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VOLUME 87, NUMBER 17 P H Y S I ...
https://www.np.phy.cam.ac.uk/system/files/documents/prl01-photonicmetal.pdfi Hkma ki aJki a0 mJkia kmaHkma0,(1). where J and H are spherical Bessel and Hankel func-tions, and the prime denotes differentiation with respectto the argument ka. -
Using APL format
https://www.np.phy.cam.ac.uk/system/files/documents/apl00-pbg-gaps.pdfSaand S. Kawakami, Phys. Rev. B58, R100961998!; H. Kosaka, T. Ka-washima, A. -
Using APL format
https://www.np.phy.cam.ac.uk/system/files/documents/apl00-pbg-gaps_0.pdfSaand S. Kawakami, Phys. Rev. B58, R100961998!; H. Kosaka, T. Ka-washima, A. -
Synchronization crossover of polariton condensates in weakly…
https://www.np.phy.cam.ac.uk/system/files/documents/PRB18_condensatelattice.pdf8). From Eq. (B5), we can see that the first intensityminimum occurs at ka = 2π/N. -
Spatiotemporal Dynamics and Control of Strong Coupling in Plasmonic…
https://www.np.phy.cam.ac.uk/system/files/documents/acsphotonics.7b00437.pdfKA KA. K A A. [( )( ) ][( )( ) ]. 0. QE 1 11 QE 2 22. 212 21 (2). where ΩQE = ω12 iγ12 is the complex frequency of thetwo-level electronic transition with ω12 being ... KA KA. K A A. [( )( ) ][( )( ) ]. 0. QE 1 11 QE 2 22. 212 21 (9). For a system -
RSC_CP_C0CP00071J 10429..10433
https://www.np.phy.cam.ac.uk/system/files/documents/pccp10-cb-sers.pdfThe association. constants (Ka) of their host–guest complexes are typically. several orders of magnitude higher than that of CDs. -
PHYSICAL REVIEW B 96, 155403 (2017) Driven-dissipative spin chain ...
https://www.np.phy.cam.ac.uk/system/files/documents/PhysRevB.96.155403.pdfMJ = cos (ka)2. J 0 0 00 J 0 00 0 J 00 0 0 J. -
PHYSICAL REVIEW B 96, 155403 (2017) Driven-dissipative spin chain ...
https://www.np.phy.cam.ac.uk/system/files/documents/copy_of_PhysRevB.96.155403.pdfMJ = cos (ka)2. J 0 0 00 J 0 00 0 J 00 0 0 J. -
PHYSICAL REVIEW B 85, 165422 (2012) Optical minibands in ...
https://www.np.phy.cam.ac.uk/system/files/documents/prb12-metallodielectric-minibands.pdf3(a)] and their momentum is. 0.04. 0.05. Fre. quen. cy (. ωa/. 2πc). 0 0.5 Wavevector (ka/π). 1 R. (b). 0.03. (a). ... be23. ω(k) = [1 κ cos(ka)], (1)where κ = β α is a tight-binding parameter that describesthe degree of coupling between two -
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https://www.np.phy.cam.ac.uk/system/files/documents/apl04-superprism.pdf3(b)] and third [Fig. 3(c)] Brillouinzones allows us to highlight the competition between theinput propagation direction ki and the strong diffractionfrom lattice vector G11 = ka , kb = / a , / b. ... mode. (b) and (c)Energy contour maps in the ka , kb
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