Having simulated the seismic behaviour of the three columns (i.e., C, M and L) using five different models for the concrete properties in the core, the numerical results are compared to their experimental counterparts. This comparison is used to understand how well the models predicted the behaviour of the columns and to identify the model that fits the experimental data best. The comparisons are based on features of the hysteretic curve as well as on the dissipated energy evolution.
3.5.1. Hysteretic curves
The differences between the experimental and numerical results are examined here by comparing the lateral force-drift relationship of the columns under cyclic loading.
In Fig. 10, the lateral force-displacement curves are also used to assess how close the five numerical models are to the experimental results for the three columns: C, M and L. It can be noted that all models behave approximately the same until the peak lateral force is reached, after which significant differences are notable. This can also be clearly seen by the comparison of the experimental and numerical lateral force-displacement envelops in Fig. 11a-c. The Park et al. [16] as well as the Kappos et al. [15] models appear to capture well the post-peak behaviour of all three columns as depicted in Fig. 11a-c. Instead, the Chang and Mander [20] model captures well the post-peak behaviour for columns C and M but fails to capture the strength degradation for L. The Mander et al. [19] model also fails to represent the strength degradation past the peak lateral force for all three columns. Finally, the model which assumes no confinement systematically under-predicts the experimental behaviour of all three columns past the peak force. This highlights the important role of (limited) confinement in the post-peak behaviour of the pre-code columns, even when the transverse reinforcement has 90o hooks.
In Table 5, a summary of key values (for the positive direction of the columns’ drift) of the cyclic test is shown for the three columns. The summary includes the peak lateral force (Fc,max), and its corresponding drift (dc,max), the ultimate lateral force (Fc,ult), and corresponding drift (dc,ult), the drift at the yield point (dc,y), and the displacement ductility at ultimate point (µΔ,ult). The ultimate point is considered here as the point at which the strength drops by 20% of Fc,max, according to [21]. Due to this assumption, the ultimate force and drift for the Mander et al. [19] model for all three columns and for the Chang and Mander [20] for column L cannot be estimated, as these models do not predict strength degradation. With regard to dc,y, the yield displacement is calculated according to Annex B.3 of EC8-1 [22]. For each column, an elastic-perfectly plastic relationship is fitted to the experimental or numerical lateral load – displacement envelope up to the ultimate point, ensuring the following requirements are satisfied: (i) the areas under and above the envelope curve must have the same values; and (ii) the area under (or above) the envelope curve is the lowest possible [23]. Finally, the displacement ductility at ultimate point is equal to the ratio of dc,ult over dc,y.
With regard to the maximum force (Fc,max), Table 5 shows that all five models predict well the maximum force for all three columns (i.e., C, M and L) with error less than 10%, in line with observations in Fig. 10 and 11. By contrast, the differences between the models and the experimental results are evident for the displacement ductility at ultimate point. For columns C and M, the ductility for the Park et al. [16], Kappos et al. [15] and Chang and Mander [20] models is approximately equal to its experimental counterpart. The ductility for the model with no confinement is notably smaller (i.e., error 12%) than its experimental counterpart for both columns C and M. The observations differ for column L. The ductility for the Park et al. [16] and Kappos et al. [15] confinement models, (which are the only two models for which the ultimate point can be determined using the conventions of this study), is notably larger (i.e., error greater than 15%) than its experimental counterpart. By contrast, the ductility for the model without confinement is only 8% smaller than the experimental one.
Table 5
Maximum and ultimate lateral force and corresponding drift, drift at yield strength and ductility at ultimate strength.
Source
|
Column
|
Fc,max
|
dc,max
|
Fc,ult
|
dc,ult
|
dc,y
|
µΔ,ult
|
Diss.
Energy
|
(kN)
|
(%)
|
(kN)
|
(%)
|
(%)
|
|
(kNm)
|
Experim.
|
C
|
69.4
|
1.2
|
55.5
|
2.8
|
0.4
|
7.4
|
53.7
|
Anal.
|
Mander et al. [19]
|
68.1
|
1.2
|
-
|
-
|
0.4
|
-
|
-
|
Kappos et al. [15]
|
68.3
|
1.2
|
54.6
|
2.9
|
0.4
|
7.8
|
42.4
|
Park et al. [16]
|
68.3
|
1.2
|
54.6
|
2.8
|
0.4
|
7.6
|
39.7
|
Chang & Mander [20]
|
68.1
|
1.2
|
54.5
|
2.7
|
0.4
|
7.3
|
35.5
|
No Confinement
|
68.3
|
1.2
|
54.6
|
2.4
|
0.4
|
6.5
|
27.3
|
Experim.
|
M
|
69.7
|
1.6
|
55.8
|
2.7
|
0.7
|
4.2
|
45.1
|
Anal.
|
Mander et al. [19]
|
64.3
|
1.2
|
-
|
-
|
0.6
|
-
|
-
|
Kappos et al. [15]
|
64.4
|
1.2
|
51.5
|
2.7
|
0.6
|
4.2
|
33.9
|
Park et al. [16]
|
64.5
|
1.2
|
51.6
|
2.6
|
0.6
|
4.1
|
31.9
|
Chang & Mander [20]
|
64.3
|
1.2
|
51.4
|
2.6
|
0.7
|
4.0
|
31.6
|
No Confinement
|
64.3
|
1.2
|
51.4
|
2.0
|
0.7
|
3.1
|
17.1
|
Experim.
|
L
|
53.2
|
1.7
|
42.6
|
2.4
|
1.0
|
2.5
|
25.0
|
Anal.
|
Mander et al. [19]
|
54.5
|
2.0
|
-
|
-
|
0.8
|
-
|
-
|
Kappos et al. [15]
|
53.4
|
1.7
|
42.7
|
2.4
|
0.8
|
3.0
|
19.8
|
Park et al. [16]
|
53.2
|
1.7
|
42.6
|
2.3
|
0.8
|
2.9
|
17.8
|
Chang & Mander [20]
|
54.1
|
2.0
|
-
|
-
|
0.8
|
-
|
-
|
No Confinement
|
52.1
|
1.3
|
41.6
|
1.8
|
0.8
|
2.3
|
10.4
|
As observed in Fig. 10, the fire influences the stiffness of the column, especially in column L, due to concrete strength loss. Ιn Fig. 12, the secant stiffness-drift relationship obtained experimentally and analytically for the five models is presented for the three columns. The secant stiffness is calculated dividing the maximum compressive force or each cycle with the corresponding displacement concentrating only on the positive displacements at each cycle. It should be noted that for all five models the initial secant stiffness obtained analytically is smaller than the experimental one for all three columns. Nonetheless, the differences after 0.5% drift are negligible for all models.
Finally, the strength degradation between the first and third cycle of each drift level obtained experimentally and numerically for the three columns is shown in Fig. 13. It can be seen that for column C, the degradation of strength estimated analytically by all five models follows closely the experimental results up to 2% drift. For the final three cycles associated with larger drifts, the discrepancies are substantial for all models. A similar observation is true for column M. For column L, the discrepancies are substantial for all cycles highlighting the inadequacy of the analytical model to capture the strength degradation within the three cycles of the most severely damaged column.
3.5.2. Dissipated energy
The evolution of the total hysteretic dissipated energy with the drift, based on the experimental and numerical results, is depicted in Fig. 14. The dissipated energy is computed as the sum of the energy dissipation for each hysteretic cycle and corresponds to the interior area of the lateral force-displacement loop of that cycle. The cumulative hysteretic dissipated energy value at the ultimate drift are also distinctly marked in Fig. 14 and their values reported in Table 5. For the experimental results, it is observed that the energy dissipated by columns M and L were respectively 16% and 53% lower that column C up to the ultimate drift. Therefore, the prior fire damage decreases the energy capacity of the columns. When compared to the numerical results, it can be seen that the energy curves overlap substantially and in all cases appear to dissipate less energy than is observed in the experiments.
In Table 5, the values of the cumulative dissipated energy at ultimate drift are reported. Values for the Mander et al. [19] model for all three columns as well as the Chang and Mander [20] model for column L are not reported as the ultimate drift could not be estimated as the strength did not deteriorate by 20% for these models. The comparison of the remaining models shows that the Kappos et al. [15] and Park et al. [16] models yield very similar results for all three columns. In particular, the energy dissipated by these models for column C is approximately 25% lower that its experimental counterpart. For the other two columns (i.e., M and L), the error from use of the Kappos et al. [15] remains very similar. However, for Park et al. [16] models, the error is raised to ~30%. By contrast, the no confinement model systematically dissipates substantially less energy than seen in the experiments for all three columns (error equal or larger than 45% for all three scenarios).
Overall, Kappos et al. [15] model produced analytical results which matched better to the experimental than its alternatives, and Park et al. [16] followed closely, this justified the recommendation for these two models in the proposed framework in Sect. 2.