Comments: Strong no_sub_tour constraints
significantly increase our ability to manage the
Elementary_Trip problem through branch and cut.
Notice that, since the Elementary_Trip model tends
to overestimate the energy purchase value, values
UB_S1 are significantly larger than values UB_G
obtained in Table 4.
Table 6: Behavior of the Surrogate Components.
Inst. UB_G W_Price W_Price8 W_ML
1 735.3 735.3 735.3 740.8
2 951.3 966.8 951.3 980.6
3 999.2 1010.3 995.0 1030.0
4 508.2 512.6.2 504.3 508.2
5 969.0 986.5 972.6 1040.2
6 1486.3 1487.0 1487.0 1512.5
7 3065.5 3025.7 3003.5 3197.3
8 4211.8 4225.8 4200.6 4354.6
9 9594.3 9397.7 9365.9 9456.1
10 8560.3 8508.9 8475.1
Comments: Solving PV_Prod_VRP while relying on
the parametric pricing mechanism often behaves
better than the PV_Prod_VRP MILP. As for the the
machine learning oriented approach, the gap between
our best PV_Prod_VRP value and W_ML_ILP is in
average around 4%, with a peak at 7%.
5 CONCLUSIONS
We dealt here with synchronization between
consumption and production. We shortcut the
production sub-problem and replaced it by a
parametric surrogate sub-problem. But since in true
life solar energy production forecasting involves a
uncertainty, going further with machine learning
could help us in managing related risk of failure.
ACKNOWLEDGEMENTS
We thank both Labex IMOBS3 and PGMO program
for funding this research.
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