摘要
Why no late type M and much later type N white dwarfs with surface temperatures less than 3000 K had ever been observed? What are the heat sources of these later type white dwarfs? In this paper, we find that the energy source of white dwarfs is the nucleons decay catalyzed by magnetic monopoles.
Why no late type M and much later type N white dwarfs with surface temperatures less than 3000 K had ever been observed? What are the heat sources of these later type white dwarfs? In this paper, we find that the energy source of white dwarfs is the nucleons decay catalyzed by magnetic monopoles.
作者
Qiuhe Peng
Jingjing Liu
Qiuhe Peng;Jingjing Liu(Department of Astronomy, Nanjing University, Nanjing, China;College of Science, Hainan Tropical Ocean University, Sanya, China)
