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Add Apollo optimizer (https://arxiv.org/pdf/2412.05270) #196

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4 changes: 3 additions & 1 deletion src/Optimisers.jl
Original file line number Diff line number Diff line change
Expand Up @@ -5,6 +5,8 @@ using Functors: functor, fmap, fmap_with_path,
isleaf, @functor, fmapstructure, children, AbstractWalk
using LinearAlgebra

using Random: randn!

include("interface.jl")
export AbstractRule

Expand All @@ -23,7 +25,7 @@ include("rules.jl")
export Descent, Adam, Momentum, Nesterov, Rprop, RMSProp,
AdaGrad, AdaMax, AdaDelta, AMSGrad, NAdam, AdamW, RAdam, OAdam, AdaBelief,
WeightDecay, SignDecay, ClipGrad, ClipNorm, OptimiserChain, Lion,
AccumGrad
AccumGrad, Apollo, GradNormGrowthLimiter

VERSION >= v"1.11.0-DEV.469" && eval(Meta.parse("public apply!, init, setup, update, update!"))

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130 changes: 130 additions & 0 deletions src/rules.jl
Original file line number Diff line number Diff line change
Expand Up @@ -599,6 +599,136 @@ function apply!(o::AdaBelief, state, x::AbstractArray{T}, dx) where T
return (mt, st, βt .* β), dx′
end


"""
GradNormGrowthLimiter(γ = 1.1; m = 1e-3, ϵ = 1e-8, throw = true, paramscale_min = true)
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should the default value for m correspond to the original paper (i.e. m=0 i suppose)?

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m=0 makes sense when this is applied to the entire model, but could be fatal when applied tensor-wise. I think it is better to have non-footgun defaults, and make it clearer that this isn't a faithful reproduction?

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I've kept a non-zero default, but I've tweaked the docs to clarify that this method isn't quite the same as in those papers. (I also switched the "scaling m by the number of parameters" to using sqrt).


Gradient norm growth limiter from Chen et al. (https://arxiv.org/pdf/2410.01623) and used with Apollo in Zhu et al. (https://arxiv.org/pdf/2412.05270).
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Suggested change
Gradient norm growth limiter from Chen et al. (https://arxiv.org/pdf/2410.01623) and used with Apollo in Zhu et al. (https://arxiv.org/pdf/2412.05270).
Gradient norm growth limiter from [Chen et al.](https://arxiv.org/abs/2410.01623) and used with Apollo in [Zhu et al.](https://arxiv.org/abs/2412.05270).

With Optimisers.jl this will apply per-tensor, which may not be the same as the implementations in these papers. It still seems to help, but the ideal settings may vary.
This also introduces `m` a hard minimum on the gradient norm, and never rescales grads below this, preventing a tensor from getting "trapped" near zero.
This can be a fixed min, or scaled by the number of parameters in the tensor (with `paramscale_min = true`).
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explain the role of gamma?

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Done in the new version.

"""
struct GradNormGrowthLimiter <: AbstractRule
γ::Float64
m::Float64 #Min grad norm, to stop a tensor getting stuck near zero
ϵ::Float64
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We don't allow unicode field names, suggest:

Suggested change
γ::Float64
m::Float64 #Min grad norm, to stop a tensor getting stuck near zero
ϵ::Float64
gamma::Float64
mu::Float64 # Min grad norm, to stop a tensor getting stuck near zero
epsilon::Float64

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Done, but changed the variable names to avoid eg. gamma.

throw::Bool
paramscale_min::Bool
end

GradNormGrowthLimiter(γ = 1.1; m = 1e-3, ϵ = 1e-8, throw = true, paramscale_min = true) = GradNormGrowthLimiter(γ, m, ϵ, throw, paramscale_min)
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We don't have greek-letter keyword options, nor field names -- the API should never ask the user to type these. They are used only in documentation / as local variables. Probably the first 3 should be positional.

Bikeshedding names bit, to avoid overly long things, the constructor could be:

Suggested change
GradNormGrowthLimiter= 1.1; m = 1e-3, ϵ = 1e-8, throw = true, paramscale_min = true) = GradNormGrowthLimiter(γ, m, ϵ, throw, paramscale_min)
NormGrowLimit= 1.1, m = 1e-3, ε = 1e-8; throw = true, scale = true) = NormGrowLimit(γ, m, ε, throw, scale)

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I went with NormGrowthCap here.


init(o::GradNormGrowthLimiter, x::AbstractArray{T}) where T = T(0)

function apply!(o::GradNormGrowthLimiter, state, x::AbstractArray{T}, dx) where T
current_norm = _norm(dx, 2)
if o.throw && !isfinite(current_norm)
throw(DomainError("gradient has L2-norm $current_norm, for array $(summary(x))"))
end
if state == 0
return (current_norm), dx
else
#If you're below the hard min, then don't scale
if o.paramscale_min
minthresh = o.m * length(dx)
else
minthresh = o.m
end
if current_norm < minthresh
return current_norm, dx
end
ratio = current_norm / (state + o.ϵ)
if ratio > o.γ
λ = T((o.γ * state) / (current_norm + o.ϵ))
return current_norm * λ, dx * λ
else
return current_norm, dx
end
end
end

nonfirstdims(x) = prod(size(x)[2:end])

"""
Apollo(η::Real, rank::Int; u = 100, sort_dims = false)
Apollo(η::Real; rank_function::Function = dim -> ceil(Int, sqrt(dim)), u = 100, sort_dims = false)
Apollo(opt::AdamW, rank::Int; u = 100, sort_dims = false)
Apollo(opt::AdamW; rank_function::Function = dim -> ceil(Int, sqrt(dim)), u = 100, sort_dims = false)

Apollo optimizer from Zhu et al. (https://arxiv.org/pdf/2412.05270). Tracks moments in a low-rank subspace, aiming for Adam-like behavior with minimal additional memory usage.
First argument can be an AdamW optimizer, or a learning rate (which will use the default AdamW optimizer with that learning rate). Second argument can be a rank, or a function
to compute the rank from the second dimension (or the product of all dims > 1) of the weight matrix (or tensor).
"""
struct Apollo{T1} <: AbstractRule
opt::T1
r::Function #Maps non-first dims to rank
u::Int #Subspace update frequency (T in paper)
sort_dims::Bool #Whether to swap the dims of x and dx when the second dim is smaller than the first
end


Apollo() = Apollo(AdamW(0.001), dim -> ceil(Int, sqrt(dim)), 100, true)
Apollo(η::Real, rank::Int; u = 100, sort_dims = true) = Apollo(AdamW(η), dim -> max(dim, rank), u, sort_dims)
Apollo(η::Real; rank_function::Function = dim -> ceil(Int, sqrt(dim)), u = 100, sort_dims = true) = Apollo(AdamW(η), rank_function, u, sort_dims)
Apollo(opt::AdamW, rank::Int; u = 100, sort_dims = true) = Apollo(AdamW(η), dim -> max(dim, rank), u, sort_dims)
Apollo(opt::AdamW; rank_function::Function = dim -> ceil(Int, sqrt(dim)), u = 100, sort_dims = true) = Apollo(opt, rank_function, u, sort_dims)

#Use the base init and apply for 1D arrays
init(o::Apollo, x::AbstractArray{T,1}) where T = init(o.opt, x)
apply!(o::Apollo, state, x::AbstractArray{T,1}, dx) where T = apply!(o.opt, state, x, dx)

function init(o::Apollo, x::AbstractArray{T}) where T
first_dim, second_dim = size(x,1), nonfirstdims(x)
if o.sort_dims && second_dim < first_dim
first_dim, second_dim = second_dim, first_dim
end
rank = o.r(second_dim)
P = similar(x, rank, first_dim)
randn!(P)
P .*= T(sqrt(1/rank))
((similar(x, rank, second_dim) .= 0, similar(x, rank, second_dim) .= 0, o.opt.beta), 1, P)
end


function apply!(o::Apollo, state, x::AbstractArray{T}, dx) where T
swapped = false
original_size = size(x)
x = reshape(x, size(x,1), nonfirstdims(x))

dx = Broadcast.materialize(dx) #This is to stop the "gradient type" @lazy test from failing due to reshape.
dx = reshape(dx, size(x,1), nonfirstdims(x))
Comment on lines +707 to +708
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Do you need to materialize in matrix case?

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For everything except the whatever comes in during the "gradient type" test you don't need materialize. I wasn't 100% sure exactly what is coming in during those tests, so wasn't sure how to separate them from regular matrix/tensors. What do you suggest here?


first_dim, second_dim = size(x,1), size(x,2)
if o.sort_dims && second_dim < first_dim
first_dim, second_dim = second_dim, first_dim
x = x'
dx = dx'
swapped = true
end
(mt, vt, βt), t, P = state
η = T(o.opt.eta)
λ = T(o.opt.lambda)
β = T.(o.opt.beta)
ϵ = T(o.opt.epsilon)
βt = T.(βt)
if mod(t, o.u) == 0
rank = o.r(second_dim)
randn!(P)
P .*= T(sqrt(1/rank))
end
R = P * dx
@.. mt = β[1] * mt + (1 - β[1]) * R
@.. vt = β[2] * vt + (1 - β[2]) * abs2(R)
Rhat = @. mt / (1 - βt[1]) / (sqrt(vt / (1 - βt[2])) + ϵ)
s = sqrt.(sum(abs2.(Rhat), dims=1))[:] ./ (sqrt.(sum(abs2.(R), dims=1))[:] .+ ϵ)
dx′′ = η * (dx .* reshape(s, 1, :)) + λ * x
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These lines allocate a lot.

Rhat isn't used?

For the rest maybe it can be something like

sum1R2 = sum(abs2, R; dims=1)  # it's already the right shape, no need for [:] & reshape(s, 1, :)?
s = @. sqrt(sum1R2) / sqrt(Rhat + ϵ)
dx′′ = @lazy η * (dx * s) + λ * x  # one fused broadcast

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I got something like this working, but the @lazy breaks things, so omitted for now.

if swapped
dx′′ = dx′′'
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Suggested change
dx′′ = dx′′'
dx′′ = transpose(dx′′)

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Also, this sort of branching introduces type instability. IDK if we care but perhaps worth some thought. Maybe there's a nicer way to just store everything transposed?

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Maybe an optimization we can figure out later if it becomes an issue?

end
return ((mt, vt, βt .* β), t+1, P), reshape(dx′′, original_size)
end


"""
WeightDecay(λ = 5e-4)
WeightDecay(; [lambda])
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3 changes: 2 additions & 1 deletion test/rules.jl
Original file line number Diff line number Diff line change
Expand Up @@ -8,12 +8,13 @@ RULES = [
# All the rules at default settings:
Descent(), Adam(), Momentum(), Nesterov(), Rprop(), RMSProp(),
AdaGrad(), AdaMax(), AdaDelta(), AMSGrad(), NAdam(),
AdamW(), RAdam(), OAdam(), AdaBelief(), Lion(),
AdamW(), RAdam(), OAdam(), AdaBelief(), Lion(), Apollo(),
# A few chained combinations:
OptimiserChain(SignDecay(0.001), Adam(0.001)),
OptimiserChain(ClipNorm(), Adam(0.001)),
OptimiserChain(ClipGrad(0.5), Momentum()),
OptimiserChain(WeightDecay(), OAdam(), ClipGrad(1)),
OptimiserChain(GradNormGrowthLimiter(1.1), Apollo()),
# Not the default:
RMSProp(centred = true), AdamW(couple=false),
]
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