Optimize For Gpu
K-DenseCommunityCreated by K-Dense, Inc.
- Skill
- Tool integration
- Science and research
- MIT
- No issues found
AutoGineer summary
Written by AutoGineer from the skill’s own files, not by the author
This skill provides a systematic approach to GPU-accelerating CPU-bound scientific Python code. It emphasizes an evidence-driven workflow: profiling existing bottlenecks, selecting the appropriate library (e.g., CuPy, cuDF, cuML, cuGraph, cuCIM, or Warp), and validating performance gains through synchronized benchmarks. It guides users to maintain numerical contracts, minimize host-device data transfers, and choose the least disruptive implementation path—from backend acceleration modes to custom Numba-CUDA kernels.
What it does
- Identifies CPU-bound bottlenecks in NumPy, pandas, and scikit-learn workflows.
- Maps scientific tasks to GPU-accelerated libraries like CuPy, cuDF, and cuML.
- Provides patterns for migrating CPU code to GPU-resident execution.
- Guides the implementation of custom CUDA kernels for specialized simulation or processing.
- Ensures correctness through comparative testing and numerical tolerance validation.
- Facilitates accurate benchmarking using CUDA events and profilers.
When to use it
- When processing large datasets that exceed CPU performance limits.
- When working with compute-intensive tasks like image processing, graph analytics, or simulations.
- When the workload involves data-parallel operations suitable for NVIDIA GPU architecture.
- When you need to optimize existing Python code without rewriting the entire application.
- When you require high-performance file I/O directly into GPU memory.
Advantages
- Significant speedups for data-parallel scientific computations.
- Maintains familiar Python API patterns through library-specific drop-in replacements.
- Reduces overhead by keeping data resident on the GPU.
- Provides a clear decision framework for choosing between high-level libraries and custom kernels.
- Promotes rigorous validation to ensure GPU results match CPU expectations.
Usage examples
- “How can I speed up my pandas groupby operation on a large dataset using my NVIDIA GPU?”
- The agent will guide you to use cuDF, either by replacing the import or using the cudf.pandas accelerator mode, and explain how to benchmark the end-to-end performance.
- “I have a slow Python loop performing particle integration. Can I run this on a GPU?”
- The agent will recommend using NVIDIA Warp to JIT-compile the loop into a GPU kernel, providing a pattern for the integration function and explaining how to manage device memory.
- “My scikit-learn random forest training is too slow. What are my options?”
- The agent will suggest using cuML's RandomForestClassifier, explain the parameter matching process, and advise on how to validate the model's accuracy against the CPU version.
- “How do I profile my GPU code to ensure I am actually getting a speedup?”
- The agent will provide instructions on using CUDA events for synchronization, the cupyx.profiler for micro-benchmarking, and Nsight Systems for end-to-end timeline analysis.
Install
Download the skill as a ZIP:
https://autogineer.com/agent-skills/k-dense-ai/optimize-for-gpu/downloadUnzip it into the cross-client skills folder of your project:
mkdir -p .agents/skills && unzip optimize-for-gpu.zip -d .agents/skills
Documentation by K-Dense, Inc.
GPU Optimization for Python with NVIDIA
Treat GPU acceleration as an evidence-driven optimization, not an automatic rewrite. Preserve the user's numerical and algorithmic contract, measure with representative data, and keep the GPU version only when synchronized end-to-end benchmarks show a useful improvement.
Reviewed against RAPIDS 26.08, CuPy 14.2, Numba-CUDA 0.30.4, and Warp 1.17.
The references contain illustrative GPU examples: source/API review is not execution on CUDA
hardware. Validate them on the user's target GPU before reporting correctness or speedup.
Do not use a moving latest documentation page to infer compatibility with a pinned release.
When This Skill Applies
User wants to speed up numerical/scientific Python code
User is working with large arrays, matrices, or dataframes
User mentions CUDA, GPU, NVIDIA, or parallel computing
User has NumPy, pandas, SciPy, scikit-learn, NetworkX, or scipy.sparse.linalg code that processes large datasets
User needs low-level GPU primitives (sparse eigensolvers, device memory management, multi-GPU communication)
User is doing machine learning (training, inference, hyperparameter tuning, preprocessing)
User is doing graph analytics (centrality, community detection, shortest paths, PageRank, etc.)
User is doing vector search, nearest neighbor search, similarity search, or building a RAG pipeline
User has Faiss, Annoy, ScaNN, or sklearn NearestNeighbors code that could be GPU-accelerated
User wants GPU-accelerated interactive dashboards, cross-filtering, or exploratory data analysis on large datasets
User is doing geospatial analysis (point-in-polygon, spatial joins, trajectory analysis, distance calculations) with GeoPandas or shapely
User is doing image processing, computer vision, or medical imaging (filtering, segmentation, morphology, feature detection) with scikit-image or OpenCV
User is working with whole-slide images (WSI), digital pathology, microscopy, or remote sensing imagery
User is loading large binary data files into GPU memory (numpy.fromfile → cupy, or Python open() → GPU array)
User needs to read files from S3, HTTP, or WebHDFS directly into GPU memory
User mentions GPUDirect Storage (GDS) or wants to bypass CPU-memory staging for file IO
User is doing physics simulation (particles, cloth, fluids, rigid bodies) or differentiable simulation
User needs mesh operations (ray casting, closest-point queries, signed distance fields) or geometry processing on GPU
User is doing robotics (kinematics, dynamics, control) with transforms and quaternions
User has Python simulation loops that could be JIT-compiled to GPU kernels
User mentions NVIDIA Warp or wants differentiable GPU simulation integrated with PyTorch/JAX
User is doing simulations, signal processing, financial modeling, bioinformatics, physics, or any compute-intensive work
User wants to optimize existing code and GPU acceleration is the right answer
Choose the Smallest Suitable Layer
Prefer a maintained library implementation over a custom kernel:
| Existing workload | Preferred path | Use for |
|---|---|---|
| NumPy / SciPy | CuPy | arrays, sparse matrices, linear algebra, FFTs, signal processing |
| pandas | cudf.pandas, then cuDF | accelerator mode first; native API for more control |
| scikit-learn | cuml.accel, then cuML | accelerator mode first; native estimators as needed |
| NetworkX | nx-cugraph, then cuGraph | backend dispatch first; native graph API at scale |
| scikit-image | cuCIM | GPU image processing and whole-slide imaging |
| Faiss / Annoy / k-NN | cuVS | exact and approximate vector search |
| Raw or remote file I/O | KvikIO | GPU buffers and GPUDirect Storage |
| Custom array kernels | Numba-CUDA-MLIR for new work; Numba-CUDA for existing code | explicit SIMT kernels and shared memory |
| Spatial or differentiable kernels | Warp | geometry, simulation kernels, robotics, autodiff |
| High-level physics simulation | Newton | maintained engine that succeeds the removed warp.sim module |
| Low-level RAPIDS primitives | RAFT (pylibraft) | sparse eigensolvers, resources, multi-GPU building blocks |
Do not move code out of PyTorch, JAX, TensorFlow, or another GPU-native framework merely to use one of these libraries. First remove CPU round trips and use the framework's compiler, profiler, mixed-precision, and batching facilities.
Treat these as legacy-only:
| Project | Status | Guidance |
|---|---|---|
| cuxfilter | Final release 26.06 | Maintain existing dashboards only. For new work, combine cuDF with HoloViews/hvPlot/Datashader and serve with Panel, Dash, Streamlit, or Bokeh. |
| cuSpatial | Archived at 25.04 | Use only in an isolated legacy environment. For new work, keep geometry in GeoPandas/Shapely and accelerate compatible tabular stages with cuDF. |
Full per-library guidance, including when each is the wrong choice and how to combine them, is in references/decision_framework.md. Install commands and CUDA version selection are in references/installation.md. Before/after conversions for every library are in references/code_transformation_patterns.md.
Optimization Workflow
1. Define the contract and baseline
Capture a representative input, expected output, and acceptable numerical tolerance.
Measure the current end-to-end path, including input, transfers, compute, and output.
Profile before changing code. Use CPU profilers for CPU code and identify whether the real limit is compute, memory bandwidth, allocation, transfer, synchronization, or storage.
Record hardware, package versions, dtypes, shapes, batch size, and warm-up policy with results.
2. Check suitability before porting
GPU execution is promising when the hot path exposes substantial independent work, runs often enough to amortize initialization and transfer, and has a working set that fits available device memory with room for temporaries. Keep a CPU path when the workload is small, mostly sequential, dominated by unsupported operations, or requires frequent host-device round trips.
Do not use fixed row-count thresholds as proof. Benchmark the user's actual shapes and hardware. For out-of-core data, estimate peak working memory and choose chunking, Dask, or a streaming design before allocating.
3. Try the least disruptive implementation
If the code already uses a GPU-native framework, optimize within that framework.
Try accelerator or backend modes (
cudf.pandas,cuml.accel,nx-cugraph).Move to a native GPU API only where accelerator coverage or performance is insufficient.
Write a custom kernel only when profiling shows an operation without a suitable library implementation.
Read the relevant library reference before writing code; compatible names can still differ in defaults, dtypes, output types, and supported arguments.
4. Keep a coherent GPU data path
Transfer inputs once and keep intermediates device-resident.
Reuse allocations and prefer
out=or in-place forms when semantics allow.Batch small operations; fuse elementwise work when it removes intermediate arrays.
Use pinned host memory and non-default streams only after profiling shows transfer overlap matters.
Choose
float32, mixed precision, or reduced-precision storage only when the contract permits it.
5. Validate semantics before speed
Compare CPU and GPU outputs on small deterministic fixtures and representative data.
Use explicit tolerances for floating-point results and test edge cases, NaNs, ordering, and dtypes.
For approximate nearest-neighbor indexes, report recall@k against exact search; do not compare an exact CPU algorithm with an approximate GPU algorithm as if they were equivalent.
Check accelerator warnings and logs for CPU fallback.
6. Benchmark GPU code correctly
GPU work is asynchronous, so a CPU timer around an unsynchronized call measures enqueue time. Warm up context creation and JIT compilation, then use CUDA events or a library-aware timer:
from cupyx.profiler import benchmark
print(benchmark(gpu_function, (arg1, arg2), n_warmup=10, n_repeat=100))Use %gpu_timeit in notebooks, Nsight Systems (nsys) for end-to-end timelines, and Nsight
Compute (ncu) for kernel analysis. Report both synchronized kernel/region time and realistic
end-to-end latency; include transfer and conversion costs when production pays them.
Measure peak device memory as well as time. For CuPy, distinguish live allocations
from memory retained by its pool; a high nvidia-smi reading after arrays are
released is not by itself a leak. Record the allocator and pooling policy, include
temporary buffers and FFT caches, and leave headroom for CUDA context/library
allocations outside the pool limit. Avoid clearing the pool inside timed repeats
unless production does so. See CuPy memory management.
7. Keep, revise, or reject the port
Retain the GPU path only when it passes correctness checks and improves the metric the user cares about on representative data. If it does not, explain whether the limiting factor is problem size, transfers, unsupported fallback, memory pressure, launch granularity, or the algorithm itself.
Important Notes
Provide a CPU fallback when the application requires portability; otherwise fail early with a clear hardware and dependency error.
Test against a trusted reference with problem-specific tolerances; changed algorithms, precision, reduction order, and random streams can produce more than roundoff differences.
GPU memory is limited — for datasets larger than GPU memory, consider chunking or using RAPIDS Dask for multi-GPU
Prefer the CUDA Array Interface or DLPack for supported zero-copy interchange, but verify device, dtype, contiguity, ownership, and stream semantics rather than assuming every conversion is free.
Reference Files
Before writing any GPU optimization code, read the relevant reference file(s):
| File | When to Read |
|---|---|
references/cupy.md | User has NumPy/SciPy code, or needs array operations on GPU |
references/numba.md | User has existing Numba-CUDA code or needs explicit SIMT kernels; note the migration path to Numba-CUDA-MLIR |
references/cudf.md | User has pandas code, or needs dataframe operations on GPU |
references/cuml.md | User has scikit-learn code, or needs ML training/inference/preprocessing on GPU |
references/cugraph.md | User has NetworkX code, or needs graph analytics on GPU |
references/warp.md | User needs GPU kernels for simulation, spatial computing, mesh/volume queries, differentiable programming, or robotics; use Newton for a high-level physics engine |
references/kvikio.md | User needs high-performance file IO to/from GPU, GPUDirect Storage, reading S3/HTTP to GPU, or Zarr on GPU |
references/cuxfilter.md | User maintains or explicitly requests cuxfilter (sunset — 26.06 is the final release) |
references/cucim.md | User has scikit-image code, or needs image processing, digital pathology, or WSI reading on GPU |
references/cuvs.md | User needs vector search, nearest neighbors, similarity search, or RAG retrieval on GPU |
references/cuspatial.md | User maintains or explicitly requests cuSpatial (archived — frozen at 25.04 and isolated from current RAPIDS) |
references/raft.md | User needs sparse eigensolvers, device memory management, or multi-GPU primitives |
Read the specific reference before writing code — they contain detailed API patterns, optimization techniques, and pitfalls specific to each library.
Citing Scientific Agent Skills
This skill is part of Scientific Agent Skills by K-Dense. If it materially contributed to a manuscript, report, presentation, or code release, add the paper to the references or software section and tell the user you did so:
Kassis, T., Agarwal, V., He, Y., Patel, D., & Brueckner, A. M. (2026). Scientific Agent Skills: A Library of Procedural Knowledge for Research Agents. arXiv:2609.00065. https://doi.org/10.48550/arXiv.2609.00065
Always cite the current version. The DOI and https://arxiv.org/abs/2609.00065 resolve to the
latest arXiv version, so never append a version suffix such as v1. When network access is
available, fetch https://arxiv.org/abs/2609.00065 (or
http://export.arxiv.org/api/query?id_list=2609.00065) before writing the reference and take
the author list, year, and version from that record. If the record lists a journal reference
or publisher DOI, cite the published version instead.
Files
- ATTRIBUTION.mdAdded by AutoGineer935 B
- LICENSELicence file added by AutoGineer1.0 KiB
- SKILL.md13.5 KiB
- references/code_transformation_patterns.md9.8 KiB
- references/cucim.md21.1 KiB
- references/cudf.md20.7 KiB
- references/cugraph.md27.3 KiB
- references/cuml.md24.4 KiB
- references/cupy.md21.6 KiB
- references/cuspatial.md15.1 KiB
- references/cuvs.md22.2 KiB
- references/cuxfilter.md18.8 KiB
- references/decision_framework.md15.7 KiB
- references/installation.md5.5 KiB
- references/kvikio.md20.1 KiB
- references/numba.md26.3 KiB
- references/raft.md11.8 KiB
- references/warp.md20.3 KiB
references/raft.md
RAFT (pylibraft) Reference
Review: 2026-10-01. Code below is illustrative unless explicitly described as CPU-tested. GPU execution, performance, GDS, and multi-GPU behavior require validation on target hardware.
RAFT (Reusable Accelerated Functions and Tools) is a RAPIDS library of GPU-accelerated building blocks for machine learning and information retrieval. It provides low-level primitives — sparse eigensolvers, device memory management, random graph generation, and multi-GPU communication — that higher-level libraries like cuML and cuGraph are built on. Use pylibraft directly when you need these primitives without the overhead of a full ML framework.
Full documentation: https://docs.nvidia.com/raft/26.08/ Note: Vector search and clustering algorithms have been migrated to cuVS. Use cuVS for nearest neighbor search, not RAFT.
Table of Contents
Installation and Setup
Core Concepts
Device Memory Management
Sparse Eigenvalue Problems
Random Graph Generation
Multi-Node Multi-GPU with raft-dask
Interoperability
Performance Tips
Common Pitfalls
Installation and Setup
Use uv add in standalone examples; follow the user's existing project package manager when one
is already configured.
# pylibraft (core library)
uv add --extra-index-url=https://pypi.nvidia.com "pylibraft-cu12==26.8.*" # For CUDA 12.x
uv add --extra-index-url=https://pypi.nvidia.com "pylibraft-cu13==26.8.*" # For CUDA 13.x
# raft-dask (multi-node multi-GPU support, optional)
uv add --extra-index-url=https://pypi.nvidia.com "raft-dask-cu12==26.8.*" # For CUDA 12.x
uv add --extra-index-url=https://pypi.nvidia.com "raft-dask-cu13==26.8.*" # For CUDA 13.xpylibraft and raft-dask wheels (including the companion libraft wheel) are also published directly to PyPI, so the extra index is optional.
Verify:
import pylibraft
from pylibraft.common import DeviceResources
handle = DeviceResources()
handle.sync()
print("pylibraft is working")Core Concepts
DeviceResources (CUDA Resource Handle)
DeviceResources manages expensive CUDA resources (streams, stream pools, library handles for cuBLAS/cuSOLVER). Create one and reuse it across multiple RAFT calls to avoid repeated allocation overhead.
from pylibraft.common import DeviceResources, Stream
# Default stream
handle = DeviceResources()
# Custom stream
stream = Stream()
handle = DeviceResources(stream)
# With a CuPy stream
import cupy
cupy_stream = cupy.cuda.Stream()
handle = DeviceResources(stream=cupy_stream.ptr)
# Always sync before reading results
handle.sync()RAFT functions are asynchronous by default — they return immediately and work continues on the GPU. You must call handle.sync() before accessing output data on the CPU. If you don't pass a handle, RAFT allocates temporary resources internally and synchronizes before returning (convenient but slower for repeated calls).
Stream
A thin wrapper around cudaStream_t for ordering GPU operations:
from pylibraft.common import Stream
stream = Stream()
stream.sync() # Synchronize all work on this stream
ptr = stream.get_ptr() # Get the raw cudaStream_t pointer (uintptr_t)Device Memory Management
device_ndarray
device_ndarray is RAFT's lightweight GPU array type. It implements __cuda_array_interface__, making it interoperable with CuPy, Numba, PyTorch, and other GPU libraries.
from pylibraft.common import device_ndarray
import numpy as np
# Allocate empty GPU array
gpu_arr = device_ndarray.empty((1000, 50), dtype=np.float32)
# From a NumPy array (copies data to GPU)
cpu_data = np.random.rand(1000, 50).astype(np.float32)
gpu_arr = device_ndarray(cpu_data)
# Back to NumPy (copies data to CPU)
result = gpu_arr.copy_to_host()
# Properties
print(gpu_arr.shape) # (1000, 50)
print(gpu_arr.dtype) # float32
print(gpu_arr.c_contiguous) # True (row-major)
print(gpu_arr.f_contiguous) # FalseConfiguring Output Types
You can configure all RAFT compute APIs to return CuPy arrays or PyTorch tensors instead of device_ndarray:
import pylibraft.config
pylibraft.config.set_output_as("cupy") # All APIs return cupy arrays
pylibraft.config.set_output_as("torch") # All APIs return torch tensors
# Custom conversion
pylibraft.config.set_output_as(lambda arr: arr.copy_to_host()) # Return numpySparse Eigenvalue Problems
eigsh — Sparse Symmetric Eigenvalue Decomposition
GPU-accelerated Lanczos method for finding eigenvalues/eigenvectors of large sparse symmetric matrices. A narrower interface than SciPy: the 26.08 implementation accepts real float32/float64 CSR values and int32/int64 indices. It does not implement SciPy generalized/shift-invert parameters such as M or sigma.
import cupy as cp
import cupyx.scipy.sparse as sp
from pylibraft.sparse.linalg import eigsh
from pylibraft.common import DeviceResources
# Create a sparse symmetric matrix (CSR format)
n = 10000
density = 0.01
A = sp.random(n, n, density=density, dtype=cp.float32, format='csr')
A = A + A.T # Make symmetric
# Find 6 largest eigenvalues
handle = DeviceResources()
eigenvalues, eigenvectors = eigsh(A, k=6, which='LM', handle=handle)
handle.sync()
print(f"Eigenvalues shape: {eigenvalues.shape}") # (6,)
print(f"Eigenvectors shape: {eigenvectors.shape}") # (10000, 6)Parameters:
A— Sparse symmetric CSR matrix (cupyx.scipy.sparse.csr_matrix)k— Number of eigenvalues to compute (default: 6). Must be1 <= k < nwhich— Which eigenvalues:'LM': largest in magnitude (default)'LA': largest algebraic'SA': smallest algebraic'SM': smallest in magnitude
v0— Starting vector (optional, random if None)ncv— Number of Lanczos vectors. Must bek + 1 < ncv < nmaxiter— Maximum iterationstol— Convergence tolerance (0 = machine precision)seed— Random seed for reproducibilityhandle— OptionalDeviceResourceshandle
When to use: Spectral methods (spectral clustering, graph partitioning, PageRank-like computations), dimensionality reduction on sparse data, physics simulations with large sparse Hamiltonians, structural analysis (vibration modes).
Random Graph Generation
rmat — R-MAT Graph Generation
Generates random graphs using the Recursive Matrix (R-MAT) model, commonly used for benchmarking graph algorithms with realistic structure (power-law degree distribution, community structure).
import cupy as cp
from pylibraft.random import rmat
from pylibraft.common import DeviceResources
n_edges = 100000
r_scale = 16 # log2 of source node count (2^16 = 65536 nodes)
c_scale = 16 # log2 of destination node count
theta_len = max(r_scale, c_scale) * 4
# Output: edge list as (src, dst) pairs
out = cp.empty((n_edges, 2), dtype=cp.int32)
# Probability distribution at each R-MAT level
theta = cp.tile(cp.asarray([0.57, 0.19, 0.19, 0.05], dtype=cp.float32),
max(r_scale, c_scale)) # Each four-probability level sums to one
handle = DeviceResources()
rmat(out, theta, r_scale, c_scale, seed=42, handle=handle)
handle.sync()
print(f"Generated {n_edges} edges")
print(f"Edge list shape: {out.shape}") # (100000, 2)
print(f"Sample edges:\n{out[:5].get()}") # First 5 edges on CPUWhen to use: Benchmarking graph algorithms, generating synthetic social/web graphs, testing graph processing pipelines at scale.
Multi-Node Multi-GPU with raft-dask
raft-dask provides a Comms class for managing NCCL and UCX communication across workers in a Dask cluster. This is the foundation for distributed GPU computing in RAPIDS.
from dask_cuda import LocalCUDACluster
from dask.distributed import Client
from raft_dask.common import Comms, local_handle
# Set up a local multi-GPU Dask cluster
cluster = LocalCUDACluster()
client = Client(cluster)
def run_on_gpu(sessionId):
handle = local_handle(sessionId)
# Use handle with RAFT or cuML algorithms
return "done"
# Initialize multi-GPU communication
comms = Comms(client=client)
comms.init()
# Submit work to each GPU worker
futures = [
client.submit(run_on_gpu, comms.sessionId, workers=[w], pure=False)
for w in comms.worker_addresses
]
# Wait for results
from dask.distributed import wait
wait(futures, timeout=60)
results = client.gather(futures) # Propagate worker failures, not just completion
# Clean up
comms.destroy()
client.close()
cluster.close()Comms parameters:
comms_p2p(bool) — Enable UCX peer-to-peer communication (default: False). Enable for algorithms that need direct GPU-to-GPU transfers.client— Dask distributed clientverbose(bool) — Enable verbose loggingstreams_per_handle(int) — Number of CUDA streams per handle
Interoperability
RAFT's device_ndarray implements __cuda_array_interface__, enabling zero-copy sharing with other GPU libraries:
import cupy as cp
import torch
import numpy as np
from pylibraft.common import device_ndarray
# pylibraft -> CuPy (zero-copy)
raft_arr = device_ndarray(np.random.rand(100).astype(np.float32))
cupy_arr = cp.asarray(raft_arr)
# pylibraft -> PyTorch (zero-copy)
torch_tensor = torch.as_tensor(raft_arr, device='cuda')
# CuPy -> pylibraft (pass directly — RAFT APIs accept __cuda_array_interface__)
cupy_data = cp.random.rand(100, 50, dtype=cp.float32)
# Can pass cupy_data directly to pylibraft functions like eigsh()
# pylibraft -> NumPy (copy)
numpy_arr = raft_arr.copy_to_host()RAFT functions accept any object implementing __cuda_array_interface__ as input — you don't need to convert to device_ndarray first. This means CuPy arrays, Numba device arrays, PyTorch CUDA tensors, and cuDF columns all work directly.
Performance Tips
Reuse DeviceResources. Creating a
DeviceResourcesallocates CUDA library handles (cuBLAS, cuSOLVER). Create once, pass to all calls.Batch your syncs. RAFT calls are asynchronous. Queue multiple operations before calling
handle.sync()rather than syncing after each one.Choose precision by residual and conditioning checks. Throughput ratios are hardware-specific; float32 is not automatically adequate for spectral problems.
Pre-allocate outputs. Many RAFT functions accept an
outparameter. Pre-allocating avoids repeated GPU memory allocation.Keep data on GPU. RAFT interoperates with CuPy, cuDF, and cuML via
__cuda_array_interface__. Pass GPU arrays directly between libraries instead of round-tripping through CPU.
Common Pitfalls
Forgetting to sync. RAFT operations are asynchronous. Reading results without calling
handle.sync()gives undefined/stale data. If you omit thehandleparameter, RAFT syncs internally (safe but slower).Using RAFT for vector search. Vector search (k-NN, IVFPQ, CAGRA, etc.) has been migrated to cuVS. RAFT no longer maintains these algorithms.
Wrong sparse format.
eigsh()requirescupyx.scipy.sparse.csr_matrix. Other sparse formats (COO, CSC) must be converted first.Matrix contract. The 26.08 Python implementation supports real symmetric float32/float64 CSR matrices. Despite broad Hermitian wording in the docstring, complex values raise an unsupported-dtype error. Validate symmetry, residuals and orthogonality; compare eigenspaces for repeated eigenvalues rather than vector signs.
dtype mismatch. RAFT functions are picky about dtypes. Use
float32orfloat64explicitly — don't rely on implicit conversion.
Requirements and compatibility
Works with: Claude Code, Claude apps, OpenAI Codex, GitHub Copilot, Cursor, Gemini CLI, Kiro, OpenCode, Goose, Amp, Roo Code, JetBrains Junie, Factory Droid, Devin (ex-Windsurf), Mistral Vibe, OpenHands, Letta
“Works with” means the tool reads the open Agent Skills format; a skill written for one tool may use features others lack.
Needs: Needs network access, Needs Python
The author says: Requires an NVIDIA CUDA-capable GPU for GPU execution. RAPIDS 26.08 requires Python 3.11-3.14 on Linux or WSL2, NumPy 2, CuPy 14, and compatible CUDA 12 or 13 wheels. Package installation needs network access.
Security
No issues found by our static scan· No issues found
A static scan is not a guarantee. Skills are third-party content: review a skill before you let an agent use it.
Attribution and licence
- Created by
- K-Dense, Inc.
- Publisher
- K-Dense (Community)
- Source
- K-Dense-AI/scientific-agent-skills · skills/optimize-for-gpu · commit a25cf9e
- Licence
- MIT License (redistribution allowed)
- LICENSE (added by AutoGineer from LICENSE.md)
- ATTRIBUTION.md (written by AutoGineer)
- Synced
AutoGineer is not affiliated with or endorsed by K-Dense, Inc. or K-Dense.
Download ZIP
The ZIP holds the skill’s files, its licence files and an ATTRIBUTION.md. Download optimize-for-gpu.zip