通过截断的M分数Lane-Emden解决方案进行恒星结构
Mohamed I Nouh1, Emad A-B Abdel-Salam2, Abaker A Hassaballa3,4
1Astronomy Department, National Research Institute of Astronomy and Geophysics, Helwan, Cairo, 11421, Egypt.
Scientific reports
|April 11, 2025
概括
本研究介绍了使用截断的M分数导数对Lane-Emden方程的分数概括. 分数模型显示,恒星半径和质量随着分数参数的减少而减少,影响恒星结构的洞察力.
科学领域:
- 天体物理学和计算物理
- 恒星结构和进化过程
- 分数计算的应用 分数计算的应用
背景情况:
- 莱恩-埃姆登方程模型的自我引力,球形对称的多热带恒星在水静电平衡.
- 在天体物理学中,它对于理解正常恒星,白矮星和天体系统至关重要.
- 传统模型缺乏在恒星物理中纳入复杂的分数行为框架.
研究的目的:
- 引入使用截断的M分数导数 (TMD) 的莱恩-埃姆登方程的新型分数概括.
- 探索微积分计算对多热带气体球体结构性质的影响.
- 开发新的多热带恒星模型,超出经典的Lane-Emden框架.
主要方法:
- 截断的M分数Lane-Emden方程 (TMD-LEE) 的公式.
- 应用加速功率序列方法来解决TMD-LEE.E的应用.
- 在各种多热带指数中生成分数多热带模型.
主要成果:
- 获得了TMD-LEE的解决方案,创建了分数多热带模型.
- 分数Lane-Emden函数的初始零数随着分数参数的减少而增加.
- 在这些分数模型中,恒星半径和质量随着分数参数的减少而减少.
结论:
- 分数因素显著影响恒星的结构缩放,为恒星物理提供了新的见解.
- 开发的分数多变形模型扩展了古典多变形理论.
- 这些模型在分数计算框架内理解复杂的天体物理现象方面具有潜在的应用.
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