发育中的白矮星冷却过程中的核心结晶和堆积
Pier-Emmanuel Tremblay1, Gilles Fontaine2, Nicola Pietro Gentile Fusillo3
1Department of Physics, University of Warwick, Coventry, UK. p-e.tremblay@warwick.ac.uk.
Nature
|January 11, 2019
概括
科学家们观察到白矮星的冷却速度有所放缓, 这种结晶会释放潜在的热量,显著延迟这些恒星残余的冷却过程.
科学领域:
- 天文学与天体物理学
- 恒星进化
- 凝聚物质物理学
背景情况:
- 白矮星是恒星的冷却残余,由电子退化压力支.
- 理论模型预测白矮星核中的相位转化,释放潜热并减缓冷却.
- 对这种结晶引起的冷却延迟缺乏直接的观察证据.
研究的目的:
- 在白矮星中寻找预测的结晶阶段过渡的观测证据.
- 量化白矮体结晶过程中隐性热释放引起的冷却延迟.
- 调查元素沉积中的重力能量在进一步减缓冷却中的作用.
主要方法:
- 分析了来自盖亚卫星的光度和偏数据,寻找距离太阳100帕塞克内的白矮星.
- 在这些白矮星的冷却过程中发现了堆积.
- 使用理论建模来解释堆积是由于核心结晶过程中的潜热释放.
主要成果:
- 在白矮星冷却过程中观察到显著的堆积, 表明偏离预期的冷却速度.
- 这种堆积是由白矮星核结晶时释放的潜在热量引起的.
- 发现了元素沉积释放的重力能量进一步促进了冷却延迟.
结论:
- 这项研究提供了白矮星核心结晶的第一个直接观测证据.
- 这些发现证实了暗热释放及其对白矮星冷却的重大影响的理论预测.
- 这些结果提高了我们对强度合库伦等离子体的能量释放的理解,并改善了恒星年龄的确定方法.
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