通知公告
9月9日|Method of detection of Dark Energy-Dark Matter interaction in Non-virialised clusters
報(bào)告題目：Method of detection of Dark Energy-Dark Matter interaction in Non-virialised clusters
報(bào)告人： Morgan Le Delliou 博士（巴西圣保羅州立大學(xué)理論物理研究所博士后）
時(shí)間安排：2016年9月9日（星期五）下午3：00
地點(diǎn)：近代物理所5號(hào)樓1006會(huì)議室
報(bào)告人簡(jiǎn)介：
Morgan Le Delliou 博士，是巴西圣保羅州立大學(xué)理論物理研究所博士后， 1995年獲得巴黎Xi—Orsay大學(xué)理論物理碩士；2002年獲得加拿大Queen 大學(xué)理論物理博士學(xué)位。他主要從事暗物質(zhì)暈結(jié)構(gòu)和暗能量分析、非線性結(jié)構(gòu)的成因. 主要工作發(fā)表在MNRAS, Astronomy and Astrophysics, JCAP, PLB, GRG, 和 PRD.
報(bào)告內(nèi)容摘要：
the possibility of detection of Dark matter–Dark energy interaction. In particular, we try to detect the effects from such interaction in the balance of general clusters and for that purpose, we evaluate the departure from virial equilibrium of unbalanced clusters. We extend the use, from previous works, of the Layzer–Irvine equation for dynamical virial evolution of a simple model of interacting dark sector, with weak lensing and X-ray observations giving respectively the mass profiles and the intracluster gas temperatures. Selecting a set of clusters, we generate measurements, through a Monte Carlo method, of observed virial ratios, interaction strength, rest virial ratio and departure from equilibrium factors. We found a compounded interaction strength for the set of clusters of $?1.61^+2.23_?16.34$, compatible with no interaction, but acompounded rest virial ratio of $?0.78 ± 0.13$, which would entail a 2σ detection. We confirm quantitatively that clusters of galaxies are out of equilibrium but further investigation is needed to constrain a possible interaction in the dark sector.
