论文标题
关于冷暗物质的性质和起源的假设
Hypothesis on the nature and origin of cold dark matter
论文作者
论文摘要
天体物理学和宇宙学上最大的奥秘之一是冷暗物质的性质和起源，它代表了宇宙中质量的84％以上。暗物质反应并产生引力，并控制银河中心周围恒星的动力学，但是，不会吸收或发射任何类型的电磁辐射。到目前为止，与已知物质类型的任何关系尚未确定，尚未找到拟议的新粒子。在这里，我提出并讨论了暗物质是如何从超轻的费米颗粒中演变而成的，这些颗粒与大爆炸后不久与宇宙的其余部分分离。我的描述明确考虑了它们的干扰，并揭示了两个这样的粒子之间的纠缠以及它们向大规模的宇宙大小的巨大深色量子场的转变。此外，我认为暗物质和超大型黑洞具有相同的起源，并且同时发展。如果粒子的脱钩时间大约是大爆炸后的半秒钟，我的假设预测，超级质量黑洞的最小质量非常适合50,000个太阳能的最小此类物体。超轻的费米粒子似乎很可能是中微子。
One of the greatest mysteries in astrophysics and cosmology is the nature and the origin of cold dark matter, which represents more than 84% of the mass in the universe. Dark matter reacts on and produces gravitational forces and governs the dynamics of stars around galactic centres, however, does not absorb or emit any kind of electromagnetic radiation. So far, any relation to known types of matter has not been conclusive, and proposed new particles have not been found. Here, I propose and discuss how dark matter evolved from ultra-light fermionic particles that decoupled from the rest of the universe shortly after the Big Bang. My description explicitly considers their interference, and reveals the emergence of entanglement between two such particles, as well as their transformation to massive dark-matter quantum fields of cosmic sizes. Furthermore, I argue that dark matter and supermassive black holes have the same origin and evolved simultaneously. If the particles' decoupling time was about half a second after the Big Bang, my hypothesis predicts a minimum mass for supermassive black holes that fits well to the smallest known such object of 50,000 solar masses. It seems very much likely that the ultra-light fermionic particle was the neutrino.
