Experimental Investigation of Dynamic Behavior of Cantilever Retaining Walls
Transcript of Experimental Investigation of Dynamic Behavior of Cantilever Retaining Walls
1Chapter 27
2Experimental Investigation of Dynamic
3Behaviour of Cantilever Retaining Walls
4Panos Kloukinas, Augusto Penna, Anna Scotto di Santolo, Subhamoy
5Bhattacharya, Matthew Dietz, Luiza Dihoru, Aldo Evangelista,
6Armando L. Simonelli, Colin A. Taylor, and George Mylonakis
7Abstract The dynamic behaviour of cantilever retaining walls under earthquake
8action is explored by means of 1-g shaking table testing, carried out on scaled models
9at the Bristol Laboratory for Advanced Dynamics Engineering (BLADE), University
10of Bristol, UK. The experimental program encompasses different combinations of
11retaining wall geometries, soil configurations and input ground motions. The
12response analysis of the systems at hand aimed at shedding light onto the salient
13features of the problem, such as: (1) the magnitude of the soil thrust and its point of
14application; (2) the relative sliding as opposed to rocking of the wall base and the
15corresponding failure mode; (3) the importance/interplay between soil stiffness, wall
16dimensions, and excitation characteristics, as affecting the above. The results of the
17experimental investigations were in good agreement with the theoretical models used
18for the analysis and are expected to be useful for the better understanding and the
19optimization of earthquake design of this particular type of retaining structure.
P. Kloukinas (*) • G. Mylonakis
Department of Civil Engineering, Geotechnical Engineering Laboratory,
University of Patras, 26504 Patras, Greece
e-mail: [email protected]; [email protected]
A. Penna • A.L. Simonelli
Department of Engineering, University of Sannio,
Piazza Roma 21, 82100 Benevento, Italy
e-mail: [email protected]; [email protected]
A.S. di Santolo • A. Evangelista
Department of Civil and Environmental Engineering,
University of Naples Federico II, via Claudio 21, 80125 Napoli, Italy
e-mail: [email protected]; [email protected]
S. Bhattacharya • M. Dietz • L. Dihoru • C.A. Taylor
Department of Civil Engineering, University of Bristol,
Queen’s Building, University Walk, Bristol BS8 1TR, UK
e-mail: [email protected]; [email protected]; [email protected];
A. Ilki and M.N. Fardis (eds.), Seismic Evaluation and Rehabilitationof Structures, Geotechnical, Geological and Earthquake Engineering 26,
DOI 10.1007/978-3-319-00458-7_27, © Springer International Publishing Switzerland 2014
20 27.1 Introduction
21 Reinforced concrete cantilever retaining walls represent a popular type of retaining
22 system. It is widely considered as advantageous over conventional gravity walls as
23 it combines economy and ease in construction and installation. The concept is
24 deemed particularly rational, as it exploits the stabilizing action of the soil weight
25 over the footing slab against both sliding and overturning, thus allowing construc-
26 tion of walls of considerable height.
27 The traditional approach for the analysis of cantilever walls is based on the well-
28 known limit equilibrium analysis, in conjunction with a conceptual vertical surface
29 AD (Fig. 27.1b, c) passing through the innermost point of the wall base (vertical
30 virtual back approach). A contradictory issue in the literature relates to the calculation
31 of active thrust acting on the virtual wall back, under a certain mobilized obliquity
32 ranging naturally from 0 (a perfectly smooth plane) to φ (a perfectly rough plane).
33 Efforts have been made by numerous investigators to establish the proper roughness
34 for the analysis and design or this type of structures as reported by Evangelista et al.
concretewall (γw)
H
B
A
D
C
90 − f
t
b
B
D
H
V
H
V
ei
B
B´ = B – 2e
H´PAE
d E
PAE = 1–2Kg E (1 – av)g H'
2
C
A
a b
d
bodyforces
ah x Ww ah x Ws
equivalent wallinclination(ω = ω wall)
dry, cohesionlessbackfill (f, γ)
b - characteristic(ω = ω b )
vertical virtualback (ω = 0)
a - characteristic(ω = ω a )
ωwall
WsWw
PAE v
PAE h
SFsliding = H / Hult
SFbearing capacity =V / Vult
+ω
β
+ ah γ+ av γ
γ
+ye
4 2 2 2
Fig. 27.1 Pseudo-dynamic analysis of cantilever retaining walls for seismic loading: (a) Problem
under consideration, (b) seismic Rankine stress field characteristics, (c) Modified virtual back
approach by stress limit analysis, (d) Stability analysis according to Meyerhof (CEN 2003)
P. Kloukinas et al.
35(2009, 2010) and Kloukinas andMylonakis (2011). Nevertheless, the issue of seismic
36behaviour remains little explored. In fact many modern Codes, including the
37Eurocodes (CEN 2004) and the Italian Building Code (NTC 2008), do not explicitly
38refer to cantilever walls. The current Greek Seismic Code (EAK 2003) address the
39case of cantilever retaining walls adopting the virtual back approach in the context of
40a pseudo-static analysis under the assumption of gravitational infinite slope
41conditions (Rankine 1857) and various geometric constraints.
42Recent theoretical findings obtained by means of stress limit analysis
43(Evangelista et al. 2010; Evangelista and Scotto di Santolo 2011; Kloukinas and
44Mylonakis 2011) for the seismic problem of Fig. 27.1a indicate that a uniform
45Rankine stress field can develop in the backfill, when the wall heel is sufficiently
46long and the stress characteristics do not intersect the stem of the wall (ωβ < ωwall).
47Given that the inclination of the stress characteristics depends on acceleration level,
48a Rankine condition is valid for the vast majority of cantilever wall configurations
49under strong seismic action. This is applicable even to short heel walls, with an
50error of about 5 % (Huntington 1957; Greco 2001).
51Following the above stress limit analysis studies, closed-form expressions are
52derived for both the pseudodynamic earth pressure coefficient KAE and the resultant
53thrust inclination, δE (Fig. 27.1c), given by (Kloukinas and Mylonakis 2011):
δE ¼ tan�1 sinφ sin Δ1e � β þ ψ eð Þ1� sinφ cos Δ1e � β þ ψ eð Þ
� �(27.1)
54where Δ1e ¼ sin�1[sin(β + ψe)/sinφ] and ψe ¼ tan�1[ah/(1�av)] are the so-called
55Caquot angle and the inclination of the overall body force in the backfill. The same
56result for δE has been derived, in a different form, by Evangelista et al. (2009,
572010). In the case of gravitational loading (ψe ¼ 0), the inclination δE equals the
58slope angle β, coinciding to the classical Rankine analysis. In presence of a
59horizontal body force component, δE is always greater than β, increasing with
60ψe up to the maximum value of φ, improving consequently wall stability. The
61robustness of the above stress limit analysis becomes evident since under Rankine
62conditions and mobilized inclination δE, the stress limit analysis and the
63Mononobe-Okabe formula results coincide. These findings have been confirmed
64by numerical analysis results (Evangelista et al. 2010; Evangelista and Scotto di
65Santolo 2011).
66A second key issue in the design of the particular type of retaining systems deals
67with the stability analysis shown in Fig. 27.1d. Traditionally, stability control of
68retaining walls is based on safety factors against bearing capacity, sliding and
69overturning. Of these, only the first two are known to be rationally defined, whereas
70the safety factor against overturning is known to be misleading, lacking a physical
71basis (Greco 1997; NTC 2008; Kloukinas and Mylonakis 2011). It is important to
72note that the total gravitational and seismic actions on the retaining wall are resisted
73upon the external reactions H and V acting on the foundation slab. The combination
27 Experimental Investigation of Dynamic Behaviour of Cantilever Retaining Walls
74 of these two actions, together with the resulting eccentricity e, determines the
75 bearing capacity of the wall foundation, based on classical limit analysis procedures
76 for a strip footing subjected to an eccentric inclined load (e.g. EC7, EC8). This
77 suggests that the wall stability is actually a footing problem and from this point of
78 view, understanding the role of the soil mass above the foundation slab and the soil-
79 wall interaction is of paramount importance. The above observations provided the
80 initial motivation for the herein-reported work.
81 27.2 Shaking Table Experimental Investigation
82 The dynamic behaviour of L-shaped cantilever walls was explored by means of 1-g
83 shaking table testing. The aim of the experimental investigation is to better under-
84 stand the soil-wall dynamic interaction problem, the relationship between design
85 parameters, stability safety factors and failure mechanisms, and the validation of
86 the seismic Rankine theoretical model. The test series were conducted to the Bristol
87 Laboratory for Advanced Dynamics Engineering (BLADE), University of Bristol,
88 UK. Details on the experimental hardware, materials, configurations and procedure
89 are provided in the ensuing.
90 27.2.1 Experimental Hardware
91 27.2.1.1 Earthquake Simulator (ES)
92 The 6DOF ES consists of a 3 m � 3m cast aluminum platformweighing 3.8 tonnes,
93 with payload capacity of 15 tonnes maximum and operating frequency range of
94 1–100 Hz. The platform sits inside an isolated, reinforced concrete seismic block
95 that has a mass of 300 tonnes and is attached to it by eight 70 kN servo hydraulic
96 actuators of 0.3 m stroke length. Hydraulic power for the ES is provided by a set of
97 six shared variable volume hydraulic pumps providing up to 900 l/min at a working98 pressure of 205 bar, with maximum flow capacity of around 1,200 l/min for up to
99 16 s at times of peak demand with the addition of extra hydraulic accumulators.
100 27.2.1.2 Equivalent Shear Beam (ESB) Container
101 The apparatus, shown in Fig. 27.2a, consists of 11 rectangular aluminum rings,
102 which are stacked alternately with rubber sections to create a flexible box of inner
103 dimensions 4.80 m long by 1 mwide and 1.15 m deep (Crewe et al. 1995). The rings
104 are constructed from aluminum box section to minimize inertia while providing
105 sufficient constraint for the K0 condition. The stack is secured to the shaking table
P. Kloukinas et al.
106by its base and shaken horizontally lengthways (in the x direction). Its floor is
107roughened by sand-grain adhesion to aid the transmission of shear waves; the
108internal end walls are similarly treated to enable complementary shear stresses.
109Internal side walls were lubricated with silicon grease and covered with latex
110membrane to ensure plane strain conditions.
111This type of containers should be ideally designed to match the shear stiffness of
112the soil contained in it, as shown in Fig. 27.2b. However, the shear stiffness of the
113soil varies during shaking depending on the strain level. Therefore the matching of
114the two stiffnesses (end-wall and soil) is possible only at a particular strain level.
115The “shear stack” at the University of Bristol is designed considering a value of
116strains in the soil close to failure (0.01–1 %). Therefore it is much more flexible
117than the soil deposit at lower strain amplitudes; as a consequence, the soil will
118always dictate the overall behaviour of the container (Bhattacharya et al. 2012).
119Indeed the shear stack resonant frequency and damping in the first shear mode in the
120long direction when empty were measured prior to testing as 5.7 Hz and 27 %
121respectively, sufficiently different from the soil material properties.
12227.2.1.3 Instrumentation
123As seen in Fig. 27.3, 21 1-D accelerometers have been used to monitor the shaking
124table, the shear stack and the wall-soil system, with the main area of interest laying
125on the wall itself and the soil mass in its vicinity, as well as the response of the free
126field. 4 LVDT transducers were used to measure the dynamic response and perma-
127nent displacements of the wall and 32 strain gauges were attached on the stem and
128the base of the wall, on three cross sections, to monitor the bending of the wall. The
129signal conditioning was made via appropriate amplifier and filter modules and data
130acquisitions frequency was set at 1,024 Hz. Additionally to the 57 data channels
131employed overall, a grid of coloured sand was used for monitoring the settlement of
132the backfill surface.
Fig. 27.2 Equivalent shear beam container (“shear stack”)
27 Experimental Investigation of Dynamic Behaviour of Cantilever Retaining Walls
133 27.2.2 Shaking Table Model Setup
134 27.2.2.1 Model Geometry
135 The dimensions of the model are illustrated in Fig. 27.3, with the type and the
136 positions of the instrumentation used. The model consists of an L-shaped retaining
137 wall supporting a backfill of thickness 0.6 m and length five times its thickness,
138 resting on a 0.4 m thick base soil layer (equal to the wall foundation width, B).
139 The properties of the soil layers and detailed description of the instrumentation and
140 the various wall configurations are provided in the below.
141 The retaining wall was constructed from Aluminium 5,083 plates of thickness
142 32 mm. The width of the wall stem is 970 mm. A central wall segment of 600 mm
143 width was created by two 1 mm thick vertical slits penetrating 400 mm down into
144 the wall. The location of the slits was 185 mm from each side of the wall stem. The
145 base of the wall is subdivided into four 240 mm-wide aluminium segments that are
146 each secured to the wall stem using three M12 bolts. Properties of the aluminium
147 alloy are: unit weight γ ¼ 27 kN/m3, Young’s modulus E ¼ 70 GPa, Poisson’s
148 ratio ν ¼ 0.3.
zx
A1 A2
A7
A8A9A10A11
A3A4,5
A6
A13A14 A12
A15A16A17
A18
A19
A20 A21
D1
D3
D4
D2D: LVDT
A: Accelerometer
horizontal
vertical
1200
4800
1200200400900 900
300
300
300
600
400
1150
250
250
(+)
(+)
z
y
185600185
97032
32
570
b2 b1
Strain gaugepositions
88
50 front view(zy plane)
shaking table level
120 93
1 mmslits
400
wall model details
Configuration 1300
b2b1
7000
M12 bolts
Configuration 2250Configuration 3250
cross section(zx plane)
Fig. 27.3 Geometry and instrumentation of the shaking table model (dimensions in mm)
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14927.2.2.2 Soil Material Properties
150The required soil configuration consists of a dense supporting layer and a medium
151dense backfill. The material proposed for both layers is Leighton Buzzard (LB)
152sand BS 881–131, Fraction B (D50 ¼ 0.82 mm, Gs ¼ 2,640 kg/m3, emin ¼ 0.486,
153emax ¼ 0.78). This particular soil has been used extensively in experimental
154research at Bristol and a wide set of strength and stiffness data is available (detailed
155references in Bhattacharya et al. 2012). The empirical correlation between peak
156friction angle φ and relative density Dr provided by the experimental work of
157Cavallaro et al. (2001) was used for a preliminary estimation of the soil strength
158properties.
159The packing density for each layer, determined from sand mass and volume
160measurements during deposition, and the corresponding predictions for the peak
161friction angles strength are summarized in Table 27.1. The base deposit was formed
162by pouring sand in layers of 150–200 mm from a deposition height of 0.6 m and
163then densifying by shaking. After densification, the height of the layer was reduced
164to 390 mm. The top layer was formed by pouring sand in axisymmetric conditions
165close to the centre of the desired backfill region, without further densification. The
166pouring was carried out by keeping the fall height steady, about equal to 200 mm, to
167minimize the densification effect of the downward stream of sand.
16827.2.2.3 Model Wall Configurations
169Three different Configurations (#1, #2, #3) for the wall model presented in Fig. 27.3
170were used to provide different response in sliding and rocking of the base. The
171characteristics of these configurations are shown in Table 27.2. After testing
172Configuration 1, the wall model was modified for Configuration 2. The wall heel
173was shortened by 50 mm and the toe was totally removed. In Configuration 3, the
174geometry of Configuration 2 was retained, after increasing the frictional resistance
175of the base interface from 23.5� to 28� (approximately equal to the critical state
t1:1Table 27.1 Soil properties
Soil layers Voids ratio, e Relative density, Dr Unit weight, γd kN/m3 Friction angle, φ a t1:2
Foundation 0.61 60 % 16.14 42� t1:3
Backfill 0.72 22 % 15.07 34� t1:4
t1:5aEstimated from Cavallaro et al. (2001)
t2:1Table 27.2 Pseudostatic critical accelerations and associated safety factors (SF)
Test
configuration
Critical acceleration
for SFsliding ¼ 1
SFBearing capacity at
critical sliding
acceleration
Critical
acceleration for
SFBearing capacity ¼ 1
SFsliding at critical
bearing capacity
acceleration t2:2
No 1 0.18g 7.45 0.35g 0.68 t2:3
No 2 0.14g 1.46 0.17g 0.93 t2:4
No 3 0.23g 0.44 0.17g 1.14 t2:5
27 Experimental Investigation of Dynamic Behaviour of Cantilever Retaining Walls
176 angle), by pasting rough sandpaper. The interface friction angles were measured
177 in-situ by means of static pull tests on the wall. The differences between these three
178 Configurations, in terms of a pseudo-dynamic stability analysis according to EC7
179 (CEN 2003) are summarised in Table 27.2, ranging from a purely sliding-sensitive
180 wall (Configuration 1), to a purely rotationally sensitive one (Configuration 3).
181 A set of characteristic pictures of model details and installation procedures are
182 presented in Fig. 27.4.
183 27.2.3 Experimental Procedure
184 Each model Configuration was tested under the same dynamic excitation, described
185 in detail in the following paragraphs. Two different input motions, harmonic and
186 earthquake, were used in the form of sequential, increasing amplitude time
187 histories. The dynamic properties of the soil layers and the soil-wall interactive
188 system were investigated by means of the white noise exploratory procedure
189 described below. This kind of testing was repeated after every severe yielding of
190 the system to track for significant changes in the dynamic response and properties.
191 27.2.3.1 White Noise Excitation
192 During white noise exploratory testing, a random noise signal of bandwidth
193 1–100 Hz and RMS acceleration ¼ 0.005g was employed. During each exploratory
Fig. 27.4 Details of the experimental setup: (a) longitudinal aspect of the model, (b) wall face
instrumentation – Config. 2, (c),(d) pairs of accelerometers on shaking table and upper ring,
(e) backfill accelerometer, (f) sand pouring procedure, (g), (h) back and front view of the wall
P. Kloukinas et al.
194series test, and simultaneous data acquisition, system transmissibility was moni-
195tored using a two-channel spectrum analyser. The analyzer computes the frequency
196response function (FRF) between the input and the output signals of interest.
197Natural frequency and damping values for any resonances up to 40 Hz (i.e. within
198the seismic frequency range) were determined for well-defined resonances using
199the output of the analyser’s curve fitting algorithm by means of a least-squares error
200technique. Additionally, transfer functions can be determined between any pair of
201data channels to get a clear view of the system dynamics.
20227.2.3.2 Harmonic Excitation
203This type of input acceleration was imposed by sinusoidal excitation consisting of
20415 steady cycles. To smoothen out the transition between transient and steady-state
205response, the excitation comprises of a 5-cycle ramp up to full test level at the
206beginning of the excitation, and a 5-cycle ramp down to zero at the end. With
207reference to frequency and acceleration level, a set of five frequencies (4, 7, 13, 25
208and 43 Hz) was used at low acceleration amplitude of 0.05g, to study the dynamic
209response of the system. The excitation frequency of 7 Hz was then selected for a
210series of harmonic excitations with increasing amplitude, until failure. The
211conditions of the excitation are considered to be essentially pseudostatic, as the
212above frequency is much smaller than the resonant frequencies of the system, with
213respect to both the free field and the soil-wall system.
21427.2.3.3 Earthquake Excitation
215Three earthquake records from the Italian and American database were selected for
216the earthquake testing. Specifically, the Tolmezzo record from the Friuli, 1976
217earthquake, the Sturno record from Irpinia, 1980 and the Northridge record from
218Los Angeles, 1994. The authentic signals were scaled by a frequency scale factor
219of 5, derived from the scaling law n0.75, which is valid for 1-g modelling (Muir
220Wood et al. 2002), assuming a geometrical scale factor of n ¼ 9, corresponding to a
221prototype of 5.4 m high. The frequency-scaled signals were applied at low acceler-
222ation amplitude of 0.05g to measure the dynamic response of the model and then the
223Sturno record was selected for carrying out increasing amplitude dynamic testing,
224until failure in sliding or rocking of the retaining wall.
22527.3 Experimental Results and Discussion
226Some characteristic experimental measurements are presented in Figs. 27.5, 27.6,
22727.7, 27.8 and 27.9, for the observed failure mechanisms, accelerations, dynamic
228and permanent displacements and bending moments, organized in sets of graphs
229suitable for direct comparisons. Most of the results presented herein mainly relate to
27 Experimental Investigation of Dynamic Behaviour of Cantilever Retaining Walls
230 Configurations 1 and 3, for they exhibit yielding near similar acceleration conditions
231 but in different modes. Limited results are presented for Configuration 2, which is
232 significantly weaker compared to the others, failing almost simultaneously in foun-
233 dation sliding and rotation (i.e., bearing capacity) mode, thus is less important for
234 comparison reasons.
235 In Fig. 27.5, measured settlement profiles at the state of failure are plotted
236 together with the assumed failure mechanisms for Configurations 2 and 3. The
237 following are worthy of note: First, these failure mechanisms were observed only
238 for transient earthquake loading, whereas in the case of harmonic excitation, the
239 settlement profile could not clearly reveal the emergence of the main failure planes,
240 as it had more-or-less a smooth parabolic shape. This can be explained in view of a
241 non-uniform settlement and deformation mechanism and stronger dynamic effects
242 imposed by earthquake loading. Although there is actually not a “rigid block”
243 response in the retained soil mass, the experimental findings show that the earth-
244 quake excitation induces a more uniform acceleration distribution within the
245 retained soil mass, which corresponds to a more uniform stress field, as assumed
246 in the pseudo-static analyses. Second, the assumed failure mechanisms confirm the
247 estimations based on the material properties, the stability analysis and the yield
248 accelerations presented in Tables 27.1 and 27.2 respectively.
249 The measurements of system displacement for all tested configurations are
250 summarized in Fig. 27.6. The total, cumulative settlement and rotation of the
251 wall, for each series of sequential input motions are presented in Fig. 27.6a, b,
252 and the incremental displacements for each input motion are presented in
253 Fig. 27.6c–e, indicating different behaviour of the wall models under the same
254 input. The measurements confirm the predictions for the expected failure modes
255 and the levels of critical acceleration. The sliding failure is clearly visible in
256 Configuration 1, as is the bearing capacity failure in Configuration 3. Configuration
257 2 although designed to be weaker in sliding, also exhibits significant rotational
258 deformations caused by the high eccentricities induced by the seismic thrust.
259 Rotational deformations are also observed in Configuration 1 for high acceleration
Fig. 27.5 Backfill surface settlement distribution at failure: (a) initial grid geometry – dimensions
in mm, (b),(c) settlement distributions for Configurations 2 and 3, respectively
P. Kloukinas et al.
260levels, revealing that walls resting on a compliant base exhibits local bearing
261capacity failure near the toe, due to high compressive stress concentration. This
262observation elucidates the importance of properly designing retaining structures to
263avoid developing significant rotational response.
264Results from Configurations 1 and 3 under harmonic excitation are plotted
265together in Fig. 27.7.
Fig. 27.6 Measurements of wall displacement and rotation for all configurations and various base
excitations. (a) Cumulative footing rotation versus sliding (LVDT-D1), (b) Cumulative footing
settlement (LVDT-D4) versus sliding, (c), (d) and (e) Incremental wall displacement (LVDTs
D1-D2-D3) for configurations 1, 2 and 3, respectively
27 Experimental Investigation of Dynamic Behaviour of Cantilever Retaining Walls
Fig. 27.7 Comparison of typical experimental results for Configurations 1 and 3 under harmonic-
sinusoidal excitation: (a) measured wall accelerations, (b) corresponding wall displacements,
(c) negative acceleration distribution (maximum inertial forces towards the wall), (d) increment
of wall displacement (LVDTs D1-D2-D3) and (e) peak seismic increment of bending moment for
positive and negative acceleration
P. Kloukinas et al.
266The following can be observed: First the response of each Configuration is as
267expected. A translational response mode is evident in Configuration 1 and a rocking
268one in Configuration 3, respectively. Sliding discontinuities are obvious on the
269acceleration time histories of Configuration 1 (Fig. 27.7a), at a critical acceleration
270slightly higher than that of Table 27.2. Note that the translational yield acceleration
271is not steady, but always increases after every successive yielding, as even a small
272rotation causes penetration of the wall toe into the foundation soil thus increasing
273passive resistance. On the other hand, Configuration 3 starts rotating at initiation of
274yielding, without any evidence of sliding discontinuities on the recorded
275accelerogram. Second, in both cases the wall stem appears to have an amplified
276response, mainly because of foundation rocking and secondarily of pure bending of
277the stem. Naturally, this is more evident in Configuration 3. Third, both models
278exhibit a consistent, repeatable, behaviour with respect to yielding.
279The same results for earthquake loading on Configurations 1 and 3 are presented
280in Fig. 27.8. In this case, the input motion contains higher effective peak
281accelerations, but the number of important strong cycles (half cycle pulses) is
282only three. The sliding failure is again clearly visible in Configuration 1, as is the
283bearing capacity failure in Configuration 3 caused by the high eccentricities
284induced by seismic thrust. An important notice about the failure modes arising
285from the combination of the two comparisons is that the bearing capacity failure is
286more affected by the input acceleration level, whereas the behaviour of pure sliding
287mechanisms is mainly controlled by the time interval of the strong motion, as
288known from sliding block theory. Accordingly, rotational mechanisms appear to
289be more critical under strong earthquakes, even though they are strong enough
290against sliding (Figs. 27.7d and 27.8d). Moreover, some rotational deformation is
291also observed in Configuration 1 for high acceleration level, revealing that any wall
292resting on a compliant base exhibits local bearing capacity failure near the toe, due
293to concentration of high compressive stresses. This observation elucidates the
294importance of properly designing retaining structures to avoid development of
295significant rotational response.
296From the acceleration distributions of Figs. 27.7c and 27.8c, it can be observed
297that the earthquake loading results to conditions closer to the assumptions of
298pseudostatic analysis, as a soil mass moving together with the wall is evident,
299especially for the rotational mode of Configuration 3. Contrary to earthquake
300excitation, wall and soil under harmonic loading appear to respond in a quite
301different way. At last, the peak seismic increment of bending moments is compared
302in Figs. 27.7e and 27.8e. A noteworthy observation is that the earth pressure on the
303wall stem increases when the system moves towards the backfill, that is for an
304acceleration not critical for overall stability. On the other hand, at yielding acceler-
305ation of the system, earth pressure on the stem is minimum. This is in agreement
306with the findings of the analysis presented by Green et al. (2008) on a full scale
307numerical model and the experimental and numerical results of Al Atik and Sitar
308(2010). Comparing Configurations 1 and 3, it can be clearly identified that rota-
309tional modes induce lower earth pressure on the wall but different distribution
310leading to higher point of application of the thrust.
27 Experimental Investigation of Dynamic Behaviour of Cantilever Retaining Walls
Fig. 27.8 Comparison of typical experimental results for Configurations 1 and 3 under seismic
excitation: (a) measured wall accelerations, (b) corresponding wall displacements, (c) negative
acceleration distribution (maximum inertial forces towards the wall), (d) increment of wall
displacement (LVDTs D1-D2-D3) and (e) peak seismic increment of bending moment for positive
and negative acceleration
P. Kloukinas et al.
311Finally, the response of Configuration 2 to harmonic and earthquake excitation
312with PGA ¼ 0.17g presented in Fig. 27.9, exhibits a similar behaviour to both
313Configurations 1 and 3, resulting to simultaneous sliding and rotational failure. As
314seen from both the acceleration time histories (Fig. 27.9a) and the failure
315mechanisms (Fig. 27.9b) the sliding failure mode prevails, which is consistent to
316the critical accelerations estimated in Table 27.2.
31727.4 Conclusions
318A series of shaking table tests on scaled models of cantilever retaining walls were
319conducted in the BLADE laboratory at the University of Bristol. The initial
320motivation of this experimental study was the validation of recent stress limit
321analysis solutions for the seismic design of this type of retaining structures
322(Evangelista et al. 2009, 2010; Kloukinas and Mylonakis 2011) in conjunction
323with the absence of any specific, relative regulations in established seismic codes,
324including EC8. Special issues related to stability design and response of walls
325founded on compliant base, were also incorporated. Preliminary interpretation of
326the experimental findings confirms the predictions of the theoretical analysis, with
327reference to the failure mechanisms and the critical yield accelerations of the
328system. Pseudo-static stability analysis proves to behave adequately for both
Fig. 27.9 Typical experimental results for Configuration 2: (a) measured wall accelerations for
harmonic sinusoidal and seismic excitation, (b) negative acceleration distribution (maximum
inertial forces towards the wall)
27 Experimental Investigation of Dynamic Behaviour of Cantilever Retaining Walls
329 harmonic and seismic excitation, although important dynamic effects are evident in
330 the first case, dealing with the response of the backfill and the wall stem. On the
331 other hand, earthquake loading results to conditions closer to the assumptions of the
332 pseudo-static analysis, which are the uniform distribution of the acceleration and
333 the “rigid block” response of the backfill. Finally, the responses of the various wall
334 configurations confirm the equivalent footing analysis of wall stability and high-
335 light the importance of a proper design of walls founded on compliant base with
336 respect to sliding and rocking.
337 Acknowledgments The research leading to these results has received funding from the European
338 Union Seventh Framework Programme (FP7/2007–2013) for access to the Bristol Laboratory for
339 Advanced Dynamics Engineering (BLADE), University of Bristol, UK under grant agreement n�
340 227887 [SERIES].
341 References
342 Al Atik L, Sitar N (2010) Seismic earth pressures on cantilever retaining structures. J Geotech
343 Geoenviron Eng ASCE 136(10):1324–1333
344 Bhattacharya S, Lombardi D, Dihoru L, Dietz MS, Crewe AJ, Taylor CA (2012) Model container
345 design for soil-structure interaction studies. In: Fardis MN, Rakicevic ZT (eds) Role of seismic
346 testing facilities in performance-based earthquake engineering: SERIES workshop, vol
347 22, Geotechnical, geological and earthquake engineering. Springer, Dordrecht/New York
348 Cavallaro A, Maugeri M, Mazzarella R (2001) Static and dynamic properties of Leighton Buzzard
349 sand from laboratory tests. In: Proceedings of 4th international conference on recent advanced
350 in geotechnical earthquake engineering and soil dynamics and symposium in honour of
351 Professor WD Liam Finn, San Diego, CA, 26–31 March 2001
352 CEN (2003) EN 1997–1:2003 Eurocode 7 geotechnical design, Part 1: general rules. European
353 Committee for Standardization, Brussels
354 CEN (2004) EN 1998–1:2004 Eurocode 8 design of structures for earthquake resistance, Part 5:
355 foundations, retaining structures and geotechnical aspects. European Committee for
356 Standardization, Brussels
357 Crewe AJ, Lings ML, Taylor CA, Yeung AK, Andrighetto R (1995) Development of a large
358 flexible shear stack for testing dry sand and simple direct foundations on a shaking table.
359 In: Elnashai AS (ed) European seismic design practice. Balkema, Rotterdam
360 EAK 2000 (2003) Greek seismic code, Earthquake Planning and Protection Organization, Athens
361 Evangelista A, Scotto di Santolo A (2011) Dynamic active earth pressure on cantilever retaining
362 walls. Comput Geotech 38(8):1041–1051
363 Evangelista A, Scotto di Santolo A, Simonelli AL (2009) Dynamic response of cantilever retaining
364 walls. In: Proceedings of international conference on performance-based design in earthquake
365 geotechnical engineering – from case history to practice – Tokyo, 15–18 June 2009
366 Evangelista A, Scotto di Santolo A, Simonelli AL (2010) Evaluation of pseudostatic active earth
367 pressure coefficient of cantilever retaining walls. Soil Dyn Earthq Eng 30(11):1119–1128
368 Greco VR (1997) Stability of retaining walls against overturning. J Geotech Geoenviron Eng
369 ASCE 123(8):778–780
370 Greco VR (2001) Active earth thrust on cantilever walls with short heel. Can Geotech J
371 38(2):401–409
372 Green RA, Olgun CG, Cameron WI (2008) Response and modeling of cantilever retaining walls
373 subjected to seismic motions. Comput-Aided Civil Infrastruct Eng 23(4):309–322
374 Huntington W (1957) Earth pressures and retaining walls. Wiley, New York
P. Kloukinas et al.
375Kloukinas P, Mylonakis G (2011) Rankine Solution for seismic earth pressures on L-shaped
376retaining walls. In: 5 ICEGE, Santiago, Chile, 10–13 January 2011
377Muir Wood D, Crewe A, Taylor CA (2002) Shaking table testing of geotechnical models. UPMG-
378Int J Phys Model Geotech 2:01–13
379NTC (2008) Italian building code, DM 14 Jan, GU n 29, 4 Feb, n 30
380Rankine WJM (1857) On the stability of loose earth. Phil Trans Roy Soc Lond 147:9–27
27 Experimental Investigation of Dynamic Behaviour of Cantilever Retaining Walls