view article

Figure 3
Intensity autocorrelation function Δg2 = g2 − 1 averaged over 14328 repeated measurements from sample A. The blue solid line shows the fitting of Δg2 = βexp[−2τ/τ0(Q)]. The inset shows the fit with the Stokes–Einstein equation τ0(Q) = 1/(DQ2) (red dashed line).

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Follow J. Synchrotron Rad.
Sign up for e-alerts
Follow J. Synchrotron Rad. on Twitter
Follow us on facebook
Sign up for RSS feeds