Neural Network primitives from NNlib.jl

Flux re-exports all of the functions exported by the NNlib package. This includes activation functions, described on their own page. Many of the functions on this page exist primarily as the internal implementation of Flux layer, but can also be used independently.

Attention

Primitives for the Attention layer.

NNlib.scaled_dot_product_attention — Function
scaled_dot_product_attention(query, key, value, [bias]; [fdrop, mask, scale, is_causal, q_offset, q_lengths, kv_lengths, q_segments, kv_segments, maxlen])
sdpa(query, key, value, [bias]; kws...)

Multihead dot product attention used in transformer architectures, with an explicit head axis.

The input arrays must have the shape (head_dim, nheads, seq_len, batch_size...), that is a feature (head) dimension, a heads dimension, a sequence-length dimension, then an arbitrary number of batch dimensions or none. The number of heads is taken from the second dimension of each input, so no nheads keyword is needed.

This is the reverse of the (batch_size, seq_len, nheads, head_dim) layout of JAX and Flax. It is not the reverse of PyTorch's (batch_size, nheads, seq_len, head_dim): an array ported from PyTorch by reversing its dimensions has size (head_dim, seq_len, nheads, batch_size) and still needs permutedims(x, (1, 3, 2, 4)). A missing permutation cannot be detected, since the array is a valid input whose heads are taken as the sequence.

Grouped-query attention (GQA) is supported: if key and value have fewer heads than query, they are shared across query heads. The number of query heads must then be divisible by the number of key/value heads.

Returns the attention output array of size (v_head_dim, nheads, q_len, batch_size...).

See also scaled_dot_product_attention_with_weights if you need the attention weights too.

Arguments

  • query: Query array of size (qk_head_dim, nheads, q_len, batch_size...).
  • key: Key array of size (qk_head_dim, nkvheads, kv_len, batch_size...).
  • value: Value array of size (v_head_dim, nkvheads, kv_len, batch_size...).
  • bias: Either nothing or an array broadcastable to size (kv_len, q_len, nheads, batch_size...). It will be added to the attention logits before applying the softmax. Default nothing.
  • fdrop: A dropout function or layer to be applied on the attention weights right after the softmax. Default identity (no dropout).
  • mask: Either nothing or a boolean array broadcastable to size (kv_len, q_len, nheads, batch_size...). The mask is applied to the attention logits just before the softmax. See make_causal_mask for creating causal masks. Default nothing.
  • scale: The multiplier used to scale the queryᵀ * key dot products before the softmax. Default nothing, meaning 1 / √(qk_head_dim).
  • is_causal: If true, a causal mask is applied so that each query position can only attend to key positions up to and including its own. Equivalent to mask = make_causal_mask(query; dims=3) for equal query and key lengths, but a fused implementation does not have to materialize the mask. If :bottom_right, the mask is aligned with the last valid key instead of the first: the queries are taken as the last positions of the keys, as when decoding with a KV cache, and q_offset is kv_lengths .- q_lengths, these being the sizes of the arrays where not given. This is the causal mask of FlashAttention and PyTorch's causal_lower_right. Default false.
  • q_offset: With is_causal=true, the number of keys that precede the first query: the query i attends to the keys j ≤ q_offset + i. An integer, or an integer array with one entry for each batch element. It counts the keys given, which with a sliding-window cache is not the absolute position. It has no effect without is_causal, and is set by is_causal=:bottom_right. Default 0.
  • q_lengths, kv_lengths: Either nothing or the number of valid positions of each query and of each key/value sequence in the batch, the following ones being padding: an integer array with one entry for each batch element, or an integer for all of them. The keys past kv_lengths are not attended to, and the output is zero at the queries past q_lengths. Each can be given without the other. Default nothing.
  • q_segments, kv_segments: Either nothing or the lengths of the sequences packed one after the other along the sequence dimension of query and of key and value, as an integer vector. See below. kv_segments defaults to q_segments.
  • maxlen: With q_segments, either nothing or an integer at least as large as every segment. It saves reading the lengths of the segments on the host where they are on a GPU, which waits for the device, and stands in for them where they cannot be read, as the traced ones of Reactant. Default nothing.

mask, is_causal and kv_lengths can be combined: a key is then attended to only where all of them allow it.

Packed sequences

With q_segments, the inputs hold sequences of different lengths one after the other, without padding: they have size (head_dim, nheads, total_len), without batch dimensions, and the output has the size of query. The s-th segment of query attends to the s-th segment of key and value only, as a batch element does in a padded batch: is_causal applies within each segment, and q_offset, q_lengths and kv_lengths take one entry for each segment. The lengths of the segments have to add up to the sequence lengths of the arrays. A bias or a mask is not supported.

This is how documents packed in a sequence are kept from attending to each other, and how a batch of sequences of different lengths avoids padding: layers other than the attention act on the (features, total_len) array of all the positions.

Fused implementation

Without an fdrop, the output is computed tile by tile, with the softmax taken online over the tiles of keys: the attention weights are never materialized, so that memory grows linearly rather than quadratically with the sequence length. This is what Arrays and GPU arrays of Float16, Float32 and Float64 take, and on the GPU those of BFloat16, with any of the arguments above. The bias and the mask, if any, have to be on the device of the inputs.

Any other call takes the materialized implementation, which forms the weights. NNlib.is_fused_attention tells which of the two a call takes.

The fused implementation has a gradient with respect to query, key, value and scale, which recomputes the weights tile by tile and does not materialize them either. It is what automatic differentiation based on ChainRules (as that of Zygote) and the reverse mode of Enzyme use. Under them a call with a bias takes the materialized implementation, which gives the gradient with respect to the bias too, and so does every call under the other automatic differentiation packages. A query that attends to no key, whose output is NaN, takes no part in the fused gradient.

With CUDA.jl and cuDNN.jl loaded, the Float16 and BFloat16 CuArrays that cuDNN's own fused kernel has an engine for are handed to it: it runs on tensor cores, and has a gradient. It supports scale, is_causal, q_lengths, kv_lengths and grouped-query attention, and requires:

  • no bias, fdrop or mask (that is nothing, identity and nothing);
  • with is_causal, a causal mask aligned with the first key: the default q_offset of zero, and for :bottom_right as many queries as keys, without q_lengths or kv_lengths;
  • a head dimension that is a multiple of 8 and at most 256;
  • a value with the same head dimension as query.

Examples

# (head_dim, nheads, seq_len, batch)
q = rand(Float32, 16, 8, 20, 4)
k = v = rand(Float32, 16, 8, 30, 4)
y = scaled_dot_product_attention(q, k, v)
# size(y) == (16, 8, 20, 4)

# grouped-query attention: 8 query heads sharing 2 key/value heads
q = rand(Float32, 16, 8, 20, 4)
k = v = rand(Float32, 16, 2, 30, 4)
y = scaled_dot_product_attention(q, k, v)

# a padded batch, whose first key/value sequence has 12 valid positions out of 30
y = scaled_dot_product_attention(q, k, v; kv_lengths=[12, 30, 30, 30])

# decoding with a KV cache of 64 positions: 3 new queries for each batch element,
# appended to the 10, 20, 30 and 40 keys already cached
q = rand(Float32, 16, 8, 3, 4)
k = v = rand(Float32, 16, 8, 64, 4)
y = scaled_dot_product_attention(q, k, v; is_causal=:bottom_right, kv_lengths=[13, 23, 33, 43])
# the same, with the offsets of the queries
y = scaled_dot_product_attention(q, k, v; is_causal=true, q_offset=[10, 20, 30, 40],
                                 kv_lengths=[13, 23, 33, 43])

# three documents of 5, 12 and 3 positions packed in one sequence, each attending
# causally to itself only
x = rand(Float32, 16, 8, 20)
y = scaled_dot_product_attention(x, x, x; is_causal=true, q_segments=[5, 12, 3])
# size(y) == (16, 8, 20)
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NNlib.scaled_dot_product_attention_with_weights — Function
scaled_dot_product_attention_with_weights(query, key, value, [bias]; kws...)
sdpa_with_weights(query, key, value, [bias]; kws...)

Return the output of scaled_dot_product_attention together with the attention weights it is computed from, in a single pass.

The arguments are those of scaled_dot_product_attention. The weights have size (kv_len, q_len, nheads, batch_size...), with α[j, i, h, b] the weight of the key j for the query i in the head h: the softmax over the keys of the attention logits, after fdrop. They are zero at the queries past q_lengths. With q_segments they have size (kv_len, q_len, nheads), and are zero but for the keys of the segment of each query.

Returning the weights means materializing them, so this function never takes a fused implementation: prefer scaled_dot_product_attention when they are not needed.

Examples

q = rand(Float32, 16, 8, 20, 4)
k = v = rand(Float32, 16, 8, 30, 4)
y, α = scaled_dot_product_attention_with_weights(q, k, v)
# size(y) == (16, 8, 20, 4)
# size(α) == (30, 20, 8, 4)
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NNlib.is_fused_attention — Function
NNlib.is_fused_attention(query, key, value, [bias]; kws...)

Return true if scaled_dot_product_attention called with the same arguments is computed by a fused implementation, which does not materialize the attention weights, and false if it takes the materialized one.

This is about a call outside of automatic differentiation: under it, the materialized implementation is differentiated where the fused one has no gradient, as with a bias.

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NNlib.make_causal_mask — Function
make_causal_mask(x; dims)

Return a boolean square matrix m of the same type as x and of side size(x, dims). Its elements are set such that m[i, j] == i ≤ j.

Can be used as the mask of scaled_dot_product_attention, whose inputs have the sequence length along dims=3. For a plain causal mask, prefer the is_causal=true keyword there, which lets a fused implementation avoid materializing the mask.

Calling make_causal_mask(x) without dims is deprecated. It keeps returning the mask for dims=2, the sequence dimension of the deprecated dot_product_attention.

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Softmax

Flux's Flux.logitcrossentropy uses NNlib.logsoftmax internally.

NNlib.softmax — Function
softmax(x; dims = 1)

Softmax turns input array x into probability distributions that sum to 1 along the dimensions specified by dims. It is semantically equivalent to the following:

softmax(x; dims = 1) = exp.(x) ./ sum(exp.(x), dims = dims)

with additional manipulations enhancing numerical stability. For Float16 and BFloat16 inputs, the sums are computed in Float32.

For a matrix input x it will by default (dims = 1) treat it as a batch of vectors, with each column independent. Keyword dims = 2 will instead treat rows independently, and so on.

See also logsoftmax.

Examples

julia> softmax([1, 2, 3])
3-element Vector{Float64}:
 0.09003057317038046
 0.24472847105479764
 0.6652409557748218

julia> softmax([1 2 3; 2 2 2])  # dims=1
2×3 Matrix{Float64}:
 0.268941  0.5  0.731059
 0.731059  0.5  0.268941

julia> softmax([1 2 3; 2 2 2]; dims=2)
2×3 Matrix{Float64}:
 0.0900306  0.244728  0.665241
 0.333333   0.333333  0.333333

Note that, when used with Flux.jl, softmax must not be passed to layers like Dense which accept an activation function. The activation is broadcasted over the result, thus applies to individual numbers. But softmax always needs to see the whole column.

julia> using Flux

julia> x = randn(Float32, 4, 4, 3, 13);

julia> model = Chain(Conv((4, 4), 3 => 8, tanh), Flux.flatten, Dense(8 => 7), softmax);

julia> model(x) |> size
(7, 13)

julia> Dense(4 => 7, softmax)(x)
ERROR: `softmax(x)` called with a number, but it expects an array. 
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NNlib.softmax! — Function
softmax!(out, x; dims = 1)
softmax!(x; dims = 1)

In-place version of softmax, writing the result into out (or x itself).

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NNlib.logsoftmax — Function
logsoftmax(x; dims = 1)

Computes the log of softmax in a more numerically stable way than directly taking log.(softmax(xs)). Commonly used in computing cross entropy loss.

It is semantically equivalent to the following:

logsoftmax(x; dims = 1) = x .- log.(sum(exp.(x), dims = dims))

For Float16 and BFloat16 inputs, the sum is computed in Float32.

See also softmax.

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Pooling

Flux's AdaptiveMaxPool, AdaptiveMeanPool, GlobalMaxPool, GlobalMeanPool, MaxPool, and MeanPool use NNlib.PoolDims, NNlib.maxpool, and NNlib.meanpool as their backend.

NNlib.PoolDims — Type
PoolDims(x_size::NTuple{M}, k::Union{NTuple{L, Int}, Int};
         stride=k, padding=0, dilation=1, ceil_mode=false)  where {M, L}

Dimensions for a "pooling" operation that can have an arbitrary input size, kernel size, stride, dilation, and channel count. Used to dispatch onto efficient implementations at compile-time.

With ceil_mode=true the output size is rounded up instead of down, as with PyTorch's ceil_mode=True: a last window that runs past the padded input is kept, as long as it starts inside the input or the low padding. Its positions past the padded input count neither as input nor as padding: max pooling skips them, and mean pooling leaves them out of the divisor even with count_include_pad=true. ceil_mode is dropped when it doesn't change the output size.

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NNlib.lpnormpool — Function
lpnormpool(x, p::Real, k::NTuple{N, Integer}; pad=0, stride=k, ceil_mode=false)

Perform Lp pool operation with value of the Lp norm p and window size k on input tensor x, also known as LPPool in pytorch. This pooling operator from Learned-Norm Pooling for Deep Feedforward and Recurrent Neural Networks.

Arguments:

  • x and k: Expects ndim(x) ∈ 3:5, and always length(k) == ndim(x) - 2
  • p is restricted to 0 < p < Inf.
  • pad: See pad_zeros for details.
  • stride: Either a tuple with the same length as k, or one integer for all directions. Default is k.
  • ceil_mode: When true, round the output size up instead of down: a last window that runs past the padded input is kept if it starts inside the input or the low padding. See PoolDims.

For all elements x in a size k window, lpnormpool computes (∑ᵢ xᵢ^p)^(1 / p) as an element of the output.

Thus lpnormpool(x, 1, k) ./ prod(k) ≈ meanpool(x, k) and lpnormpool(x, 2, k).^2 ./ prod(k) ≈ meanpool(x.^2, k). With ceil_mode=true, the sum of a last window that runs past the input is over its elements in the input; PyTorch's LPPool instead scales it by prod(k) over their number.

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NNlib.maxpool — Function
maxpool(x, k::NTuple{N, Integer}; pad=0, stride=k, ceil_mode=false)

Perform max pool operation with window size k on input tensor x.

Arguments:

  • x and k: Expects ndim(x) ∈ 3:5, and always length(k) == ndim(x) - 2
  • pad: See pad_zeros for details.
  • stride: Either a tuple with the same length as k, or one integer for all directions. Default is k.
  • ceil_mode: When true, round the output size up instead of down, as PyTorch's ceil_mode=True: a last window that runs past the padded input is kept if it starts inside the input or the low padding. See PoolDims.
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NNlib.meanpool — Function
meanpool(x, k::NTuple{N, Integer}; pad=0, stride=k, count_include_pad=true, ceil_mode=false)

Perform mean pool operation with window size k on input tensor x.

Arguments:

  • x and k: Expects ndim(x) ∈ 3:5, and always length(k) == ndim(x) - 2
  • pad: See pad_zeros for details.
  • stride: Either a tuple with the same length as k, or one integer for all directions. Default is k.
  • count_include_pad: When true (the default), padding (zero) elements are included in the averaging denominator, so each output element divides by the full window size prod(k). When false, only the in-bounds (non-padding) elements are counted, matching cuDNN's CUDNN_POOLING_AVERAGE_COUNT_EXCLUDE_PADDING and PyTorch's count_include_pad=false. Has no effect when pad == 0.
  • ceil_mode: When true, round the output size up instead of down, as PyTorch's ceil_mode=True: a last window that runs past the padded input is kept if it starts inside the input or the low padding. Its positions past the padded input are left out of the denominator also with count_include_pad=true, as in PyTorch. See PoolDims.
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Padding

NNlib.pad_circular — Function
pad_circular(x, pad::Tuple; [dims])
pad_circular(x, pad::Int; [dims])

Pad the array x "circularly" across the border by wrapping around values from the opposite side of x.

pad can a tuple of integers (l1, r1, ..., ln, rn) of some length 2n that specifies the left and right padding size for each of the dimensions in dims. If dims is not given, it defaults to the first n dimensions.

If pad is an integer, it is applied on both sides on every dimension in dims. In this case, dims defaults to the first ndims(x)-2 dimensions (i.e. excludes the channel and batch dimension).

The pad length on either side in any dimension must not exceed the size of x in that dimension, i.e. pad_circular is not able to create abitrary sized tilings of x.

See also pad_repeat, pad_reflect, pad_symmetric, and pad_constant.

julia> r = reshape(1:9, 3, 3)
3×3 reshape(::UnitRange{Int64}, 3, 3) with eltype Int64:
 1  4  7
 2  5  8
 3  6  9

julia> pad_circular(r, (1,2,1,2))
6×6 Matrix{Int64}:
 9  3  6  9  3  6
 7  1  4  7  1  4
 8  2  5  8  2  5
 9  3  6  9  3  6
 7  1  4  7  1  4
 8  2  5  8  2  5
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NNlib.pad_constant — Function
pad_constant(x, pad::Tuple, val = 0; [dims = :])
pad_constant(x, pad::Int, val = 0; [dims = :])

Pad the array x with the constant value val.

pad can be a tuple of integers. If it is of some length 2 * length(dims) that specifies the left and right padding size for each of the dimensions in dims as (l1, r1, ..., ln, rn). If supplied with a tuple of length length(dims) instead, it applies symmetric padding. If dims is not given, it defaults to all dimensions.

For integer pad input, it is applied on both sides on every dimension in dims.

See also pad_zeros, pad_repeat, pad_reflect, pad_symmetric, and pad_circular.

julia> r = reshape(1:4, 2, 2)
2×2 reshape(::UnitRange{Int64}, 2, 2) with eltype Int64:
 1  3
 2  4

julia> pad_constant(r, (1, 2, 3, 4), 8)
5×9 Matrix{Int64}:
 8  8  8  8  8  8  8  8  8
 8  8  8  1  3  8  8  8  8
 8  8  8  2  4  8  8  8  8
 8  8  8  8  8  8  8  8  8
 8  8  8  8  8  8  8  8  8

julia> pad_constant(r, 1, 8)
4×4 Matrix{Int64}:
 8  8  8  8
 8  1  3  8
 8  2  4  8
 8  8  8  8

julia> r = reshape(1:27, 3, 3, 3)
3×3×3 reshape(::UnitRange{Int64}, 3, 3, 3) with eltype Int64:
[:, :, 1] =
 1  4  7
 2  5  8
 3  6  9

[:, :, 2] =
 10  13  16
 11  14  17
 12  15  18

[:, :, 3] =
 19  22  25
 20  23  26
 21  24  27

julia> pad_constant(r, (2,1), dims = 1) # assymetric padding
6×3×3 Array{Int64, 3}:
[:, :, 1] =
 0  0  0
 0  0  0
 1  4  7
 2  5  8
 3  6  9
 0  0  0

[:, :, 2] =
  0   0   0
  0   0   0
 10  13  16
 11  14  17
 12  15  18
  0   0   0

[:, :, 3] =
  0   0   0
  0   0   0
 19  22  25
 20  23  26
 21  24  27
  0   0   0

julia> pad_constant(r, (2,1, 3), dims = (1,2)) # padding must always be either the same length as dims, or double it
ERROR: ArgumentError: Could not parse padding (2, 1, 3) and dims (1, 2)
Stacktrace:
[...]
source
NNlib.pad_reflect — Function
pad_reflect(x, pad::Tuple; [dims])
pad_reflect(x, pad::Int; [dims])

Pad the array x reflecting its values across the border.

pad can a tuple of integers (l1, r1, ..., ln, rn) of some length 2n that specifies the left and right padding size for each of the dimensions in dims. If dims is not given, it defaults to the first n dimensions.

If pad is an integer, it is applied on both sides on every dimension in dims. In this case, dims defaults to the first ndims(x)-2 dimensions (i.e. excludes the channel and batch dimension).

See also pad_repeat, pad_symmetric, pad_circular, and pad_constant.

julia> r = reshape(1:9, 3, 3)
3×3 reshape(::UnitRange{Int64}, 3, 3) with eltype Int64:
 1  4  7
 2  5  8
 3  6  9

julia> pad_reflect(r, (1,2,1,2))
6×6 Matrix{Int64}:
 5  2  5  8  5  2
 4  1  4  7  4  1
 5  2  5  8  5  2
 6  3  6  9  6  3
 5  2  5  8  5  2
 4  1  4  7  4  1
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NNlib.pad_repeat — Function
pad_repeat(x, pad::Tuple; [dims])
pad_repeat(x, pad::Int; [dims])

Pad the array x repeating the values on the border.

pad can a tuple of integers (l1, r1, ..., ln, rn) of some length 2n that specifies the left and right padding size for each of the dimensions in dims. If dims is not given, it defaults to the first n dimensions.

If pad is an integer, it is applied on both sides on every dimension in dims. In this case, dims defaults to the first ndims(x)-2 dimensions (i.e. excludes the channel and batch dimension).

See also pad_reflect, pad_symmetric, pad_circular, and pad_constant.

julia> r = reshape(1:9, 3, 3)
3×3 reshape(::UnitRange{Int64}, 3, 3) with eltype Int64:
 1  4  7
 2  5  8
 3  6  9

julia> pad_repeat(r, (1,2,3,4))
6×10 Matrix{Int64}:
 1  1  1  1  4  7  7  7  7  7
 1  1  1  1  4  7  7  7  7  7
 2  2  2  2  5  8  8  8  8  8
 3  3  3  3  6  9  9  9  9  9
 3  3  3  3  6  9  9  9  9  9
 3  3  3  3  6  9  9  9  9  9
source
NNlib.pad_symmetric — Function
pad_symmetric(x, pad::Tuple; [dims])
pad_symmetric(x, pad::Int; [dims])

Pad the array x reflecting its values symmetrically across the border, i.e. the border values of x are present in the padding values, in contrast to pad_reflect.

pad can a tuple of integers (l1, r1, ..., ln, rn) of some length 2n that specifies the left and right padding size for each of the dimensions in dims. If dims is not given, it defaults to the first n dimensions.

If pad is an integer, it is applied on both sides on every dimension in dims. In this case, dims defaults to the first ndims(x)-2 dimensions (i.e. excludes the channel and batch dimension).

See also pad_repeat, pad_reflect, pad_circular, and pad_constant.

julia> r = reshape(1:9, 3, 3)
3×3 reshape(::UnitRange{Int64}, 3, 3) with eltype Int64:
 1  4  7
 2  5  8
 3  6  9

julia> pad_symmetric(r, (1,2,1,2))
6×6 Matrix{Int64}:
 1  1  4  7  7  4
 1  1  4  7  7  4
 2  2  5  8  8  5
 3  3  6  9  9  6
 3  3  6  9  9  6
 2  2  5  8  8  5
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NNlib.pad_zeros — Function
pad_zeros(x, pad::Tuple; [dims])
pad_zeros(x, pad::Int; [dims])

Pad the array x with zeros. Equivalent to pad_constant with the constant equal to 0.

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Convolution

Flux's Conv and CrossCor layers use NNlib.DenseConvDims and NNlib.conv internally.

NNlib.conv — Function
conv(x, w; stride = 1, pad = 0, dilation = 1, flipped = false, groups = 1)

Apply convolution filter w to input x. x and w are 3d/4d/5d tensors in 1d/2d/3d convolutions respectively. They may have real or complex element types.

The dimensions are arranged as follows, with the spatial dimensions first:

  • x: (spatial..., channels_in, batch)
  • w: (spatial..., channels_in ÷ groups, channels_out)
  • output: (spatial_out..., channels_out, batch)

The output spatial size for each dimension is (spatial + 2*pad - (dilation*(spatial_w - 1) + 1)) ÷ stride + 1.

Keyword arguments

  • stride: stride of the filter (Int or tuple of one Int per spatial dimension).
  • pad: zero padding. An Int or tuple applies symmetric padding; a tuple of 2*ndims entries gives (left, right) padding per spatial dimension.
  • dilation: spacing between filter elements (atrous convolution).
  • flipped: if false (default), perform true mathematical convolution; if true, perform cross-correlation (the usual deep-learning convention).
  • groups: number of groups for grouped convolution.

Examples

julia> x = rand(Float32, 28, 28, 3, 16);  # (width, height, channels_in, batch)

julia> w = rand(Float32, 5, 5, 3, 8);     # (width, height, channels_in, channels_out)

julia> size(conv(x, w))                    # 28 - 5 + 1 = 24
(24, 24, 8, 16)

julia> size(conv(x, w; stride=2, pad=1))
(13, 13, 8, 16)
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NNlib.ConvDims — Type
ConvDims

Type system-level information about convolution dimensions. Critical for things like im2col!() to generate efficient code, and helpful to reduce the number of kwargs getting passed around.

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NNlib.depthwiseconv — Function
depthwiseconv(x, w; stride=1, pad=0, dilation=1, flipped=false)

Depthwise convolution operation with filter w on input x. x and w are 3d/4d/5d tensors in 1d/2d/3d convolutions respectively. The filter w has shape (spatial..., channel_multiplier, channels_in).

This is equivalent to a grouped conv with groups = channels_in, and is implemented in terms of it.

source
NNlib.DepthwiseConvDims — Type
DepthwiseConvDims

Concrete subclass of ConvDims for a depthwise convolution. Differs primarily due to characterization by C_in, C_mult, rather than C_in, C_out. Useful to be separate from DenseConvDims primarily for channel calculation differences.

source
NNlib.unfold — Function
unfold(x, kernel_size; stride = 1, pad = 0, dilation = 0, flipped = true)

Places sliding windows of x into a container tensor of size (num_windows, window_size, batchsize). The window size is determined by the prod(spatial dims of kernel)*input_channels. The number of sliding windows will match those of convolution (conv) with the same kernel_size and arguments. Note that by default conv flips the spatial dimensions of its kernel (default flipped=false), whereas unfold does not (default flipped=true). Uses NNlib.im2col! as backend.

See also fold, the adjoint/transpose operator and a potential inverse of unfold.

Example

The below example demonstrates that unfold uses the same sliding windows as conv. In general batched_mul + unfold should not be used to achieve convolution.

julia> x = reshape([100 2 3 40 5 6 700], 7, 1, 1);  # 1D data, 1 channel, batch of 1

julia> w = reshape([1 0 -1], 3, 1, 1);  # 1D conv kernel of length 3

julia> kws = (pad=1, stride=2, flipped=true);  # use same args for conv and unfold

julia> z = NNlib.unfold(x, size(w); kws...)
4×3×1 Array{Int64, 3}:
[:, :, 1] =
  0  100   2
  2    3  40
 40    5   6
  6  700   0

julia> y1 = conv(x, w; kws...)
4×1×1 Array{Int64, 3}:
[:, :, 1] =
  -2
 -38
  34
   6

julia> y2 = z ⊠ w  # ⊠ (\boxtimes) is NNlib.batched_mul
4×1×1 Array{Int64, 3}:
[:, :, 1] =
  -2
 -38
  34
   6
source
NNlib.fold — Function
fold(y, output_size, kernel_size; stride = 1, pad = 0, dilation = 0, flipped = true)

The adjoint/transpose operator of unfold. It accumulates sliding windows from the output of unfold into a container tensor of size output_size. An inverse to unfold may be obtained (in some cases) by using fold and accounting for scaling issues with a divisor (see example). Uses NNlib.col2im! as backend.

See also unfold.

Example

julia> x = reshape([100 2 3 40 5 6 700], 7, 1, 1);  # 1D data, 1 channel, batch of 1

julia> y = NNlib.unfold(x, (3,1,1))  # sliding window of size 3
5×3×1 Array{Int64, 3}:
[:, :, 1] =
 100   2    3
   2   3   40
   3  40    5
  40   5    6
   5   6  700

julia> z = NNlib.fold(y, size(x), (3,1,1))  # sum of contributions in y. 100 appears once, 40 three times
7×1×1 Array{Int64, 3}:
[:, :, 1] =
 100
   4
   9
 120
  15
  12
 700

julia> divisor = NNlib.fold(NNlib.unfold(ones(size(x)...), (3,1,1)), size(x), (3,1,1))
7×1×1 Array{Float64, 3}:
[:, :, 1] =
 1.0
 2.0
 3.0
 3.0
 3.0
 2.0
 1.0

julia> z ./ divisor
7×1×1 Array{Float64, 3}:
[:, :, 1] =
 100.0
   2.0
   3.0
  40.0
   5.0
   6.0
 700.0

In general, an inverse to unfold does not exist if divisor contains zeros.

source

Dropout

NNlib.dropout — Function
dropout([rng], A, p; [dims])

Returns an array in which each element of A is either replaced with zero, with probability p, or else multiplied by 1/(1-p).

By default every element is treated independently. With keyword dims=1, a choice is made for every value of the 1st index i.e. each row of a matrix is either zero or not.

Optional first argument is the random number generator used. Inside a Reactant-compiled function, pass one (e.g. a Reactant.ReactantRNG) to get a new mask on every call, since default_rng() there is seeded once at compile time.

Examples

julia> dropout(ones(2, 10), 0.2)
2×10 Matrix{Float64}:
 1.25  1.25  0.0   1.25  1.25  1.25  1.25  1.25  1.25  1.25
 1.25  1.25  1.25  0.0   1.25  1.25  0.0   1.25  1.25  1.25

julia> mean(dropout(ones(10^4, 5), 0.2), dims=1)
1×5 Matrix{Float64}:
 0.998  1.00075  0.99125  0.99575  1.00075

julia> dropout(ones(5, 5), 0.7, dims=1)  # whole row the same
5×5 Matrix{Float64}:
 3.33333  3.33333  3.33333  3.33333  3.33333
 0.0      0.0      0.0      0.0      0.0
 0.0      0.0      0.0      0.0      0.0
 3.33333  3.33333  3.33333  3.33333  3.33333
 0.0      0.0      0.0      0.0      0.0

julia> mean(dropout(ones(10^4, 5), 0.3, dims=1), dims=1)
1×5 Matrix{Float64}:
 1.00571  1.00571  1.00571  1.00571  1.00571
source
NNlib.dropout! — Function
dropout!(B, A, p; [dims])

This does exactly B .= dropout(A, p; dims), or rather, it's the implementation of out-of-place dropout.

source

Normalization

Flux's BatchNorm, InstanceNorm, GroupNorm, and LayerNorm layers wrap the functional normalization operators below as their backend.

NNlib.normalise — Function
normalise(x; dims=ndims(x), eps=1f-5)

Normalise x to zero mean and unit standard deviation across the dimension(s) given by dims. Per default, dims is the last dimension. eps is a small term added to the variance for numerical stability.

It is layernorm without scale and bias. For half-precision (Float16/BFloat16) inputs the statistics are computed in Float32.

Examples

julia> using Statistics

julia> x = [90, 100, 110, 130, 70];

julia> y = NNlib.normalise(x);

julia> isapprox(std(y; corrected=false), 1, atol=1e-5)
true
source
NNlib.batchnorm — Function
batchnorm(g, b, x, running_mean=nothing, running_var=nothing, momentum=0.1f0;
          eps=1f-5, training=true, track_stats=true)

Functional batch normalization. g and b are the per-channel scale and bias (either may be nothing for no affine transform); x are the feature maps. For an input with N dimensions the N-1th is the channel dimension (the usual convention for WHCN images); statistics are computed over every D_1×…×D_{N-2}×1×D_N slice, so per channel.

If running_mean/running_var are supplied:

  • with training=true (default) they are updated in place (when track_stats=true) with an exponential moving average controlled by momentum, while statistics of the current batch are used to normalise;
  • with training=false they are used to normalise (inference / test mode).

eps is added to the variance for numerical stability. On the GPU, 3D/4D/5D CuArrays are dispatched to the cuDNN implementation.

For half-precision (Float16/BFloat16) feature maps the statistics are computed in Float32 and the result is cast back; g, b, running_mean and running_var must then be Float32.

See also instancenorm, groupnorm, layernorm.

source
NNlib.instancenorm — Function
instancenorm(g, b, x, running_mean=nothing, running_var=nothing, momentum=0.1f0;
             eps=1f-5, training=true, track_stats=false)

Functional instance normalization. Arguments match batchnorm, but for an input with N > 2 dimensions statistics are computed over every D_1×…×D_{N-2}×1×1 slice, so per channel and per sample in the batch. When tracked, the running statistics (length size(x, N-1)) accumulate the per-channel average across the batch.

Normalising a dense CPU or GPU array with its own statistics, with g and b of length size(x, N-1), runs fused kernels; other cases use the generic code.

See also batchnorm, groupnorm, layernorm.

source
NNlib.groupnorm — Function
groupnorm(g, b, x, G::Integer; eps=1f-5)

Functional group normalization. g and b are the per-channel scale and bias (either may be nothing); x are the feature maps. For an input with N > 2 dimensions the N-1th is the channel dimension; its C = size(x, N-1) channels are split into G groups (G must divide C) and statistics are computed over each group together with the spatial dimensions, per sample. eps is added to the variance.

Normalising a dense CPU or GPU array, with g and b of length C, runs fused kernels; other cases use the generic code.

See also batchnorm, instancenorm, layernorm.

source
NNlib.layernorm — Function
layernorm(g, b, x; dims=1, eps=1f-5)

Functional layer normalization. g and b are the scale and bias (either may be nothing); x is normalised over the dimensions dims (the leading dimension by default).

g and b, when given, must broadcast against the normalised region, e.g. have size size(x)[dims] with singleton trailing dimensions.

Normalising a dense CPU or GPU array over leading dims (1:k), with g and b of the shape of those dimensions, runs fused kernels; other cases use the generic code.

See also normalise, batchnorm, instancenorm, groupnorm.

source
NNlib.rmsnorm — Function
rmsnorm(g, x; dims=1, eps=1f-5)

Functional root mean square normalization. x is divided by its root mean square over the dimensions dims (the leading dimension by default) and multiplied by the scale g (nothing for no scaling):

y = g .* x ./ sqrt.(mean(abs2, x; dims) .+ eps)

Unlike layernorm, the mean is not subtracted and there is no bias.

g, when given, must broadcast against the normalised region, e.g. have size size(x)[dims] with singleton trailing dimensions. eps is added to the mean square for numerical stability.

For half-precision (Float16/BFloat16) inputs the mean square is computed in Float32 and the result is cast back; g must then be Float32.

See also layernorm, normalise.

Examples

julia> x = Float32[3 0; 4 2];

julia> NNlib.rmsnorm(nothing, x) ≈ x ./ sqrt.(Float32[12.5 2])
true

julia> NNlib.rmsnorm(Float32[2, 1], x) ≈ Float32[2, 1] .* NNlib.rmsnorm(nothing, x)
true
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Upsampling

Flux's Upsample layer uses NNlib.upsample_nearest, NNlib.upsample_bilinear, and NNlib.upsample_trilinear as its backend. Additionally, Flux's PixelShuffle layer uses NNlib.pixel_shuffle as its backend.

NNlib.upsample_nearest — Function
upsample_nearest(x, scale::NTuple{S,Int})
upsample_nearest(x; size::NTuple{S,Int})

Upsamples the array x by integer multiples along the first S dimensions. Subsequent dimensions of x are not altered.

Either the scale factors or the final output size can be specified.

See also upsample_bilinear, for two dimensions of an N=4 array.

Example

julia> upsample_nearest([1 2 3; 4 5 6], (2, 3))
4×9 Matrix{Int64}:
 1  1  1  2  2  2  3  3  3
 1  1  1  2  2  2  3  3  3
 4  4  4  5  5  5  6  6  6
 4  4  4  5  5  5  6  6  6

julia> ans == upsample_nearest([1 2 3; 4 5 6]; size=(4, 9))  # equivalent
true

julia> upsample_nearest([1 2 3; 4 5 6], (2,))
4×3 Matrix{Int64}:
 1  2  3
 1  2  3
 4  5  6
 4  5  6

julia> ans == upsample_nearest([1 2 3; 4 5 6], size=(4,))
true
source
NNlib.upsample_linear — Function
upsample_linear(x::AbstractArray{T,3}, scale::Real; align_corners::Bool = true)
upsample_linear(x::AbstractArray{T,3}; size::Integer, align_corners::Bool = true)

Upsamples the first dimension of the array x by the upsample provided scale, using linear interpolation. As an alternative to using scale, the resulting array size can be directly specified with a keyword argument.

The size of the output is equal to (scale*S1, S2, S3), where S1, S2, S3 = size(x).

source
NNlib.upsample_bilinear — Function
upsample_bilinear(x::AbstractArray{T,4}, scale::NTuple{2,Real}; align_corners::Bool = true, antialias::Bool = false)
upsample_bilinear(x::AbstractArray{T,4}; size::NTuple{2,Integer}, align_corners::Bool = true, antialias::Bool = false)

Upsamples the first 2 dimensions of the array x by the upsample factors stored in scale, using bilinear interpolation. As an alternative to using scale, the resulting image size can be directly specified with a keyword argument.

The size of the output is equal to (scale[1]*S1, scale[2]*S2, S3, S4), where S1, S2, S3, S4 = size(x).

With antialias = true, the output can also be smaller than the input: as in PyTorch's F.interpolate(x, size, mode="bilinear", antialias=True) and PIL, the triangle filter is then stretched by the downsampling factor and renormalised at the borders. Pass align_corners = false to match them. See also upsample_bicubic.

Examples

julia> x = reshape(Float32[1 2 3; 4 5 6], (2,3,1,1))
2×3×1×1 Array{Float32, 4}:
[:, :, 1, 1] =
 1.0  2.0  3.0
 4.0  5.0  6.0

julia> upsample_bilinear(x, (2, 3))
4×9×1×1 Array{Float32, 4}:
[:, :, 1, 1] =
 1.0  1.25  1.5  1.75  2.0  2.25  2.5  2.75  3.0
 2.0  2.25  2.5  2.75  3.0  3.25  3.5  3.75  4.0
 3.0  3.25  3.5  3.75  4.0  4.25  4.5  4.75  5.0
 4.0  4.25  4.5  4.75  5.0  5.25  5.5  5.75  6.0

julia> ans == upsample_bilinear(x; size=(4, 9))  # specify ouput size instead
true

julia> upsample_bilinear(x, (2.5, 3.5))  # non-integer scaling factors are allowed
5×10×1×1 Array{Float32, 4}:
[:, :, 1, 1] =
 1.0   1.22222  1.44444  1.66667  1.88889  …  2.33333  2.55556  2.77778  3.0
 1.75  1.97222  2.19444  2.41667  2.63889     3.08333  3.30556  3.52778  3.75
 2.5   2.72222  2.94444  3.16667  3.38889     3.83333  4.05556  4.27778  4.5
 3.25  3.47222  3.69444  3.91667  4.13889     4.58333  4.80556  5.02778  5.25
 4.0   4.22222  4.44444  4.66667  4.88889     5.33333  5.55556  5.77778  6.0
source
NNlib.upsample_trilinear — Function
upsample_trilinear(x::AbstractArray{T,5}, scale::NTuple{3,Real}; align_corners::Bool = true)
upsample_trilinear(x::AbstractArray{T,5}; size::NTuple{3,Integer}, align_corners::Bool = true)

Upsamples the first 3 dimensions of the array x by the upsample factors stored in scale, using trilinear interpolation. As an alternative to using scale, the resulting image size can be directly specified with a keyword argument.

The size of the output is equal to (scale[1]*S1, scale[2]*S2, scale[3]*S3, S4, S5), where S1, S2, S3, S4, S5 = size(x).

Examples

upsample_trilinear(x, (2, 3, 4))
upsample_trilinear(x; size=(4, 9, 11))  # specify ouput size instead
upsample_trilinear(x, (2.5, 3.5, pi))  # non-integer scaling factors are allowed
source
NNlib.pixel_shuffle — Function
pixel_shuffle(x, r::Integer)

Pixel shuffling operation, upscaling by a factor r.

For 4-arrays representing N images, the operation converts input size(x) == (W, H, r^2*C, N) to output of size (r*W, r*H, C, N). For D-dimensional data, it expects ndims(x) == D+2 with channel and batch dimensions, and divides the number of channels by r^D.

Used in super-resolution networks to upsample towards high resolution features. Reference: Shi et. al., "Real-Time Single Image and Video Super-Resolution ...", CVPR 2016, https://arxiv.org/abs/1609.05158

Examples

julia> x = [10i + j + channel/10 for i in 1:2, j in 1:3, channel in 1:4, batch in 1:1]
2×3×4×1 Array{Float64, 4}:
[:, :, 1, 1] =
 11.1  12.1  13.1
 21.1  22.1  23.1

[:, :, 2, 1] =
 11.2  12.2  13.2
 21.2  22.2  23.2

[:, :, 3, 1] =
 11.3  12.3  13.3
 21.3  22.3  23.3

[:, :, 4, 1] =
 11.4  12.4  13.4
 21.4  22.4  23.4

julia> pixel_shuffle(x, 2)  # 4 channels used up as 2x upscaling of image dimensions
4×6×1×1 Array{Float64, 4}:
[:, :, 1, 1] =
 11.1  11.3  12.1  12.3  13.1  13.3
 11.2  11.4  12.2  12.4  13.2  13.4
 21.1  21.3  22.1  22.3  23.1  23.3
 21.2  21.4  22.2  22.4  23.2  23.4

julia> y = [i + channel/10 for i in 1:3, channel in 1:6, batch in 1:1]
3×6×1 Array{Float64, 3}:
[:, :, 1] =
 1.1  1.2  1.3  1.4  1.5  1.6
 2.1  2.2  2.3  2.4  2.5  2.6
 3.1  3.2  3.3  3.4  3.5  3.6

julia> pixel_shuffle(y, 2)  # 1D image, with 6 channels reduced to 3
6×3×1 Array{Float64, 3}:
[:, :, 1] =
 1.1  1.3  1.5
 1.2  1.4  1.6
 2.1  2.3  2.5
 2.2  2.4  2.6
 3.1  3.3  3.5
 3.2  3.4  3.6
source

Rotation

NNlib.imrotate — Function
imrotate(arr::AbstractArray{T, 4}, θ; method=:bilinear, rotation_center=size(arr) .÷ 2 .+ 1)

Rotates an array in the first two dimensions around the center pixel rotation_center. The default value of rotation_center is defined such that there is a integer center pixel for even and odd sized arrays which it is rotated around. For an even sized array of size (4,4) this would be (3,3), for an odd array of size (3,3) this would be (2,2) However, rotation_center can be also non-integer numbers if specified.

The angle θ is interpreted in radians.

The adjoint is defined with ChainRulesCore.jl. This method also runs with CUDA (and in principle all KernelAbstractions.jl supported backends).

Keywords

  • method=:bilinear for bilinear interpolation or method=:nearest for nearest neighbour
  • rotation_center=size(arr) .÷ 2 .+ 1 means there is a real center pixel around it is rotated.

Examples

julia> arr = zeros((4,4,1,1)); arr[2,2,1,1] = 1;

julia> arr
4×4×1×1 Array{Float64, 4}:
[:, :, 1, 1] =
 0.0  0.0  0.0  0.0
 0.0  1.0  0.0  0.0
 0.0  0.0  0.0  0.0
 0.0  0.0  0.0  0.0

julia> NNlib.imrotate(arr, deg2rad(90)) # rotation around (3,3)
4×4×1×1 Array{Float64, 4}:
[:, :, 1, 1] =
 0.0  0.0  0.0  0.0
 0.0  0.0  0.0  1.0
 0.0  0.0  0.0  0.0
 0.0  0.0  0.0  0.0

julia> NNlib.imrotate(arr, deg2rad(90), rotation_center=(2,2))
4×4×1×1 Array{Float64, 4}:
[:, :, 1, 1] =
 0.0  0.0  0.0  0.0
 0.0  1.0  0.0  0.0
 0.0  0.0  0.0  0.0
 0.0  0.0  0.0  0.0

julia> arr = zeros((3,3,1,1)); arr[1,2,1,1] = 1
1

julia> arr
3×3×1×1 Array{Float64, 4}:
[:, :, 1, 1] =
 0.0  1.0  0.0
 0.0  0.0  0.0
 0.0  0.0  0.0

julia> NNlib.imrotate(arr, deg2rad(45))
3×3×1×1 Array{Float64, 4}:
[:, :, 1, 1] =
 0.0  0.207107  0.0
 0.0  0.0       0.207107
 0.0  0.0       0.0

julia> NNlib.imrotate(arr, deg2rad(45), method=:nearest)
3×3×1×1 Array{Float64, 4}:
[:, :, 1, 1] =
 0.0  0.0  1.0
 0.0  0.0  0.0
 0.0  0.0  0.0
source

Batched Operations

Flux's Flux.Bilinear layer uses NNlib.batched_mul internally.

NNlib.batched_mul — Function
batched_mul(A, B) -> C
A ⊠ B  # \boxtimes

Batched matrix multiplication. Result has C[:,:,k...] == A[:,:,k...] * B[:,:,k...] where k... represent any indices in the last dimensions.

If ndims(A) == ndims(B) == 3 and size(B,3) == 1 then instead C[:,:,k] == A[:,:,k] * B[:,:,1], and similarly for A.

To transpose each matrix, apply batched_transpose to the array, or batched_adjoint for conjugate-transpose:

julia> A, B = randn(2,5,17), randn(5,9,17);

julia> A ⊠ B |> size
(2, 9, 17)

julia> batched_adjoint(A) |> size
(5, 2, 17)

julia> batched_mul(A, batched_adjoint(randn(9,5,17))) |> size
(2, 9, 17)

julia> A ⊠ randn(5,9,1) |> size
(2, 9, 17)

julia> batched_transpose(A) == PermutedDimsArray(A, (2,1,3))
true

The equivalent PermutedDimsArray may be used in place of batched_transpose. Other permutations are also handled by BLAS, provided that the batch index k is not the first dimension of the underlying array. Thus PermutedDimsArray(::Array, (1,3,2)) and PermutedDimsArray(::Array, (3,1,2)) are fine.

However, A = PermutedDimsArray(::Array, (3,2,1)) is not acceptable to BLAS, since the batch dimension is the contiguous one: stride(A,3) == 1. This will be copied, as doing so is faster than batched_mul_generic!.

Both this copy and batched_mul_generic! produce @debug messages, and setting for instance ENV["JULIA_DEBUG"] = NNlib will display them.

source
batched_mul(A::Array{T,3}, B::Matrix)
batched_mul(A::Matrix, B::Array{T,3})
A ⊠ B

This is always matrix-matrix multiplication, but either A or B may lack a batch index.

  • When B is a matrix, result has C[:,:,k] == A[:,:,k] * B[:,:] for all k.

  • When A is a matrix, then C[:,:,k] == A[:,:] * B[:,:,k]. This can also be done by reshaping and calling *, for instance A ⊡ B using TensorCore.jl, but is implemented here using batched_gemm instead of gemm.

julia> randn(16,8,32) ⊠ randn(8,4) |> size
(16, 4, 32)

julia> randn(16,8,32) ⊠ randn(8,4,1) |> size  # equivalent
(16, 4, 32)

julia> randn(16,8) ⊠ randn(8,4,32) |> size
(16, 4, 32)

See also batched_vec to regard B as a batch of vectors, A[:,:,k] * B[:,k].

source
NNlib.batched_mul! — Function
batched_mul!(C, A, B) -> C
batched_mul!(C, A, B, α=1, β=0)

In-place batched matrix multiplication, equivalent to mul!(C[:,:,k], A[:,:,k], B[:,:,k], α, β) for all k. If size(B,3) == 1 then every batch uses B[:,:,1] instead.

This will call batched_gemm! whenever possible. For real arrays this means that, for X ∈ [A,B,C], either stride(X,1)==1 or stride(X,2)==1, the latter may be caused by batched_transpose or by for instance PermutedDimsArray(::Array, (3,1,2)). Unlike batched_mul this will never make a copy.

For complex arrays, the wrapper made by batched_adjoint must be outermost to be seen. In this case the strided accepted by BLAS are more restricted, if stride(C,1)==1 then only stride(AorB::BatchedAdjoint,2) == 1 is accepted.

source
NNlib.batched_adjoint — Function
batched_transpose(A::AbstractArray{T,3})
batched_adjoint(A)

Equivalent to applying transpose or adjoint to each matrix A[:,:,k].

These exist to control how batched_mul behaves, as it operates on such matrix slices of an array with ndims(A)==3.

PermutedDimsArray(A, (2,1,3)) is equivalent to batched_transpose(A), and is also understood by batched_mul (and more widely supported elsewhere).

BatchedTranspose{T, S} <: AbstractBatchedMatrix{T, 3}
BatchedAdjoint{T, S}

Lazy wrappers analogous to Transpose and Adjoint, returned by batched_transpose etc.

source
NNlib.batched_transpose — Function
batched_transpose(A::AbstractArray{T,3})
batched_adjoint(A)

Equivalent to applying transpose or adjoint to each matrix A[:,:,k].

These exist to control how batched_mul behaves, as it operates on such matrix slices of an array with ndims(A)==3.

PermutedDimsArray(A, (2,1,3)) is equivalent to batched_transpose(A), and is also understood by batched_mul (and more widely supported elsewhere).

BatchedTranspose{T, S} <: AbstractBatchedMatrix{T, 3}
BatchedAdjoint{T, S}

Lazy wrappers analogous to Transpose and Adjoint, returned by batched_transpose etc.

source
NNlib.batched_vec — Function
batched_vec(A::AbstractArray{T,3}, B::AbstractMatrix)
batched_vec(A::AbstractArray{T,3}, b::AbstractVector)
batched_vec(A::AbstractArray, B::AbstractArray)

Batched matrix-vector multiplication. For the 3D case: the result has C[:,:,k] == A[:,:,k] * B[:,k] for all k, or else C[:,:,k] == A[:,:,k] * b for b::Vector.

For the general N-D case where ndims(A) == ndims(B) + 1: the result has C[:,k...] == A[:,:,k...] * B[:,k...] for all batch indices k.... The batch dimensions must match: size(A)[3:end] == size(B)[2:end].

With the same argument types, batched_mul(A, B) would regard B as a fixed matrix, not a batch of vectors. Both reshape and then call batched_mul(::Array{T,3}, ::Array{T,3}).

julia> A, B, b = randn(16,8,32), randn(8,32), randn(8);

julia> batched_vec(A,B) |> size
(16, 32)

julia> batched_vec(A,b) |> size
(16, 32)

julia> A4d, B3d = randn(16,8,10,32), randn(8,10,32);  # 4D and 3D arrays

julia> batched_vec(A4d, B3d) |> size
(16, 10, 32)
source

Gather and Scatter

Flux's Embedding layer uses NNlib.gather as its backend.

NNlib.gather — Function
NNlib.gather(src, idx) -> dst

Reverse operation of scatter. Gathers data from source src and writes it in a destination dst according to the index array idx. For each k in CartesianIndices(idx), assign values to dst according to

dst[:, ... , k] .= src[:, ... , idx[k]...]

Notice that if idx is a vector containing integers and src is a matrix, previous expression simplifies to

dst[:, k] .= src[:, idx[k]]

and k will run over 1:length(idx).

The elements of idx can be integers or integer tuples and may be repeated. A single src column can end up being copied into zero, one, or multiple dst columns.

See gather! for an in-place version.

Examples

julia> NNlib.gather([1,20,300,4000], [2,4,2])
3-element Vector{Int64}:
   20
 4000
   20

julia> NNlib.gather([1 2 3; 4 5 6], [1,3,1,3,1])
2×5 Matrix{Int64}:
 1  3  1  3  1
 4  6  4  6  4
source
gather(src, IJK...)

Convert the tuple of integer vectors IJK to a tuple of CartesianIndex and call gather on it: gather(src, CartesianIndex.(IJK...)).

Examples

julia> src = reshape([1:15;], 3, 5)
3×5 Matrix{Int64}:
 1  4  7  10  13
 2  5  8  11  14
 3  6  9  12  15

julia> NNlib.gather(src, [1, 2], [2, 4])
2-element Vector{Int64}:
  4
 11
source
NNlib.gather! — Function
NNlib.gather!(dst, src, idx)

Reverse operation of scatter!. Gathers data from source src and writes it in destination dst according to the index array idx. For each k in CartesianIndices(idx), assign values to dst according to

dst[:, ... , k] .= src[:, ... , idx[k]...]

Notice that if idx is a vector containing integers, and both dst and src are matrices, previous expression simplifies to

dst[:, k] .= src[:, idx[k]]

and k will run over 1:length(idx).

The elements of idx can be integers or integer tuples and may be repeated. A single src column can end up being copied into zero, one, or multiple dst columns.

See gather for an allocating version.

source
gather!(dst, src, IJK...)

Convert the tuple of integer vectors IJK to a tuple of CartesianIndex and call gather! on it: gather!(dst, src, CartesianIndex.(IJK...)).

Examples

julia> src = reshape([1:15;], 3, 5)
3×5 Matrix{Int64}:
 1  4  7  10  13
 2  5  8  11  14
 3  6  9  12  15

julia> dst = zeros(Int, 2);

julia> NNlib.gather!(dst, src, [1, 2], [2, 4])
2-element Vector{Int64}:
  4
 11
source
NNlib.scatter — Function
NNlib.scatter(op, src, idx; [init, dstsize])

Scatter operation allocating a destination array dst and calling scatter!(op, dst, src, idx) on it.

  • If keyword init is provided, it is used to initialize the content of dst. Otherwise, the init values is inferred from the reduction operator op for some common operators (e.g. init = 0 for op = +).

  • If dstsize is provided, it will be used to define the size of destination array, otherwise it will be inferred by src and idx.

See scatter! for full details on how idx works.

Examples

julia> NNlib.scatter(+, [10,100,1000], [3,1,2])
3-element Vector{Int64}:
  100
 1000
   10

julia> NNlib.scatter(+, [1 2 3 4; 5 6 7 8], [2,1,1,5])
2×5 Matrix{Int64}:
  5  1  0  0  4
 13  5  0  0  8

julia> NNlib.scatter(*, [10,200,3000], [1,4,2]; init = 10, dstsize = 6)
6-element Vector{Int64}:
   100
 30000
    10
  2000
    10
    10
source
NNlib.scatter! — Function
NNlib.scatter!(op, dst, src, idx)

Scatter operation, which writes data in src into dst at locations idx. A binary reduction operator op is applied during the scatter. For each index k in idx, accumulates values in dst according to

dst[:, ..., idx[k]...] = (op).(dst[:, ..., idx[k]...], src[:, ..., k...])

See also scatter, gather.

Arguments

  • op: Operations to be applied on dst and src, e.g. +, -, *, /, max, min and mean.
  • dst: The destination for src to aggregate to. This argument will be mutated.
  • src: The source data for aggregating.
  • idx: The mapping for aggregation from source (index) to destination (value). The idx array can contain either integers or tuples.

Examples

julia> NNlib.scatter!(+, ones(3), [10,100], [1,3])
3-element Vector{Float64}:
  11.0
   1.0
 101.0

julia> NNlib.scatter!(*, fill(0.5, 2, 4), [1 10; 100 1000], [3,2])
2×4 Matrix{Float64}:
 0.5    5.0   0.5  0.5
 0.5  500.0  50.0  0.5
source

Sampling

NNlib.grid_sample — Function
grid_sample(input::AbstractArray{T, 4}, grid::AbstractArray{T, 4}; padding_mode = :zeros)
grid_sample(input::AbstractArray{T, 5}, grid::AbstractArray{T, 4}; padding_mode = :zeros)

Given `input`, compute output by sampling `input` values at pixel
locations from `grid`. Uses bilinear interpolation to calculate output values.

This implementation assumes the extrema (`-1` and `1`) are considered
as referring to the center points of the input’s corner pixels
(i.e. align corners is `true`).

# Arguments

- `input`: Input array in `(W_in, H_in, [D_in,] C, N)` shape.
- `grid`: Input grid in `(2, W_out, H_out, [D_out,] N)` shape.
    Where for each `(W_out, H_out, [D_out,] N)` grid contains `(x, y [,z])`
    coordinates that specify sampling locations normalized by the `input` shape.

    Therefore, `x`, `y` and [`z`] should have values in `[-1, 1]` range.
    For example, `(x = -1, y = -1, [z = -1])` is the left-top[-front] pixel of `input`,
    and `(x = 1, y = 1, [z = 1])` is the right-bottom-back pixel of `input`.

    Out-of-bound values are handled according to the `padding_mode`.
- `padding_mode`: Out-of-bound padding.
    `:zeros` to use `0` for out-of-bound grid locations.
    `:border` to use border values for out-of-bound grid locations.
    Default is `:zeros`.

# Returns

`(W_out, H_out, [D_out,] C, N)` sampled grid from `input`.

# Examples

In the example below, grid contains two out-of-bound sampling locations,
which are handled differently, depending on the `padding_mode`.

```jldoctest
julia> x = reshape(collect(1.0:4.0), (2, 2, 1, 1))
2×2×1×1 Array{Float64, 4}:
[:, :, 1, 1] =
1.0  3.0
2.0  4.0

julia> grid = Array{Float64}(undef, 2, 3, 2, 1);

julia> grid[:, 1, 1, 1] .= (-3, -1);

julia> grid[:, 2, 1, 1] .= (0, -1);

julia> grid[:, 3, 1, 1] .= (1, -1);

julia> grid[:, 1, 2, 1] .= (-1, 1);

julia> grid[:, 2, 2, 1] .= (0, 1);

julia> grid[:, 3, 2, 1] .= (3, 1);

julia> grid_sample(x, grid; padding_mode=:zeros)
3×2×1×1 Array{Float64, 4}:
[:, :, 1, 1] =
0.0  3.0
1.5  3.5
2.0  0.0

julia> grid_sample(x, grid; padding_mode=:border)
3×2×1×1 Array{Float64, 4}:
[:, :, 1, 1] =
1.0  3.0
1.5  3.5
2.0  4.0
```
source

Audio

The spectral functions require the FFTW package to be loaded.

NNlib.hann_window — Function
hann_window(
    window_length::Int, ::Type{T} = Float32; periodic::Bool = true,
) where T <: Real

Hann window function (ref: Window function § Hann and Hamming windows - Wikipedia).

$w[n] = \frac{1}{2}[1 - \cos(\frac{2 \pi n}{N - 1})]$

Where $N$ is the window length.

julia> lineplot(hann_window(100); width=30, height=10)
     ┌──────────────────────────────┐
   1 │⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⣠⠚⠉⠉⠉⠢⡀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⡔⠁⠀⠀⠀⠀⠀⠘⢄⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⠀⠀⠀⠀⢀⠞⠀⠀⠀⠀⠀⠀⠀⠀⠈⢆⠀⠀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⠀⠀⠀⢀⡎⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠈⢣⠀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⠀⠀⠀⡎⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠈⢦⠀⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⠀⢀⠞⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠈⢆⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⢀⡜⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠈⢇⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⢀⠎⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠈⢦⠀⠀⠀⠀│
     │⠀⠀⠀⢠⠊⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠣⡀⠀⠀│
   0 │⣀⣀⠔⠁⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠙⢤⣀│
     └──────────────────────────────┘
     ⠀0⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀100⠀

Arguments:

  • window_length::Int: Size of the window.
  • ::Type{T}: Elemet type of the window.

Keyword Arguments:

  • periodic::Bool: If true (default), returns a window to be used as periodic function. If false, return a symmetric window.

    Following always holds:

julia> N = 256;

julia> hann_window(N; periodic=true) ≈ hann_window(N + 1; periodic=false)[1:end - 1]
true

julia> hann_window(N) ≈ hamming_window(N; α=0.5f0, β=0.5f0)
true

Returns:

Vector of length window_length and eltype T.

source
NNlib.hamming_window — Function
hamming_window(
    window_length::Int, ::Type{T} = Float32; periodic::Bool = true,
    α::T = T(0.54), β::T = T(0.46),
) where T <: Real

Hamming window function (ref: Window function § Hann and Hamming windows - Wikipedia). Generalized version of hann_window.

$w[n] = \alpha - \beta \cos(\frac{2 \pi n}{N - 1})$

Where $N$ is the window length.

julia> lineplot(hamming_window(100); width=30, height=10)
     ┌──────────────────────────────┐
   1 │⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⡠⠚⠉⠉⠉⠢⡄⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⢀⠎⠁⠀⠀⠀⠀⠀⠈⢢⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⠀⠀⠀⠀⢠⠊⠀⠀⠀⠀⠀⠀⠀⠀⠀⢣⡀⠀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⠀⠀⠀⢰⠃⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠱⡀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⠀⠀⣠⠃⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠳⡀⠀⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⠀⢰⠁⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠱⡄⠀⠀⠀⠀⠀│
     │⠀⠀⠀⠀⠀⡰⠃⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠱⡀⠀⠀⠀⠀│
     │⠀⠀⠀⢀⠴⠁⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠘⢄⠀⠀⠀│
     │⠀⢀⡠⠊⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠳⣀⠀│
   0 │⠉⠉⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠉│
     └──────────────────────────────┘
     ⠀0⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀100⠀

Arguments:

  • window_length::Int: Size of the window.
  • ::Type{T}: Elemet type of the window.

Keyword Arguments:

  • periodic::Bool: If true (default), returns a window to be used as periodic function. If false, return a symmetric window.

    Following always holds:

julia> N = 256;

julia> hamming_window(N; periodic=true) ≈ hamming_window(N + 1; periodic=false)[1:end - 1]
true
  • α::Real: Coefficient α in the equation above.
  • β::Real: Coefficient β in the equation above.

Returns:

Vector of length window_length and eltype T.

source
NNlib.stft — Function
stft(x;
    n_fft::Int, hop_length::Int = n_fft ÷ 4, window = nothing,
    center::Bool = true, normalized::Bool = false,
)

Short-time Fourier transform (STFT).

The STFT computes the Fourier transform of short overlapping windows of the input, giving frequency components of the signal as they change over time.

$Y[\omega, m] = \sum_{k = 0}^{N - 1} \text{window}[k] \text{input}[m \times \text{hop length} + k] \exp(-j \frac{2 \pi \omega k}{\text{n fft}})$

where $N$ is the window length, $\omega$ is the frequency $0 \le \omega < \text{n fft}$ and $m$ is the index of the sliding window.

Arguments:

  • x: Input, must be either a 1D time sequence ((L,) shape) or a 2D batch of time sequence ((L, B) shape).

Keyword Arguments:

  • n_fft::Int: Size of Fourier transform.
  • hop_length::Int: Distance between neighboring sliding window frames.
  • window: Optional window function to apply. Must be 1D vector 0 < length(window) ≤ n_fft. If window is shorter than n_fft, it is padded with zeros on both sides. If nothing (default), then no window is applied.
  • center::Bool: Whether to pad input on both sides so that $t$-th frame is centered at time $t \times \text{hop length}$. Padding is done with pad_reflect function.
  • normalized::Bool: Whether to return normalized STFT, i.e. multiplied with $\text{n fft}^{-0.5}$.

Returns:

Complex array of shape (n_fft, n_frames, B), where B is the optional batch dimension.

source
NNlib.istft — Function
istft(y;
    n_fft::Int, hop_length::Int = n_fft ÷ 4, window = nothing,
    center::Bool = true, normalized::Bool = false,
    return_complex::Bool = false,
    original_length::Union{Nothing, Int} = nothing,
)

Inverse Short-time Fourier Transform.

Return the least squares estimation of the original signal (D. Griffin and J. Lim, "Signal estimation from modified short-time Fourier transform", 1984): the inverse transforms of the frames are multiplied by the window, overlap-added, and divided by the overlap-added squared window. Samples where the latter vanishes (e.g. the first one for center=false and a hann_window) cannot be recovered and are set to zero.

Arguments:

  • y: Input complex array in the (n_fft, n_frames, B) shape. Where B is the optional batch dimension.

Keyword Arguments:

  • n_fft::Int: Size of Fourier transform.
  • hop_length::Int: Distance between neighboring sliding window frames.
  • window: Window function that was applied to the input of stft. If nothing (default), then no window was applied.
  • center::Bool: Whether input to stft was padded on both sides so that $t$-th frame is centered at time $t \times \text{hop length}$. Padding is done with pad_reflect function.
  • normalized::Bool: Whether input to stft was normalized.
  • return_complex::Bool: Whether the output should be complex, or if the input should be assumed to derive from a real signal and window.
  • original_length::Union{Nothing, Int}: Optional size of the first dimension of the input to stft. Helps restoring the exact stft input size. Otherwise, the array might be a bit shorter.
source
NNlib.spectrogram — Function
spectrogram(waveform;
    pad::Int = 0, n_fft::Int, hop_length::Int, window,
    center::Bool = true, power::Real = 2.0,
    normalized::Bool = false, window_normalized::Bool = false,
)

Create a spectrogram or a batch of spectrograms from a raw audio signal.

Arguments

  • pad::Int: Then amount of padding to apply on both sides.
  • window_normalized::Bool: Whether to normalize the waveform by the window’s L2 energy.
  • power::Real: Exponent for the magnitude spectrogram (must be ≥ 0) e.g., 1 for magnitude, 2 for power, etc. If 0, complex spectrum is returned instead.

See stft for other arguments.

Returns

Spectrogram in the shape (T, F, B), where T is the number of window hops and F = n_fft ÷ 2 + 1.

source
NNlib.melscale_filterbanks — Function
melscale_filterbanks(;
    n_freqs::Int, n_mels::Int, sample_rate::Int,
    fmin::Float32 = 0f0, fmax::Float32 = Float32(sample_rate ÷ 2))

Create triangular Mel scale filter banks (ref: Mel scale - Wikipedia). Each column is a filterbank that highlights its own frequency.

Arguments:

  • n_freqs::Int: Number of frequencies to highlight.
  • n_mels::Int: Number of mel filterbanks.
  • sample_rate::Int: Sample rate of the audio waveform.
  • fmin::Float32: Minimum frequency in Hz.
  • fmax::Float32: Maximum frequency in Hz.

Returns:

Filterbank matrix of shape (n_freqs, n_mels) where each column is a filterbank.

julia> n_mels = 8;

julia> fb = melscale_filterbanks(; n_freqs=200, n_mels, sample_rate=16000);

julia> plot = lineplot(fb[:, 1]);

julia> for i in 2:n_mels
           lineplot!(plot, fb[:, i])
       end

julia> plot
     ┌────────────────────────────────────────┐
   1 │⠀⡀⢸⠀⢸⠀⠀⣧⠀⠀⢸⡄⠀⠀⠀⣷⠀⠀⠀⠀⠀⣷⠀⠀⠀⠀⠀⠀⢀⣿⡀⠀⠀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⡇⢸⡆⢸⡇⠀⣿⠀⠀⡜⡇⠀⠀⢰⠋⡆⠀⠀⠀⢰⠁⡇⠀⠀⠀⠀⠀⡸⠀⢣⠀⠀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⣿⢸⡇⡇⡇⢰⠹⡄⠀⡇⢱⠀⠀⢸⠀⢣⠀⠀⠀⡜⠀⢸⡀⠀⠀⠀⢀⠇⠀⠈⡇⠀⠀⠀⠀⠀⠀⠀⠀│
     │⠀⣿⡇⡇⡇⡇⢸⠀⡇⢀⠇⠸⡀⠀⡇⠀⠸⡀⠀⢀⠇⠀⠀⢇⠀⠀⠀⡸⠀⠀⠀⠸⡄⠀⠀⠀⠀⠀⠀⠀│
     │⢠⢻⡇⡇⡇⢱⢸⠀⢇⢸⠀⠀⡇⢀⠇⠀⠀⡇⠀⢸⠀⠀⠀⠸⡀⠀⢠⠇⠀⠀⠀⠀⢱⠀⠀⠀⠀⠀⠀⠀│
     │⢸⢸⡇⢱⡇⢸⡇⠀⢸⢸⠀⠀⢣⢸⠀⠀⠀⢸⠀⡇⠀⠀⠀⠀⢇⠀⡜⠀⠀⠀⠀⠀⠈⢇⠀⠀⠀⠀⠀⠀│
     │⢸⢸⡇⢸⠀⢸⡇⠀⢸⡇⠀⠀⢸⡎⠀⠀⠀⠈⣶⠁⠀⠀⠀⠀⠸⣤⠃⠀⠀⠀⠀⠀⠀⠘⡆⠀⠀⠀⠀⠀│
     │⢸⠀⡇⢸⠀⠀⡇⠀⠀⡇⠀⠀⠀⡇⠀⠀⠀⠀⣿⠀⠀⠀⠀⠀⠀⣿⠀⠀⠀⠀⠀⠀⠀⠀⢱⡀⠀⠀⠀⠀│
     │⢸⢸⡇⢸⠀⢸⡇⠀⢸⡇⠀⠀⢸⢇⠀⠀⠀⢀⠿⡀⠀⠀⠀⠀⢰⠛⡄⠀⠀⠀⠀⠀⠀⠀⠀⢣⠀⠀⠀⠀│
     │⢸⢸⡇⡸⡇⢸⡇⠀⢸⢸⠀⠀⡜⢸⠀⠀⠀⢸⠀⡇⠀⠀⠀⠀⡎⠀⢣⠀⠀⠀⠀⠀⠀⠀⠀⠘⡆⠀⠀⠀│
     │⢸⢸⡇⡇⡇⡸⢸⠀⡎⢸⠀⠀⡇⠈⡆⠀⠀⡇⠀⢸⠀⠀⠀⢰⠁⠀⠘⡆⠀⠀⠀⠀⠀⠀⠀⠀⠸⡄⠀⠀│
     │⡇⢸⡇⡇⡇⡇⢸⠀⡇⠈⡆⢰⠁⠀⡇⠀⢰⠁⠀⠈⡆⠀⠀⡎⠀⠀⠀⢱⠀⠀⠀⠀⠀⠀⠀⠀⠀⢣⠀⠀│
     │⡇⢸⢸⡇⡇⡇⠸⣰⠃⠀⡇⡸⠀⠀⢸⠀⡜⠀⠀⠀⢣⠀⢸⠁⠀⠀⠀⠈⡆⠀⠀⠀⠀⠀⠀⠀⠀⠈⢇⠀│
     │⡇⡇⢸⠇⢸⡇⠀⣿⠀⠀⢣⡇⠀⠀⠸⣄⠇⠀⠀⠀⠸⡀⡇⠀⠀⠀⠀⠀⢱⠀⠀⠀⠀⠀⠀⠀⠀⠀⠸⡄│
   0 │⣇⣇⣸⣀⣸⣀⣀⣟⣀⣀⣸⣃⣀⣀⣀⣿⣀⣀⣀⣀⣀⣿⣀⣀⣀⣀⣀⣀⣈⣇⣀⣀⣀⣀⣀⣀⣀⣀⣀⣱│
     └────────────────────────────────────────┘
     ⠀0⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀⠀200⠀
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Miscellaneous

NNlib.logsumexp — Function
logsumexp(x; dims = :)

Computes log.(sum(exp.(x); dims)) in a numerically stable way. Without dims keyword this returns a scalar. For Float16 and BFloat16 inputs, it is computed and returned in Float32.

See also logsoftmax.

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NNlib.within_gradient — Function
within_gradient(x) --> Bool

Returns false except when used inside a gradient call, when it returns true. Useful for Flux regularisation layers which behave differently during training and inference.

This should work with any ChainRules-based differentiation package, in which case x is ignored. But Tracker.jl overloads within_gradient(x::TrackedArray), thus for widest use you should pass it an array whose gradient is of interest. There is also an overload for ForwardDiff.jl's Dual types (and arrays of them). Enzyme.jl and Mooncake.jl are supported through package extensions, and ignore x too.

Examples

julia> using ForwardDiff, Zygote, NNlib

julia> f_good(x) = if NNlib.within_gradient(x)
                     @show 10x
                   else
                     x
                   end;

julia> Zygote.withgradient(f_good, 1.0)
10x = 10.0
(val = 10.0, grad = (10.0,))

julia> ForwardDiff.derivative(f_good, 1.0)
10x = Dual{ForwardDiff.Tag{typeof(f_good), Float64}}(10.0,10.0)
10.0

julia> f_bad(x, y) = if any(NNlib.within_gradient, (x, y))
                       @show x * y
                     else
                       x / y
                     end;

julia> Zygote.withgradient(f_bad, 2.0, 3.0)
(val = 0.6666666666666666, grad = (0.3333333333333333, -0.2222222222222222))

julia> ForwardDiff.derivative(x -> f_bad(x, 3.0), 2.0)
x * y = Dual{ForwardDiff.Tag{var"#9#10", Float64}}(6.0,3.0)
3.0

What goes wrong in f_bad is that Zygote knows any to be non-differentiable, and thus completely ignores its contents. This is not a perfect mechanism, and the only style recommended is precisely that of f_good above.

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NNlib.bias_act! — Function
bias_act!(σ, x, b)

This is equivalent to x .= σ.(x .+ b), also replacing sigmoid & tanh with sigmoid_fast & tanh_fast. It will only overwrite x when x isa StridedArray{<:AbstractFloat}.

When used within a gradient, it will overwrite only when σ has a method of derivatives_given_output which does not need the input at all. Such methods are defined by e.g. @scalar_rule relu(x) Ω > 0 where the derivative contains only Ω (the output) not x.

Warning

This is not safe to use if x is still needed for the gradient of some other function. Incorrect use will give silently wrong answers. It is intended mainly for Flux layers, in which the previous operation is known to be safe, e.g. bias_act!(σ, weight * input, bias) for a Dense layer.

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