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. 2012 Nov 6;109(47):19093–19096. doi: 10.1073/pnas.1216407109

Fig. 3.

Fig. 3.

Power spectral density of buckled nanotube with ɛ0 = −4 × 10−3 with Fz = 0.6 pN at logarithmically spaced temperatures. The built-in intrinsic damping dominates the apparent line width at the lowest temperature. (Inset) Plot of Q−1 of the f3z mode. Simulation data are shown as red dots, and theoretical predictions from Eq. 3 are plotted as a blue line. Labels beneath each spectral line correspond to their expected origin.