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: Eithernothingor an array broadcastable to size(kv_len, q_len, nheads, batch_size...). It will be added to the attention logits before applying the softmax. Defaultnothing.fdrop: A dropout function or layer to be applied on the attention weights right after the softmax. Defaultidentity(no dropout).mask: Eithernothingor 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. Seemake_causal_maskfor creating causal masks. Defaultnothing.scale: The multiplier used to scale thequeryᵀ * keydot products before the softmax. Defaultnothing, meaning1 / √(qk_head_dim).is_causal: Iftrue, a causal mask is applied so that each query position can only attend to key positions up to and including its own. Equivalent tomask = 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, andq_offsetiskv_lengths .- q_lengths, these being the sizes of the arrays where not given. This is the causal mask of FlashAttention and PyTorch'scausal_lower_right. Defaultfalse.q_offset: Withis_causal=true, the number of keys that precede the first query: the queryiattends to the keysj ≤ 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 withoutis_causal, and is set byis_causal=:bottom_right. Default0.q_lengths,kv_lengths: Eithernothingor 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 pastkv_lengthsare not attended to, and the output is zero at the queries pastq_lengths. Each can be given without the other. Defaultnothing.q_segments,kv_segments: Eithernothingor the lengths of the sequences packed one after the other along the sequence dimension ofqueryand ofkeyandvalue, as an integer vector. See below.kv_segmentsdefaults toq_segments.maxlen: Withq_segments, eithernothingor 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. Defaultnothing.
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,fdropormask(that isnothing,identityandnothing); - with
is_causal, a causal mask aligned with the first key: the defaultq_offsetof zero, and for:bottom_rightas many queries as keys, withoutq_lengthsorkv_lengths; - a head dimension that is a multiple of 8 and at most 256;
- a
valuewith the same head dimension asquery.
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)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)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.
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.
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 0.333333Note 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. 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).
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.
NNlib.logsoftmax! — Function
logsoftmax!(out, x; dims = 1)
logsoftmax!(x; dims = 1)In-place version of logsoftmax, writing the result into out (or x itself).
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.
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:
xandk: Expectsndim(x) ∈ 3:5, and alwayslength(k) == ndim(x) - 2pis restricted to0 < p < Inf.pad: Seepad_zerosfor details.stride: Either a tuple with the same length ask, or one integer for all directions. Default isk.ceil_mode: Whentrue, 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. SeePoolDims.
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.
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:
xandk: Expectsndim(x) ∈ 3:5, and alwayslength(k) == ndim(x) - 2pad: Seepad_zerosfor details.stride: Either a tuple with the same length ask, or one integer for all directions. Default isk.ceil_mode: Whentrue, round the output size up instead of down, as PyTorch'sceil_mode=True: a last window that runs past the padded input is kept if it starts inside the input or the low padding. SeePoolDims.
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:
xandk: Expectsndim(x) ∈ 3:5, and alwayslength(k) == ndim(x) - 2pad: Seepad_zerosfor details.stride: Either a tuple with the same length ask, or one integer for all directions. Default isk.count_include_pad: Whentrue(the default), padding (zero) elements are included in the averaging denominator, so each output element divides by the full window sizeprod(k). Whenfalse, only the in-bounds (non-padding) elements are counted, matching cuDNN'sCUDNN_POOLING_AVERAGE_COUNT_EXCLUDE_PADDINGand PyTorch'scount_include_pad=false. Has no effect whenpad == 0.ceil_mode: Whentrue, round the output size up instead of down, as PyTorch'sceil_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 withcount_include_pad=true, as in PyTorch. SeePoolDims.
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 5NNlib.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:
[...]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 1NNlib.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 9NNlib.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 5NNlib.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.
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 (Intor tuple of oneIntper spatial dimension).pad: zero padding. AnIntor tuple applies symmetric padding; a tuple of2*ndimsentries gives(left, right)padding per spatial dimension.dilation: spacing between filter elements (atrous convolution).flipped: iffalse(default), perform true mathematical convolution; iftrue, 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)NNlib.ConvDims — Type
ConvDimsType 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.
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.
NNlib.DepthwiseConvDims — Type
DepthwiseConvDimsConcrete 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.
NNlib.DenseConvDims — Type
DenseConvDimsConcrete subclass of ConvDims for a normal, dense, conv2d/conv3d.
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
6NNlib.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
700.0In general, an inverse to unfold does not exist if divisor contains zeros.
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 1.00571NNlib.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.
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)
trueNNlib.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 (whentrack_stats=true) with an exponential moving average controlled bymomentum, while statistics of the current batch are used to normalise; - with
training=falsethey 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.
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.
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.
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.
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)
trueUpsampling
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,))
trueNNlib.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).
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 6.0NNlib.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 allowedNNlib.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 3.6Rotation
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=:bilinearfor bilinear interpolation ormethod=:nearestfor nearest neighbourrotation_center=size(arr) .÷ 2 .+ 1means 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 0.0Batched Operations
Flux's Flux.Bilinear layer uses NNlib.batched_mul internally.
NNlib.batched_mul — Function
batched_mul(A, B) -> C
A ⊠ B # \boxtimesBatched 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))
trueThe 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.
batched_mul(A::Array{T,3}, B::Matrix)
batched_mul(A::Matrix, B::Array{T,3})
A ⊠ BThis is always matrix-matrix multiplication, but either A or B may lack a batch index.
When
Bis a matrix, result hasC[:,:,k] == A[:,:,k] * B[:,:]for allk.When
Ais a matrix, thenC[:,:,k] == A[:,:] * B[:,:,k]. This can also be done by reshaping and calling*, for instanceA ⊡ Busing TensorCore.jl, but is implemented here usingbatched_gemminstead ofgemm.
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].
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.
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.
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.
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)Gather and Scatter
Flux's Embedding layer uses NNlib.gather as its backend.
NNlib.gather — Function
NNlib.gather(src, idx) -> dstReverse 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 4gather(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
11NNlib.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.
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
11NNlib.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
initis provided, it is used to initialize the content ofdst. Otherwise, the init values is inferred from the reduction operatoropfor some common operators (e.g.init = 0forop = +).If
dstsizeis provided, it will be used to define the size of destination array, otherwise it will be inferred bysrcandidx.
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
10NNlib.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...])Arguments
op: Operations to be applied ondstandsrc, e.g.+,-,*,/,max,minandmean.dst: The destination forsrcto aggregate to. This argument will be mutated.src: The source data for aggregating.idx: The mapping for aggregation from source (index) to destination (value). Theidxarray 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 0.5Sampling
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
```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 <: RealHann 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: Iftrue(default), returns a window to be used as periodic function. Iffalse, 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)
trueReturns:
Vector of length window_length and eltype T.
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 <: RealHamming 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: Iftrue(default), returns a window to be used as periodic function. Iffalse, 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]
trueα::Real: Coefficient α in the equation above.β::Real: Coefficient β in the equation above.
Returns:
Vector of length window_length and eltype T.
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 vector0 < length(window) ≤ n_fft. If window is shorter thann_fft, it is padded with zeros on both sides. Ifnothing(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 withpad_reflectfunction.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.
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. WhereBis 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 ofstft. Ifnothing(default), then no window was applied.center::Bool: Whether input tostftwas padded on both sides so that $t$-th frame is centered at time $t \times \text{hop length}$. Padding is done withpad_reflectfunction.normalized::Bool: Whether input tostftwas 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 tostft. Helps restoring the exactstftinput size. Otherwise, the array might be a bit shorter.
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.,1for magnitude,2for power, etc. If0, 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.
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⠀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.
NNlib.glu — Function
glu(x, dim = 1)The gated linear unit from the "Language Modeling with Gated Convolutional Networks" paper.
Calculates a .* sigmoid(b), where x is split in half along given dimension dim to form a and b.
NNlib.within_gradient — Function
within_gradient(x) --> BoolReturns 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)
3.0What 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.
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.