杨光弟, 傅永平, 费秀海. 星体内部的暗物质粒子[J]. 云南大学学报(自然科学版), 2018, 40(4): 693-696. doi: 10.7540/j.ynu.20170501
引用本文: 杨光弟, 傅永平, 费秀海. 星体内部的暗物质粒子[J]. 云南大学学报(自然科学版), 2018, 40(4): 693-696. doi: 10.7540/j.ynu.20170501
YANG Guang-di, FU Yong-ping, FEI Xiu-hai. Dark matter particle in the isotropic star[J]. Journal of Yunnan University: Natural Sciences Edition, 2018, 40(4): 693-696. DOI: 10.7540/j.ynu.20170501
Citation: YANG Guang-di, FU Yong-ping, FEI Xiu-hai. Dark matter particle in the isotropic star[J]. Journal of Yunnan University: Natural Sciences Edition, 2018, 40(4): 693-696. DOI: 10.7540/j.ynu.20170501

星体内部的暗物质粒子

Dark matter particle in the isotropic star

  • 摘要: 从量子力学角度研究了暗物质与星体的相互作用,通过暗物质粒子的性质分析,星体内部的暗物质粒子受引力势作用,构成球谐振子.求解三维各向同性暗物质粒子谐振子的Schrödinger方程,得到其波函数及能量,并得到能量子的表达式和具体数值.

     

    Abstract: The gravitational interaction of the dark matter and the star is calculated by using the quantum mechanics.The gravitational potential energy and dark matter constitute a spherical harmonic oscillator system. The wave functions and the energies of the system are obtained by solving the Schrödinger equation of the isotropic harmonic oscillator.

     

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