Erratum: Quantitative modeling of fluorescent emission in photonic crystals (Physical Review B (2013) 88 (205118) DOI:10.1103/PhysRevB.88.205118);Quantitative modeling of fluorescent emission in photonic crystals

Physical Review B - Condensed Matter and Materials Physics

Volumn 88, Issue 20, 2013, Pages

  Gutmann, Johannes ^a   Zappe, Hans ^b   Goldschmidt, Jan Christoph ^a,c  

^a FRAUNHOFER INSTITUTE FOR SOLAR ENERGY SYSTEMS ISE   (Germany)

^b UNIVERSITY OF FREIBURG   (Germany)

^c IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 84890320045     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.88.239901     Document Type: Erratum

References (42)

1. E. M. Purcell, Phys. Rev. PHRVAO 0031-899X 10.1103/PhysRev.69.674 69, 674 (1946).
2. E. Yablonovitch, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett. 58.2059 58, 2059 (1987).
3. S. John, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.58.2486 58, 2486 (1987).
4. V. Bykov, Soviet Physics JETP 35, 269 (1972).
5. J. P. Dowling and C. M. Bowden, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.46.612 46, 612 (1992).
6. K. Busch and S. John, Phys. Rev. E 1063-651X 10.1103/PhysRevE.58.3896 58, 3896 (1998).
7. R. Wang, X.-H. Wang, B.-Y. Gu, and G.-Z. Yang, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.67.155114 67, 155114 (2003).
8. M. Barth, A. Gruber, and F. Cichos, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.72.085129 72, 085129 (2005).
9. I. S. Nikolaev, W. L. Vos, and A. F. Koenderink, J. Opt. Soc. Am. B JOBPDE 0740-3224 10.1364/JOSAB.26.000987 26, 987 (2009).
10. R. C. McPhedran, L. C. Botten, J. McOrist, A. A. Asatryan, C. M. de Sterke, and N. A. Nicorovici, Phys. Rev. E PLEEE8 1539-3755 10.1103/PhysRevE.69. 016609 69, 016609 (2004).
11. D. P. Fussell, R. C. McPhedran, and C. Martijn de Sterke, Phys. Rev. E PLEEE8 1539-3755 10.1103/PhysRevE.70.066608 70, 066608 (2004).
12. S. J. Myers, D. P. Fussell, J. M. Dawes, E. Mägi, R. C. McPhedran, B. J. Eggleton, and C. M. de Sterke, Opt. Express OPEXFF 1094-4087 10.1364/OE.14.012439 14, 12439 (2006).
13. W. L. Vos, A. F. Koenderink, and I. S. Nikolaev, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.80.053802 80, 053802 (2009).
14. E. V. Hooijdonk, S. Berthier, and J.-P. Vigneron, J. Appl. Phys. 0021-8979 10.1063/1.4768896 112, 114702 (2012).
15. E. V. Hooijdonk, C. Barthou, J. P. Vigneron, and S. Berthier, J. Opt. Soc. Am. B JOBPDE 0740-3224 10.1364/JOSAB.29.001104 29, 1104 (2012).
16. P. Bermel, A. Rodriguez, J. D. Joannopoulos, and M. Soljacic, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.99.053601 99, 053601 (2007).
17. B. Herter, S. Wolf, S. Fischer, J. Gutmann, B. Bläsi, and J. C. Goldschmidt, Opt. Express OPEXFF 1094-4087 10.1364/OE.21.00A883 21, A883 (2013).
18. M. J. A. de Dood, A. Polman, and J. G. Fleming, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.67.115106 67, 115106 (2003).
19. S. G. Romanov, A. V. Fokin, and R. M. D. L. Rue, Appl. Phys. Lett. APPLAB 0003-6951 10.1063/1.126126 76, 1656 (2000).
20. M. Megens, J. E. G. J. Wijnhoven, A. Lagendijk, and W. L. Vos, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.59.4727 59, 4727 (1999).
21. E. P. Petrov, V. N. Bogomolov, I. I. Kalosha, and S. V. Gaponenko, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.81.77 81, 77 (1998).
22. P. Lodahl, A. Floris van Driel, I. S. Nikolaev, A. Irman, K. Overgaag, D. Vanmaekelbergh, and W. L. Vos, Nature (London) NATUAS 0028-0836 10.1038/nature02772 430, 654 (2004).
23. J. Li, B. Jia, G. Zhou, C. Bullen, J. Serbin, and M. Gu, Adv. Mater. ADVMEW 0935-9648 10.1002/adma.200602054 19, 3276 (2007).
24. M. R. Jorgensen, J. W. Galusha, and M. H. Bartl, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.107.143902 107, 143902 (2011).
25. M. D. Leistikow, A. P. Mosk, E. Yeganegi, S. R. Huisman, A. Lagendijk, and W. L. Vos, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.107.193903 107, 193903 (2011).
26. S. Ogawa, M. Imada, S. Yoshimoto, M. Okano, and S. Noda, Science SCIEAS 0036-8075 10.1126/science.1097968 305, 227 (2004).
27. P. Vukusic and I. Hooper, Science SCIEAS 0036-8075 10.1126/science. 1116612 310, 1151 (2005).
28. J. Gutmann, J. Posdziech, M. Peters, L. Steidl, R. Zentel, H. Zappe, and J. C. Goldschmidt, Proc. SPIE PSISDG 0277-786X 10.1117/12.922681 8438, 84381O (2012).
29. J. D. Joannopoulos, S. G. Johnson, J. N. Winn, and R. D. Meade, Photonic Crystals - Molding the Flow of Light, 2nd ed. (Princeton University Press, Princeton, New Jersey, 2008).
30. S. G. Johnson and J. D. Joannopoulos, Opt. Express OPEXFF 1094-4087 10.1364/OE.8.000173 8, 173 (2001).
31. G. Lehmann and M. Taut, Phys. Status Solidi B PSSBBD 0370-1972 10.1002/pssb.2220540211 54, 469 (1972).
32. J. Hama, M. Watanabe, and T. Kato, J. Phys.: Condens. Matter JCOMEL 0953-8984 10.1088/0953-8984/2/36/007 2, 7445 (1990).
33. See Supplemental Material at http://link.aps.org/supplemental/10.1103/ PhysRevB.88.205118 for additional information about the LDOS in homogenous media, further (L)DOS results, the effects of the LDOS on the line shape of individual transitions and fractional transition rates.
34. In contrast, the LDOS within the voids (low permittivity) is strongly enhanced over its corresponding homogeneous LDOS, and the total DOS is, apart from band gaps, in good agreement with the DOS for an effective homogeneous material, as shown in Supplemental Material.
35. J. Lakowicz, Principles of Fluorescence Spectroscopy (Springer, London, 2009).
36. K. Yee, IEEE Trans. Antennas Propag. 0018-926X 10.1109/TAP.1966.1138693 14, 302 (1966).
37. A. Taflove and S. C. Hagness, Computational Electrodynamics: The Finite-Difference Time-Domain Method, 3rd ed. (Artech House, Norwood, MA, 2005).
38. M. G. Moharam and T. K. Gaylord, J. Opt. Soc. Am. JOSAAH 0030-3941 10.1364/JOSA.72.001385 72, 1385 (1982).
39. D. M. Whittaker and I. S. Culshaw, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.60.2610 60, 2610 (1999).
40. M. Fox, Quantum Optics (Oxford University Press, New York, NY, USA, 2006).
41. For the calculation of the opal FLDOS, we increased the resolution of the grid in k space to Δ k = 0.005 2 π / a to reduce binning noise. At the same time, we restricted the calculation to 1/8 of the FBZ to keep the computational effort reasonable.
42. F. L. Arbeloa, P. R. Ojeda, and I. L. Arbeloa, J. Lumin. JLUMA8 0022-2313 10.1016/0022-2313(89)90027-6 44, 105 (1989).