论文标题
暗物质现象的范式和场景
Paradigms and Scenarios for the Dark Matter Phenomenon
论文作者
论文摘要
圆盘系统中黑暗和发光物质的结构特性之间的众所周知的缩放定律太复杂了，无法由两个仅具有相同重力场的惰性成分产生。这使我们重点关注了30年的范式，该范式基于对暗物质本质（DM）的先验知识，这使我们陷入了限制的场景，尤其是偏爱无碰撞的$λ$ Cold Cold Dark Matter。在这种观察证据的推动下，我们建议通过遵循新的范式来解决暗物质的奥秘：必须通过深入分析银河尺度上的深色和发光质量分布的特性来猜测/得出DM的性质。该范式的立即应用使我们发现黑暗和标准模型颗粒之间存在直接相互作用，从而塑造了星系的内部区域。
Well known scaling laws among the structural properties of the dark and the luminous matter in disc systems are too complex to be arisen by two inert components that just share the same gravitational field. This brings us to critically focus on the 30 year old paradigm, that, resting on a priori knowledge of the nature of dark matter (DM), has led us to a restricted number of scenarios, especially favouring the collisionless $Λ$Cold Dark Matter one. Motivated by such observational evidence, we propose to resolve the dark matter mystery by following a new paradigm: the nature of DM must be guessed/derived by deeply analyzing the properties of the dark and luminous mass distribution at galactic scales. The immediate application of this paradigm leads us to the existence of a direct interaction between dark and Standard Model particles which has finely shaped the inner regions of galaxies.
