论文标题
暗物质星星
Dark matter stars
论文作者
论文摘要
CGF宇宙学中的暗物质是宇宙学SU（2）-Weak仪表（CGF）。 TOV恒星结构方程是用该暗物质组成的恒星数值求解的。星级M可以将任何值提高到最高$ 9.14 \ times 10^{ - 6} $ m_sun。对于m的每个值，恒星半径r位于5.23厘米至13.6厘米之间。当m> $ 5.09 \ times 10^{ - 6} $ m_sun时，可能会有多个r的值。对于那些恒星，从较大的r到较小的r的过渡将以$ 10^{41} $ j的顺序释放重力能量，以$ 10^{ - 10} $ s的顺序。
The dark matter in the CGF cosmology is a cosmological SU(2)-weak gauge field (the CGF). The TOV stellar structure equations are solved numerically for stars composed of this dark matter. The star mass M can take any value up to a maximum $9.14 \times 10^{-6}$ M_sun. For each value of M the star radius R lies between 5.23cm and 13.6cm. More than one value of R is possible when M > $5.09 \times 10^{-6}$ M_sun. For those stars, a transition from larger to smaller R would release gravitational energy on the order of $10^{41}$J in a time on the order of $10^{-10}$s.
