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Testing cold dark matter vs. modified gravity with Milky Way's stellar kinematic data

发布时间:2016-12-02

期数 主 讲 人
讲座时间 地 点

题目:Testing cold dark matter vs. modified gravity with Milky Way's stellar kinematic data

报 告 人:董小波 研究员

单 位:云南天文台

时 间:2016年12月05日(周一)14:30

地 点:厦门大学海韵园物理机电航空大楼407

摘 要: Using for the first time both the rotation curve data V_rot(R) and the vertical velocity dispersion data sigma(R) of the Milky Way (MW) stars, we test and verify the self-consistency of the quasi-linear formulation of modified newtonian dynamics (QUMOND, Milgrom 2010).

Then, using QUMOND as an effective/practical tool and based purely on the baryonic distribution of the MW, we derive the 3-dimensional distribution of the effective gravitational field (Phi_phantom) of the putative dark matter (DM) halo in the popular DM paradigm. The effective gravitational field Phi_phantom appears not easy to realize with commonly used density profiles of CDM theory.

Lastly we propose expects for mapping the 3-dimensional MW's gravitational field in the LAMOST and GAIA era.