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(lambda) is the linear expansion rate of montmorillonite at time of t, %. (h_{t}) is the linear expansion of montmorillonite at time of t, mm.
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The shear layers originating from the rotor tip circumference show classic linear expansion downstream, with the rate of a plane shear layer vertically and 1.5 times that horizontally.
In the process of analysis, the swelling properties of montmorillonite were determined by the measured linear expansion of montmorillonite (called the expansion rate), the formula as follows.
For more distant galaxies, then, whose light has been travelling to us for much longer times, the approximation of constant expansion rate fails, and the Hubble law becomes a non-linear integral relationship and dependent on the history of the expansion rate since the emission of the light from the galaxy in question.
These findings agree extremely well with an experimental study of E. coli growth under nearly identical conditions (solid agar medium with M9 salts, glucose, and trace elements) that reported an exponential-to-linear transition occurring around 12 hours after inoculation onto agar plates and a radial expansion rate of around 0.008 μm s −1 [ 28].
In other words, the wavelength has grown in direct proportion to the linear expansion factor of the universe.
Figure 5 Expansion rate performance test.
Transit linear expansion coefficient of the steel strand.
Average linear expansion coefficient of the steel strand.
The transit linear expansion coefficient was used to describe the thermal expansion at certain time point.
This system also performs better in terms of linear expansion.
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