Code for reproducing the results in the following paper:
Decorrelated Batch Normalization
Lei Huang, Dawei Yang, Bo Lang, Jia Deng
IEEE Conference on Computer Vision and Pattern Recognition (CVPR), 2018.
arXiv:1804.08450
- Install MAGMA (you can find the instructions in 'Install MAGMA.md' ). Note: MAGMA is required for SVD on GPU. Without MAGMA, you can run the code on CPU only, while all the CNN experiments in the paper are run on GPU.
- Install Torch with CUDA (for GPU). Note that
cutorch
should be compiled with MAGMA support if you have installed MAGMA and set the environments correctly. - Install cudnn v5.
- Install the dependency
optnet
by:
luarocks install optnet
- Run:
bash execute_MLP_0debug_MNIST.sh
This script will download MNIST automatically and you should put the mnist.t7/
under ./dataset/
. The experiment results will be saved at ./set_result/MLP/
.
- Prepare the data: download the YaleB dataset here, and put the data files under
/dataset/
so that the paths look like./dataset/YaleB/YaleB_train.dat
and./dataset/YaleB/YaleB_test.dat
. - Run:
bash execute_MLP_1FIM_YaleB_best.sh
The experiment results will be saved at directory: 'set_result/MLP/'.
You can experiment with different hyperparameters by running these scripts -- execute_MLP_1FIM_YaleB_HyperP.sh
and execute_MLP_1FIM_YaleB_HyperP_nnn.sh
.
- Prepare the data: download the PIE dataset here, and put the data file under
./dataset/
such that the paths look like./dataset/PIE/PIE_train.dat
and./dataset/PIE/PIE_test.dat
. - To experiment with different group sizes, run:
bash execute_MLP_2PIE_DBNGroup.sh
- To obtain different baseline performances, execute:
bash execute_MLP_2PIE.sh
bash execute_MLP_2PIE_nnn.sh
Note that the experiments until this point can be run on CPU, so MAGMA is not needed in above experiments.
- Prepare the data: follow the instructions for CIFAR-10 in this project . It will generate a preprocessed dataset and save a 1400MB file. Put this file
cifar_provider.t7
under./dataset/
. - Run:
bash execute_Conv_1vggA_2test_adam.sh
bash execute_Conv_1vggA_2test_base.sh
bash execute_Conv_1vggA_2test_ELU.sh
bash execute_Conv_1vggA_2test_var.sh
Note that if your machine has fewer than 4 GPUs, the environment variable CUDA_VISIBLE_DEVICES
should be changed accordingly.
- Prepare the data: same as in VGG-A experiments.
- Run:
bash exp_Conv_4Splain_1deep.lua
bash exp_Conv_4Splain_2large.lua
bash execute_Conv_2residual_old.sh
bash execute_Conv_3residual_wide_Cifar100_wr_BN_d28_h48_g16_b128_dr0.3_s1_C2.sh
bash execute_Conv_3residual_wide_Cifar100_wr_DBN_scale_L1_d28_h48_g16_b128_dr0.3_s1_C3.sh
bash execute_Conv_3residual_wide_Cifar10_wr_BN_d28_h48_g16_b128_dr0.3_s1_C2.sh
bash execute_Conv_3residual_wide_Cifar10_wr_DBN_scale_L1_d28_h48_g16_b128_dr0.3_s1_C3.sh
- Clone Facebook's ResNet repo here.
- Download ImageNet and put it in:
/tmp/dataset/ImageNet/
(you can also customize the path inopts.lua
) - Install the DBN module to Torch as a Lua package: go to the directory
./models/imagenet/cuSpatialDBN/
and runluarocks make cudbn-1.0-0.rockspec
. - Copy the model definitions in
./models/imagenet/
(resnet_BN.lua
,resnet_DBN_scale_L1.lua
andinit.lua
) to./models
directory in the cloned repofb.resnet.torch
, for reproducing the results reported in the paper. You also can compare the pre-activation version of residual networks introduced in the paper (using the model filespreresnet_BN.lua
andpreresnet_DBN_scale_L1.lua
). - Use the default configuration and our models to run experiments.
Email: [email protected]. Any discussions and suggestions are welcome!