Loss Functions

Flux provides a large number of common loss functions used for training machine learning models. They are grouped together in the Flux.Losses module.

Loss functions for supervised learning typically expect as inputs a target y, and a prediction . In Flux's convention, the order of the arguments is the following

loss(ŷ, y)

Most loss functions in Flux have an optional argument agg, denoting the type of aggregation performed over the batch:

loss(ŷ, y)                         # defaults to `mean`
loss(ŷ, y, agg=sum)                # use `sum` for reduction
loss(ŷ, y, agg=x->sum(x, dims=2))  # partial reduction
loss(ŷ, y, agg=x->mean(w .* x))    # weighted mean
loss(ŷ, y, agg=identity)           # no aggregation.

Losses Reference

Flux.Losses.maeFunction
mae(ŷ, y; agg = mean)

Return the loss corresponding to mean absolute error:

agg(abs.(ŷ .- y))

Example

julia> y_model = [1.1, 1.9, 3.1];

julia> Flux.mae(y_model, 1:3)
0.10000000000000009
source
Flux.Losses.mseFunction
mse(ŷ, y; agg = mean)

Return the loss corresponding to mean square error:

agg((ŷ .- y) .^ 2)

See also: mae, msle, crossentropy.

Example

julia> y_model = [1.1, 1.9, 3.1];

julia> y_true = 1:3;

julia> Flux.mse(y_model, y_true)
0.010000000000000018
source
Flux.Losses.msleFunction
msle(ŷ, y; agg = mean, ϵ = eps(ŷ))

The loss corresponding to mean squared logarithmic errors, calculated as

agg((log.(ŷ .+ ϵ) .- log.(y .+ ϵ)) .^ 2)

The ϵ term provides numerical stability. Penalizes an under-estimation more than an over-estimatation.

Example

julia> Flux.msle(Float32[1.1, 2.2, 3.3], 1:3)
0.009084041f0

julia> Flux.msle(Float32[0.9, 1.8, 2.7], 1:3)
0.011100831f0
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Flux.Losses.huber_lossFunction
huber_loss(ŷ, y; δ = 1, agg = mean)

Return the mean of the Huber loss given the prediction and true values y.

             | 0.5 * |ŷ - y|^2,            for |ŷ - y| <= δ
Huber loss = |
             |  δ * (|ŷ - y| - 0.5 * δ), otherwise
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Flux.Losses.label_smoothingFunction
label_smoothing(y::Union{Number, AbstractArray}, α; dims::Int=1)

Returns smoothed labels, meaning the confidence on label values are relaxed.

When y is given as one-hot vector or batch of one-hot, its calculated as

y .* (1 - α) .+ α / size(y, dims)

when y is given as a number or batch of numbers for binary classification, its calculated as

y .* (1 - α) .+ α / 2

in which case the labels are squeezed towards 0.5.

α is a number in interval (0, 1) called the smoothing factor. Higher the value of α larger the smoothing of y.

dims denotes the one-hot dimension, unless dims=0 which denotes the application of label smoothing to binary distributions encoded in a single number.

Example

julia> y = Flux.onehotbatch([1, 1, 1, 0, 1, 0], 0:1)
2×6 OneHotMatrix(::Vector{UInt32}) with eltype Bool:
 ⋅  ⋅  ⋅  1  ⋅  1
 1  1  1  ⋅  1  ⋅

julia> y_smoothed = Flux.label_smoothing(y, 0.2f0)
2×6 Matrix{Float32}:
 0.1  0.1  0.1  0.9  0.1  0.9
 0.9  0.9  0.9  0.1  0.9  0.1

julia> y_sim = softmax(y .* log(2f0))
2×6 Matrix{Float32}:
 0.333333  0.333333  0.333333  0.666667  0.333333  0.666667
 0.666667  0.666667  0.666667  0.333333  0.666667  0.333333

julia> y_dis = vcat(y_sim[2,:]', y_sim[1,:]')
2×6 Matrix{Float32}:
 0.666667  0.666667  0.666667  0.333333  0.666667  0.333333
 0.333333  0.333333  0.333333  0.666667  0.333333  0.666667

julia> Flux.crossentropy(y_sim, y) < Flux.crossentropy(y_sim, y_smoothed)
true

julia> Flux.crossentropy(y_dis, y) > Flux.crossentropy(y_dis, y_smoothed)
true
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Flux.Losses.crossentropyFunction
crossentropy(ŷ, y; dims = 1, ϵ = eps(ŷ), agg = mean)

Return the cross entropy between the given probability distributions; calculated as

agg(-sum(y .* log.(ŷ .+ ϵ); dims))

Cross entropy is typically used as a loss in multi-class classification, in which case the labels y are given in a one-hot format. dims specifies the dimension (or the dimensions) containing the class probabilities. The prediction is supposed to sum to one across dims, as would be the case with the output of a softmax operation.

For numerical stability, it is recommended to use logitcrossentropy rather than softmax followed by crossentropy .

Use label_smoothing to smooth the true labels as preprocessing before computing the loss.

See also: logitcrossentropy, binarycrossentropy, logitbinarycrossentropy.

Example

julia> y_label = Flux.onehotbatch([0, 1, 2, 1, 0], 0:2)
3×5 OneHotMatrix(::Vector{UInt32}) with eltype Bool:
 1  ⋅  ⋅  ⋅  1
 ⋅  1  ⋅  1  ⋅
 ⋅  ⋅  1  ⋅  ⋅

julia> y_model = softmax(reshape(-7:7, 3, 5) .* 1f0)
3×5 Matrix{Float32}:
 0.0900306  0.0900306  0.0900306  0.0900306  0.0900306
 0.244728   0.244728   0.244728   0.244728   0.244728
 0.665241   0.665241   0.665241   0.665241   0.665241

julia> sum(y_model; dims=1)
1×5 Matrix{Float32}:
 1.0  1.0  1.0  1.0  1.0

julia> Flux.crossentropy(y_model, y_label)
1.6076053f0

julia> 5 * ans ≈ Flux.crossentropy(y_model, y_label; agg=sum)
true

julia> y_smooth = Flux.label_smoothing(y_label, 0.15f0)
3×5 Matrix{Float32}:
 0.9   0.05  0.05  0.05  0.9
 0.05  0.9   0.05  0.9   0.05
 0.05  0.05  0.9   0.05  0.05

julia> Flux.crossentropy(y_model, y_smooth)
1.5776052f0
source
Flux.Losses.logitcrossentropyFunction
logitcrossentropy(ŷ, y; dims = 1, agg = mean)

Return the cross entropy calculated by

agg(-sum(y .* logsoftmax(ŷ; dims); dims))

This is mathematically equivalent to crossentropy(softmax(ŷ), y), but is more numerically stable than using functions crossentropy and softmax separately.

See also: binarycrossentropy, logitbinarycrossentropy, label_smoothing.

Example

julia> y_label = Flux.onehotbatch(collect("abcabaa"), 'a':'c')
3×7 OneHotMatrix(::Vector{UInt32}) with eltype Bool:
 1  ⋅  ⋅  1  ⋅  1  1
 ⋅  1  ⋅  ⋅  1  ⋅  ⋅
 ⋅  ⋅  1  ⋅  ⋅  ⋅  ⋅

julia> y_model = reshape(vcat(-9:0, 0:9, 7.5f0), 3, 7)
3×7 Matrix{Float32}:
 -9.0  -6.0  -3.0  0.0  2.0  5.0  8.0
 -8.0  -5.0  -2.0  0.0  3.0  6.0  9.0
 -7.0  -4.0  -1.0  1.0  4.0  7.0  7.5

julia> Flux.logitcrossentropy(y_model, y_label)
1.5791205f0

julia> Flux.crossentropy(softmax(y_model), y_label)
1.5791197f0
source
Flux.Losses.binarycrossentropyFunction
binarycrossentropy(ŷ, y; agg = mean, ϵ = eps(ŷ))

Return the binary cross-entropy loss, computed as

agg(@.(-y * log(ŷ + ϵ) - (1 - y) * log(1 - ŷ + ϵ)))

Where typically, the prediction is given by the output of a sigmoid activation. The ϵ term is included to avoid infinity. Using logitbinarycrossentropy is recomended over binarycrossentropy for numerical stability.

Use label_smoothing to smooth the y value as preprocessing before computing the loss.

See also: crossentropy, logitcrossentropy.

Examples

julia> y_bin = Bool[1,0,1]
3-element Vector{Bool}:
 1
 0
 1

julia> y_prob = softmax(reshape(vcat(1:3, 3:5), 2, 3) .* 1f0)
2×3 Matrix{Float32}:
 0.268941  0.5  0.268941
 0.731059  0.5  0.731059

julia> Flux.binarycrossentropy(y_prob[2,:], y_bin)
0.43989f0

julia> all(p -> 0 < p < 1, y_prob[2,:])  # else DomainError
true

julia> y_hot = Flux.onehotbatch(y_bin, 0:1)
2×3 OneHotMatrix(::Vector{UInt32}) with eltype Bool:
 ⋅  1  ⋅
 1  ⋅  1

julia> Flux.crossentropy(y_prob, y_hot)
0.43989f0
source
Flux.Losses.kldivergenceFunction
kldivergence(ŷ, y; agg = mean, ϵ = eps(ŷ))

Return the Kullback-Leibler divergence between the given probability distributions.

The KL divergence is a measure of how much one probability distribution is different from the other. It is always non-negative, and zero only when both the distributions are equal.

Example

julia> p1 = [1 0; 0 1]
2×2 Matrix{Int64}:
 1  0
 0  1

julia> p2 = fill(0.5, 2, 2)
2×2 Matrix{Float64}:
 0.5  0.5
 0.5  0.5

julia> Flux.kldivergence(p2, p1) ≈ log(2)
true

julia> Flux.kldivergence(p2, p1; agg = sum) ≈ 2log(2)
true

julia> Flux.kldivergence(p2, p2; ϵ = 0)  # about -2e-16 with the regulator
0.0

julia> Flux.kldivergence(p1, p2; ϵ = 0)  # about 17.3 with the regulator
Inf
source
Flux.Losses.squared_hinge_lossFunction
squared_hinge_loss(ŷ, y)

Return the squared hinge_loss loss given the prediction and true labels y (containing 1 or -1); calculated as sum((max.(0, 1 .- ŷ .* y)).^2) / size(y, 2).

See also: hinge_loss

source
Flux.Losses.dice_coeff_lossFunction
dice_coeff_loss(ŷ, y; smooth = 1)

Return a loss based on the dice coefficient. Used in the V-Net image segmentation architecture. Similar to the F1_score. Calculated as:

1 - 2*sum(|ŷ .* y| + smooth) / (sum(ŷ.^2) + sum(y.^2) + smooth)
source
Flux.Losses.tversky_lossFunction
tversky_loss(ŷ, y; β = 0.7)

Return the Tversky loss. Used with imbalanced data to give more weight to false negatives. Larger β weigh recall more than precision (by placing more emphasis on false negatives) Calculated as: 1 - sum(|y .* ŷ| + 1) / (sum(y .* ŷ + β(1 .- y) . ŷ + (1 - β)y . (1 .- ŷ)) + 1)

source
Flux.Losses.binary_focal_lossFunction
binary_focal_loss(ŷ, y; agg=mean, γ=2, ϵ=eps(ŷ))

Return the binaryfocalloss The input, 'ŷ', is expected to be normalized (i.e. softmax output).

For γ == 0, the loss is mathematically equivalent to Losses.binarycrossentropy.

Example

julia> y = [0  1  0
            1  0  1]
2×3 Matrix{Int64}:
 0  1  0
 1  0  1

julia> ŷ = [0.268941  0.5  0.268941
            0.731059  0.5  0.731059]
2×3 Matrix{Float64}:
 0.268941  0.5  0.268941
 0.731059  0.5  0.731059

julia> Flux.binary_focal_loss(ŷ, y) ≈ 0.0728675615927385
true

See also: Losses.focal_loss for multi-class setting

source
Flux.Losses.focal_lossFunction
focal_loss(ŷ, y; dims=1, agg=mean, γ=2, ϵ=eps(ŷ))

Return the focal_loss which can be used in classification tasks with highly imbalanced classes. It down-weights well-classified examples and focuses on hard examples. The input, 'ŷ', is expected to be normalized (i.e. softmax output).

The modulating factor, γ, controls the down-weighting strength. For γ == 0, the loss is mathematically equivalent to Losses.crossentropy.

Example

julia> y = [1  0  0  0  1
            0  1  0  1  0
            0  0  1  0  0]
3×5 Matrix{Int64}:
 1  0  0  0  1
 0  1  0  1  0
 0  0  1  0  0

julia> ŷ = softmax(reshape(-7:7, 3, 5) .* 1f0)
3×5 Matrix{Float32}:
 0.0900306  0.0900306  0.0900306  0.0900306  0.0900306
 0.244728   0.244728   0.244728   0.244728   0.244728
 0.665241   0.665241   0.665241   0.665241   0.665241

julia> Flux.focal_loss(ŷ, y) ≈ 1.1277571935622628
true

See also: Losses.binary_focal_loss for binary (not one-hot) labels

source
Flux.Losses.siamese_contrastive_lossFunction
siamese_contrastive_loss(ŷ, y; margin = 1, agg = mean)

Return the contrastive loss which can be useful for training Siamese Networks. It is given by

agg(@. (1 - y) * ŷ^2 + y * max(0, margin - ŷ)^2)

Specify margin to set the baseline for distance at which pairs are dissimilar.

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