Stau催化的d-t Nuclear Fusion
Stau-catalyzed d-t Nuclear Fusion
摘要：
质量为10-100 GeV的引力子是超引力中一个很好的激发方案。如果Stau是次轻的超对称粒子，它的寿命将达到$10^{6-8}$秒的量级。如果是这样的话，Stau对核聚变产生了很大的影响，因为它是带电粒子。本文对stau催化的d-t核聚变进行了详细的计算。我们发现，如果满足一定的技术条件，利用核聚变作为能源并非没有希望。
英文摘要：
The gravitino of mass 10-100 GeV is a well motivated scenario in supergravity. If the stau is the next lightest supersymmetry particle, its life-time becomes order of $10^{6-8}$ sec. If it is the case the stau makes a big impact on the nuclear fusion, since it is a charged particle. In this paper we perform a detailed calculation of a stau-catalyzed d-t fusion. We find that if certain technical conditions are satisfied, it is not hopeless to use the nuclear fusion as a source of energy.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
