星系暗晕中心表面密度的共形理论

Robert K. Nesbet
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引用次数: 0

摘要

许多关于星系晕引力的暗物质研究都依赖于具有核心半径 $r_0$ 和中心密度 $\rho_0$ 的模型。研究发现,对于更大范围的星系来说,中心表面密度乘积 $\rho_0 r_0$ 几乎是一个普遍常数。在没有暗物质的情况下,假设引力和希格斯标量场具有韦尔保角对称性的标准变分场论意味着非经典的向心加速度 $\Delta a$,为$a=a_N+\Delta a$,其中牛顿加速度 $a_N$ 是由于可观测的重子物质造成的。忽略星系半径非常大时的光晕截止,共形$\Delta a$在整个光晕中是恒定的,而$a=a_N+\Delta a$是一个通用函数,这与最近的一项星系研究是一致的,它约束了暗物质或替代理论引起的加速度。一个等效的暗物质源是一个纯粹的尖顶分布,其截止参数由阿罗边界半径决定。这意味着任何暗物质核心模型都具有普遍的中心表面密度。
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Conformal theory of central surface density for galactic dark halos
Numerous dark matter studies of galactic halo gravitation depend on models with core radius $r_0$ and central density $\rho_0$. Central surface density product $\rho_0 r_0$ is found to be nearly a universal constant for a large range of galaxies. Standard variational field theory with Weyl conformal symmetry postulated for gravitation and the Higgs scalar field, without dark matter, implies nonclassical centripetal acceleration $\Delta a$, for $a=a_N+\Delta a$, where Newtonian acceleration $a_N$ is due to observable baryonic matter. Neglecting a halo cutoff at very large galactic radius, conformal $\Delta a$ is constant over the entire halo and $a=a_N+\Delta a$ is a universal function, consistent with a recent study of galaxies that constrains acceleration due to dark matter or to alternative theory. An equivalent dark matter source is a pure cusp distribution with cutoff parameter determined by a halo boundary radius. This is shown here to imply universal central surface density for any dark matter core model.
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