论文标题
红色物质在红色巨人中的影响
Effects of Dark Matter in Red Giants
论文作者
论文摘要
构成所有物质的五分之二的暗物质（DM）被认为是在宇宙进化的早期阶段产生的弱相互作用的非巴里型粒子。它可以通过重力相互作用影响宇宙中的各种宇宙结构。 DM在主要序列恒星和恒星残余物（如中子星和白矮人）中的影响已经进行了研究。红色巨型阶段是恒星进化的后期。在这项工作中，我们研究了具有DM混合的低质量红色巨人，以及如何有效地改变红色巨人的亮度，温度和寿命等红色巨人的内在特性。
Dark matter (DM) which constitutes five-sixths of all matter is hypothesised to be a weakly interacting non-baryonic particle, created in the early stages of cosmic evolution. It can affect various cosmic structures in the Universe via gravitational interactions. The effect of DM in main sequence stars and stellar remnants like neutron stars and white dwarfs has already been studied. Red giant phase is a late stage of the evolution of stars. In this work, we study, low-mass red giants stars with admixture of DM and how this can effectively change the intrinsic properties of red giants such as their luminosities, temperatures and lifetimes.
