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Local polarization dynamics in ferroelectric materials

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Rep. Prog. Phys. 73 (2010) 056502<br />

S V Kal<strong>in</strong><strong>in</strong> et al<br />

Intensity, a.u.<br />

10 -1<br />

10 -2<br />

1 ms<br />

5 ms<br />

10 ms<br />

(1,1) Peak Intensity<br />

0.10<br />

0.05<br />

(f)<br />

0.005 0.010<br />

Wavevector, nm -1<br />

(g)<br />

0.00<br />

1 10<br />

Lock-<strong>in</strong> time constant, ms<br />

Figure 8. (a) Ideal image (writ<strong>in</strong>g signal) (top) and correspond<strong>in</strong>g FFT image (bottom) illustrat<strong>in</strong>g that all frequency components are<br />

present. PFM images (top) and diffractograms (bottom) acquired with (b) 0.5 ms, (c) 1 ms, (d) 5 ms and (e) 20 ms lock-<strong>in</strong> time constants.<br />

(f ) Wave-vector dependence of peak <strong>in</strong>tensity for time constant ( ) 1 ms, () 10 ms and () 5 ms. (g) Intensity of the (1 ,1) peak as a<br />

function of lock-<strong>in</strong> time constant. Reproduced from [197].<br />

assum<strong>in</strong>g the writ<strong>in</strong>g pattern is the ideal image. Hence, these<br />

def<strong>in</strong>itions provide a quantitative measure of the <strong>in</strong>formation<br />

transfer from the desired template pattern to the actual image of<br />

the result<strong>in</strong>g doma<strong>in</strong> structure, and thus describe the fidelity of<br />

<strong>ferroelectric</strong> data storage rather than read<strong>in</strong>g resolution per se.<br />

Complementary to diffractogram criterion, the PFM<br />

imag<strong>in</strong>g resolution <strong>in</strong> real space can be determ<strong>in</strong>ed from<br />

the measured width of the doma<strong>in</strong> wall between antiparallel<br />

doma<strong>in</strong>s. Given that the <strong>in</strong>tr<strong>in</strong>sic width of a <strong>ferroelectric</strong><br />

doma<strong>in</strong> wall is on the order of 1–2 unit cells (∼1 nm) [201],<br />

the typical effective doma<strong>in</strong> wall width observed <strong>in</strong> PFM<br />

is presently on the order of 5–50 nm and therefore reflects<br />

primarily the spatial resolution of the microscope. Due to the<br />

symmetry properties of the dielectric, elastic and piezoelectric<br />

constant tensors, the piezoelectric constants change sign across<br />

a 180 ◦ doma<strong>in</strong> wall, while the elastic and dielectric properties<br />

do not. Hence, the relationship between the 180 ◦ doma<strong>in</strong><br />

wall width and the resolution function can be established from<br />

equation (2.6), where, after normalization, the doma<strong>in</strong> wall<br />

profile is given by<br />

∫ x ∫ ∞<br />

PR(x) = dx ′ F ( x ′ ,y ) dy<br />

−<br />

−∞<br />

∫ ∞<br />

x<br />

−∞<br />

∫ ∞<br />

dx ′ F ( x ′ ,y ) dy + N (x) . (2.10)<br />

−∞<br />

Experimentally, the width of the doma<strong>in</strong> wall image can be<br />

determ<strong>in</strong>ed from the 25–75 criterion, or, alternatively from the<br />

derivative at the center, x 0 ,asw r = (PR + + PR − )/2PR ′ (x 0 ).<br />

These def<strong>in</strong>itions can also be used if the doma<strong>in</strong> wall profile is<br />

fitted us<strong>in</strong>g a suitable function. For example, with a Boltzmann<br />

fit, PR(x) = PR − + (PR + − PR − )/(1+exp[(x − x 0 )/x d ]), the<br />

doma<strong>in</strong> wall image width is w r = 2x d . Note that the signal<br />

gradient at the doma<strong>in</strong> wall provides an upper limit of the<br />

‘sharpness’ of any <strong>in</strong>tr<strong>in</strong>sic feature <strong>in</strong> the image.<br />

2.3.2.2. Resolution <strong>in</strong> phase images. One of the difficulties <strong>in</strong><br />

def<strong>in</strong><strong>in</strong>g the resolution <strong>in</strong> PFM stems from differences between<br />

the phase and mixed signal images. While the normalized<br />

PFM signal, pr, changes cont<strong>in</strong>uously between −1 and1on<br />

the lengthscale of w d , the phase signal for zero noise changes<br />

abruptly from 0 ◦ for pr < 0 to 180 ◦ for pr > 0. Thus, the<br />

width of phase signal is effectively zero. In the presence of<br />

noise, the evolution of a phase signal can be understood from<br />

the schematics <strong>in</strong> figure 10(a). The phase achieves limit<strong>in</strong>g<br />

values when the mixed signal is either significantly larger or<br />

smaller than the characteristic noise amplitude and changes<br />

rapidly <strong>in</strong> the region where the noise amplitude is sufficiently<br />

large to place the signal above or below the threshold value.<br />

Hence, the width of the doma<strong>in</strong> wall <strong>in</strong> the phase image is<br />

estimated as w ϕ =〈N〉/2PR ′ (x 0 ), where 〈N〉 is the average<br />

11

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