively low powers due to the high absorption coefficient (α ≈ 107m−1at λ = 633 nm) and low thermal conductivity (K= 27 W m−1K−1atT= 300 K) of In(AsN).
44. 10.1103/PhysRev.123.156010.1103/PhysRev.123.1560 ↗
45. 10.1103/PhysRevB.27.98510.1103/PhysRevB.27.985 ↗