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Accurate and Efficient Low-Rank Model Merging in Core Space
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Proposes Core Space, a lossless shared low-rank basis for merging LoRA-adapted models so any merging method (TA, TIES, TSV, Iso-C, CART) runs on small r-dimensional-per-task cores instead of full weight matrices.
Problem
Merging LoRA-adapted models is suboptimal when done on low-rank products directly, and alignment-based merging (KnOTS) requires full-size SVDs that are costly for large models.
Approach
Build shared reference bases via SVD of stacked LoRA A and B factors across tasks, project each task's LoRA update into a Tr x Tr core matrix that is exactly reconstructible, then apply any merging operator in this compact aligned space.
Key results
- On Llama 3 8B NLI, TSV in Core Space reaches 94.16% average normalized accuracy, versus 92.55% for TSV in full space, at roughly 280x lower relative merge time.
- On ViT-B/32 vision tasks, TSV + Iso-C in Core Space achieves 76.43% average normalized accuracy, above the prior best of 68.0% (TIES in KnOTS space).
- Core Space improves 8 of 9 merging methods versus full space on ViT-B/32 and provides up to ~600x merging speed-up over KnOTS on Llama 3 8B.
Measured effects reported in the paper
| What was changed | Where | Measured | Effect |
|---|---|---|---|
| merge TIES in Core Space rather than Full Space | TIES · Llama 3 8B NLI tasks | average normalized accuracy: 91.08 -> 93.30 | Helped |
| merge DARE-TIES in Core Space rather than Full Space | DARE-TIES · Llama 3 8B NLI tasks | average normalized accuracy: 89.44 -> 93.32 | Helped |
| merge TSV in Core Space rather than Full Space | TSV · Llama 3 8B NLI tasks | average normalized accuracy: 92.55 -> 94.16 | Helped |
| merge TIES in Core Space rather than KnOTS Space | TIES · ViT-B/32 vision tasks | average normalized accuracy: 67.73 -> 68.63 | Helped |
| merge DARE-TIES in Core Space rather than KnOTS Space | DARE-TIES · ViT-B/32 vision tasks | average normalized accuracy: 64.91 -> 69.39 | Helped |
| merge TSV in Core Space rather than Full Space | TSV · ViT-B/32 vision tasks | average normalized accuracy: 66.66 -> 66.41 | Hurt |
| merge CART in Core Space rather than Full Space | CART · ViT-B/32 vision tasks | average normalized accuracy: 71.52 -> 73.44 | Helped |
| merge TIES + Iso-C in Core Space rather than KnOTS Space | TIES + Iso-C · ViT-B/32 vision tasks | average normalized accuracy: 72.47 -> 75.44 | Helped |
| merge DARE-TIES + Iso-C in Core Space rather than KnOTS Space | DARE-TIES + Iso-C · ViT-B/32 vision tasks | average normalized accuracy: 67.36 -> 75.70 | Helped |
| merge TSV + Iso-C in Core Space rather than KnOTS Space | TSV + Iso-C · ViT-B/32 vision tasks | average normalized accuracy: 74.02 -> 76.43 | Helped |
| merge CART + Iso-C in Core Space rather than KnOTS Space | CART + Iso-C · ViT-B/32 vision tasks | average normalized accuracy: 71.09 -> 76.15 | Helped |
| use the concatenated reference basis instead of the first task's basis (ablation) | TIES-Core · ViT-B/32 vision tasks | average accuracy: 60.4 -> 68.6 | Helped |
Surprising findings
- Full-space TIES yields merged updates of effective rank ~766 instead of the intended 128, because trimming destroys the low-rank structure.
- In full space, up to 80% of singular values can be truncated from a Task Arithmetic merged model without accuracy loss, whereas in Core Space any truncation hurts.
Limitations
- Core Space dimension Tr grows with number of tasks and rank, so the core cost grows as T^3 r^3 with many tasks or large ranks.
- Evaluated only on 8 vision tasks and 6 NLI tasks with a single LoRA rank setup in main results.
Experimental setup
Datasets: Cars DTD EuroSAT GTSRB MNIST RESISC45 SUN397 SVHN SNLI MNLI SICK QNLI
Benchmarks: Cars DTD EuroSAT GTSRB MNIST RESISC45 SUN397 SVHN SNLI MNLI SICK QNLI
Metrics: normalized accuracy absolute accuracy merging time
Baselines: Task Arithmetic TIES DARE-TIES TSV CART Iso-C KnOTS
Builds on: LoRA KnOTS Task Arithmetic Iso-C TSV
Closest papers by meaning
- SDS-LoRA: Overcoming Anisotropic Gradient Scaling in Low-Rank Adaptation (NeurIPS 2026 · similarity 0.91)
- Flat-LoRA: Low-Rank Adaptation over a Flat Loss Landscape (ICML 2025 · similarity 0.91)
- The Expressive Power of Low-Rank Adaptation (ICLR 2024 · similarity 0.90)
- Merging LoRAs like Playing LEGO: Pushing the Modularity of LoRA to Extremes Through Rank-Wise Clustering (ICLR 2025 · similarity 0.90)
- RandLoRA: Full rank parameter-efficient fine-tuning of large models (ICLR 2025 · similarity 0.89)
- LoRA+: Efficient Low Rank Adaptation of Large Models (ICML 2024 · similarity 0.89)
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