论文标题
银河中心内部parsec中的脉冲星可以探测暗物质的存在吗？
Can Pulsars in the inner parsecs from Galactic Centre probe the existence of Dark Matter?
论文作者
论文摘要
鉴于脉冲星对银河系中暗物质的分布的质量依赖性，我们讨论了暗物质环境中深色紧凑物体的形成。我们的结果表明，由于暗物质的捕获，脉冲星质量应减少朝向银河系中心的中心，从而成为对暗物质的存在和性质的探测。因此，我们建议，在深色物质环境中，Pulsar质量的演变与未来的实验相结合，在我们的Galaxy Halo暗物质概况，暗物质粒子质量和暗物质自我相互作用强度上的特征时，可以使用约束。
We discuss the formation of dark compact objects in a dark matter environment in view of the possible mass dependence of pulsars on the distribution of dark matter in the Galaxy. Our results indicate that the pulsar masses should decrease going towards the center of the Milky Way due to dark matter capture, thus becoming a probe for the existence and nature of dark matter. We thus propose that the evolution of the pulsar mass in a dark matter rich environment can be used to put constraints, when combined with future experiments, on the characteristics of our Galaxy halo dark matter profile, on the dark matter particle mass and on the dark matter self-interaction strength.
