论文标题
暗物质和哈勃参数张力的自旋张量
The Spin Tensor of Dark Matter and the Hubble Parameter Tension
论文作者
论文摘要
允许对冷暗物质进行无刺激的自旋张量（$ω_ {\ mathrm {dm}} = 0 $）的结果是产生有效的$ \ mathrm {flrw} $动力学，而有效的暗物质密度（$ -1/3 <\ ymath）均具有小的负压稳定（$ -1/3事实证明，这可以直接地解决哈勃参数张力。
Allowing for a nonvanishing spin tensor for cold dark matter ($ω_{\mathrm{DM}}=0$) has the consequence of giving rise to an effective $\mathrm{FLRW}$ dynamics with a small negative barotropic constant for an effective dark matter density ($-1/3<ω_{\mathrm{eff}}\leq0$). This turns out to solve the Hubble parameter tension in a straightforward way.
