https://numericastronomy.com/tags/numericalsubgrid/Recent content in Numerical:subgrid on NumericAstronomyHugozh-cnFri, 24 Jul 2026 00:00:00 +0000https://numericastronomy.com/posts/2026-06-25-hydrodynamic-01/Thu, 25 Jun 2026 00:00:00 +0000https://numericastronomy.com/posts/2026-06-25-hydrodynamic-01/<blockquote> <p><strong>原文信息</strong></p> <p><strong>出处</strong>：Numerical Simulations in Cosmology: Chapter 3 — Hydrodynamic methods and sub-resolution models for cosmological simulations</p> <p><strong>作者</strong>：Milena Valentini (Universitá degli Studi di Trieste / INAF), Klaus Dolag (LMU München / MPI for Astrophysics)</p> <p><strong>arXiv</strong>：<a href="https://arxiv.org/abs/2502.06954">arXiv:2502.06954</a> <strong>页数</strong>：61 页，14 幅图</p> <p><strong>翻译说明</strong>：<div class="en-block"> <div class="en-zh">中文翻译，段落对照，上面是中文，下面是英文。</div><p class="en-en">Chinese translation, paragraph by paragraph, with Chinese on top and English below.</p></div> <span class="annotate-block" data-annotation="这是示例"> 虚线下划线 </span> 为个人添加的注释或评论。文献引用如 <sup class="citation" data-ref="K. Yoshikawa, N. Yoshida, and M. Umemura, Direct Integration of the Collisionless Boltzmann Equation in Six-dimensional Phase Space: Self-gravitating Systems, ApJ. 762, 116, (2013)." onclick="event.stopPropagation();var t=this;var ct=document.querySelector('.cite-tooltip');if(ct)ct.remove();navigator.clipboard.writeText(this.getAttribute('data-ref')).then(function(){t.classList.add('copied');setTimeout(function(){t.classList.remove('copied')},1200)});event.preventDefault()"><a href="#ref-Yoshikawa2013" id="cite-Yoshikawa2013">[1]</a></sup> 可点击复制完整引用信息。</p>