Testing Qwen3.8-27B KV cache dtypes
Qwen3.8-27B FP16: Is there a quality difference between FP8 and FP16 for the KV cache?
Local LLMvLLMDeveloper toolsQwen3.8
Chronological record
Journal
Experiments, benchmarks, failures and findings. Newest first; corrections stay visible.
15 entries
Serving Qwen3.8-27B with vLLM on four RTX 3090s
The model, memory and gateway configuration behind the long-context language-model service running on mlrig.
Local AIQwen3.8vLLMLong contextInference
mlrig: six RTX 3090s under Proxmox
A technical overview of the GPU compute host used for local language models, numerical experiments and isolated rental workloads.
Local AIHomelabProxmoxGPU computingvLLM
Running Roo Code against local vLLM models
Notes from configuring Roo Code with locally hosted DeepSeek and GPT-OSS models through vLLM.
Local AIvLLMDeveloper tools
Porter-Thomas fluctuations
A working note on the Porter-Thomas distribution and fluctuations in reduced transition strengths.
StatisticsNuclear physicsPython
Which values to choose for gl and gs?
Comparing orbital and spin contributions to calculated M1 strength functions.
Nuclear physicsM1KSHELL
Orbital contributions to the LEE
Removing selected one-body transition-density contributions to identify which orbitals produce the low-energy enhancement.
Nuclear physicsKSHELLData analysis
Another possible bug in the OBTD calculations: Why are excitations stronger than decays?
Investigating why apparent excitation contributions exceed decay contributions in OBTD grids.
Nuclear physicsOBTDKSHELL
[SOLVED] Possible bug in the OBTD calculations
Tracing how KSHELL transition states are ordered when OBTD data is loaded.
Nuclear physicsOBTDKSHELL
Visualising OBTDs
Visualising orbital contributions in one-body transition densities for selected M1 transitions.
Nuclear physicsOBTDKSHELL
Giant Resonances
Notes about pygmy resonances and the scissors mode in nuclear physics.
Nuclear physicsGiant resonances
So what is the one-body transition density?
Working notes about one-body transition operators, one-body transition densities, and second quantisation.
Nuclear physicsOBTDShell model
Overview of effective interactions
An overview of effective interactions and their role in nuclear shell-model calculations.
Nuclear physicsShell modelInteractions
GPU acceleration of the TBME calculation
Mapping a symmetric shell-model Hamiltonian onto GPU threads reduced a 186-second CPU calculation to 1.26 seconds.
CUDAC++Computational physics
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