用动态时间规整对双星演化轨迹对齐,提升插值精度
Irregularly Sampled Time Series Interpolation for Binary Evolution Simulations Using Dynamic Time Warping
- 基于动态时间规整实现多参数同步对齐,构建统一时间网格
- 在多种双星配置下优于现有方法,保持斯特藩-玻尔兹曼定律等物理关系
- 适合需要高精度双星演化模拟的天体物理研究者
双星演化模拟计算成本高昂,星族合成依赖于这些详细模型。生成数千个模型需数百小时CPU时间,而轨道插值可显著降低开销。单星轨道插值简单,但双星系统中恒星相互作用引入复杂性,使传统单轨插值方法失效。双星演化轨迹因相互作用导致路径剧烈变化并产生难以捕捉的不连续性,与单星演化有本质不同。本文提出一种基于动态时间规整的新方法,通过计算所有物理参数的共享规整路径,实现轨道对齐与迭代平均。该方法在统一时间网格上保留参数间的因果关系,实验表明其能有效维持斯特藩-玻尔兹曼定律等关键物理关系。在多个双星配置下的综合评估显示,正确的时间对齐对插值至关重要,所提方法持续优于现有方案,可高效生成更准确的双星群体样本用于天体物理研究。
原文摘要 · Abstract (English)
Binary stellar evolution simulations are computationally expensive. Stellar population synthesis relies on these detailed evolution models at a fundamental level. Producing thousands of such models requires hundreds of CPU hours, but stellar track interpolation provides one approach to significantly reduce this computational cost. Although single-star track interpolation is straightforward, stellar interactions in binary systems introduce significant complexity to binary evolution, making traditional single-track interpolation methods inapplicable. Binary tracks present fundamentally different challenges compared to single stars, which possess relatively straightforward evolutionary phases identifiable through distinct physical properties. Binary systems are complicated by mutual interactions that can dramatically alter evolutionary trajectories and introduce discontinuities difficult to capture through standard interpolation. In this work, we introduce a novel approach for track alignment and iterative track averaging based on Dynamic Time Warping to address misalignments between neighboring tracks. Our method computes a single shared warping path across all physical parameters simultaneously, placing them on a consistent temporal grid that preserves the causal relationships between parameters. We demonstrate that this joint-alignment strategy maintains key physical relationships such as the Stefan-Boltzmann law in the interpolated tracks. Our comprehensive evaluation across multiple binary configurations demonstrates that proper temporal alignment is crucial for track interpolation methods. The proposed method consistently outperforms existing approaches and enables the efficient generation of more accurate binary population samples for astrophysical studies.
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