DHARM
228 GEOTECHNICAL ENGINEERING
This should be the same as the time-rate of volume decrease. Volumetric strain = mv.∆σ
= – mv∂(σ – u), by definition of the modulus of volume change, mv.
(The negative sign denotes decrease in volume with increase in pressure).
∴ Change of volume = – mv∂(σ – u).dz,
since the elementary layer of thickness dz and unit cross-sectional area in considered.
Time-rate of change of volume = −
∂
∂
m −
t
v.( ).σ udz
∂σ
∂t
= 0, since σ is constant.
∴ Time-rate of change of volume = +
∂
∂
m
u
t
v..dz
Equating this to water lost per unit time,
ku
z
dz m
u
t
dz
w
γ .. v..
∂
∂
=
∂
∂
2
2
or
∂
∂
=
∂
∂
u
t
c
u
v z
.
2
2 ...(Eq. 7.19)
where cv =
k
m
ke
vwγγav w
=
()+
.
1
...(Eq. 7.20)
7.5 SOLUTION OF TERZAGHI’S EQUATION FOR ONE-DIMENSIONAL
CONSOLIDATION
Terzaghi solved the differential equation (Eq. 7.19) for a set of boundary conditions which
have utility in solving numerous engineering problems and presented the results in graphical
form using dimensional parameters.
The following are the boundary conditions:
- There is drainage at the top of the sample: At z = 0, u = 0, for all t.
- There is drainage at the bottom of the sample: At z = 2H, u = 0, for all t.
- The initial hydrostatic excess pressure ui is equal to the pressure increment, ∆σ u = ui
= ∆σ, at t = 0.
Terzaghi chose to consider this situation where u = ui initially throughout the depth,
although solutions are possible when ui varies with depth in any specified manner. The thick-
ness of the sample is designated by 2H, the distance H thus being the length of the longest
drainage path, i.e., maximum distance water has to travel to reach a drainage face because of
the existence of two drainage faces. (In the case of only one drainage face, this will be equal to
the total thickness of the clay layer).
The general solution for the above set of boundary conditions has been obtained on the
basis of separation of variables and Fourier Series expansion and is as follows:
u = f(z, t) =
1
(^022)
2
1
22 4 2
H
u nz
H
dz nz
H
i e
H
n
nctHv
∑ z
F
HG
I
KJ
F
HG
I
= KJ
∞
sin ππ. sin − π / ...(Eq. 7.21)