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Taoran Li

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Published work

3 published item(s)

preprint2026arXiv

Chain of Risk: Safety Failures in Large Reasoning Models and Mitigation via Adaptive Multi-Principle Steering

Large reasoning models (LRMs) increasingly expose chain-of-thought-like reasoning for transparency, verification, and deliberate problem solving. This creates a safety blind spot: harmful or policy-violating content may appear in reasoning traces even when final answers appear safe. We test whether final-answer safety is a sufficient proxy for the full reasoning-answer trajectory by scoring both stages under a unified twenty-principle safety rubric. Using prompts from seven public harmfulness and jailbreak sources, plus four out-of-distribution (OOD) sources, we evaluate 15 open-weight and API-based LRMs across 41K prompts per model. Reasoning traces consistently reveal additional safety risks beyond final answers, especially in high-severity stage-wise failures: leak cases, where unsafe reasoning precedes a safe-looking answer, and escape cases, where benign-looking reasoning precedes an unsafe final response. Principle-level analysis shows that risk concentrates in misinformation, legal compliance, discrimination, physical harm, and psychological harm. We further propose adaptive multi-principle steering, a white-box test-time mitigation that learns one unsafe-to-safe activation direction per safety principle and activates only directions whose current hidden state is closer to the unsafe than safe centroid. On three steerable open reasoning models, adaptive steering reduces unsafe counts in both reasoning traces and final answers on held-out and OOD benchmarks. DeepSeek-R1-Qwen-7B achieves a 40.8% average unsafe-count reduction while retaining 97.7% macro-averaged accuracy on BBH, GSM8K, and MMLU. These results suggest that LRM safety should be evaluated and mitigated over the full exposed reasoning-answer trajectory, not only at the final-answer stage.

preprint2021arXiv

Wind environment analysis of ground-based optical observatory

The telescopes and the infrastructures may alter the local wind environment around the observatory and further affect the observing environment. After the completion of site testing, it is necessary to analyze the wind environment of the entire site and plan the telescope layout to make use of the excellent conditions scientifically and rationally. Taking a typical observatory as an example, the effect of topographical features on wind environment and the mutual interference between telescope enclosures are analyzed by using Computational Fluid Dynamics (CFD) method. The CFD simulations are compared with the seeing data from Differential Image Motion Monitor (DIMM), the results are in good agreement, which verifies the effectiveness of the CFD method. The results of wind environment analysis can provide reasonable suggestions for site layout and construction, improving the observing environment and the image quality.

preprint2019arXiv

Stray light analysis of the Xinglong 2.16m telescope

An effort towards understanding of the stray light problems for the Xinglong 2.16-m telescope was presented to estimate the stray light performance of the telescope itself and provide a method for improving the stray light suppression. The stray light analysis for 2.16-m telescope model, which consists the onion shaped dome, telescope structure, equatorial mount and telescope optics, has been performed with two cases (1) point to 60° and (2) point to zenith, in both azimuth and elevation direction. The Point Source Normalized Irradiance Transmittance (PSNIT), which is generally used for assessing stray light and uncorrelated to entrance aperture, was calculated with a series of off-axis angles. It shows that the PSNIT values are less than 10-7 when off-axis angles are larger than 20°. The dominant contributors of stray light (primary and secondary mirror, telescope structure and dome) were identified to give advice for performance improvement. The analyses indicate that significant benefit can be realized with adding only 5 vanes inside the bottom portion of the secondary baffle. In the case of point to zenith, the PSNIT values will decrease about 40% at average.