The triple-alpha-reaction at low temperatures
The triple-alpha-reaction at low temperatures
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低温下的三α反应
DOI：
10.1007/bf01325126
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发表时间：
1986
期刊：
影响因子：
--
通讯作者：
F. Thielemann
中科院分区：
文献类型：
--
作者：
K. Langanke;M. Wiescher;F. Thielemann
我们研究了在吸积白色矮星和中子星方面具有重要意义的低温三重α反应。虽然我们在几个方面改进了Nomoto，Thielemann和Miyaji最近的研究，但我们发现相关温度范围（T=107 - 108 K）的反应速率与以前的结果非常相似。特别是，我们改进的研究证实了在温度T白色矮星上氦可能被点燃。
We have studied the triple-α-reaction at low temperatures which is of importance on accreting white dwarfs and neutron stars. Although we have improved a recent investigation of Nomoto, Thielemann and Miyaji on several points, we find a reaction rate for the relevant temperature range (T=107−108K) which is rather similar to the previous result. In particular, our improved study confirms that helium might be ignited on accreting white dwarfs at temperaturesT≦4.107 K.