The El Gordo Galaxy Cluster Challenges ?CDM for Any Plausible Collision Velocity

被引：13

作者：

Asencio, Elena ^{[1
]}

Banik, Indranil ^{[2
]}

Kroupa, Pavel ^{[1
,3
]}

机构：

[1] Univ Bonn, Helmholtz Inst Strahlen & Kernphys HISKP, Nussallee 14-16, D-53115 Bonn, Germany

[2] Univ St Andrews, Scottish Univ Phys Alliance, St Andrews KY16 9SS, Fife, Scotland

[3] Charles Univ Prague, Astron Inst, Fac Math & Phys, 5 Holesovickach 2, CZ-18000 Prague 8, Czech Republic

来源：

ASTROPHYSICAL JOURNAL | 2023年 / 954卷 / 02期

基金：

英国科学技术设施理事会;

关键词：

Galaxy clusters; Large-scale structure of the universe; Gravitation; Dark matter; ACT-CL J0102-4915; OBJECTS; MERGER; HALO;

D O I：

10.3847/1538-4357/ace62a

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

El Gordo (ACT-CL J0102-4915) is an extraordinarily large and bright galaxy cluster collision. In a previous study, we found that El Gordo is in 6.2 sigma tension with the. cold dark matter (.CDM) standard model when assuming the nominal mass and infall velocity values from the hydrodynamical simulations of Zhang et al. (M-200 = 3.2 x 10(15)M circle dot. and Vinfall = 2500 km s(-1), respectively). The recent weak-lensing study of Kim et al. showed that the mass of El Gordo is actually 2.13+(+0.25)(-0.23) x 10(15)M circle dot. Here we explore the level of tension between El Gordo and.CDM for the new mass estimate, assuming several Vinfall values. We find that in order to reduce the tension below the 5s level, the El Gordo subclusters should have Vinfall < 2300 km s(-1) (V-infall < 1800 km s(-1) when considering the combined tension with the Bullet Cluster). To the best of our knowledge, the El Gordo hydrodynamical simulations conducted so far require V-infall. 2500 km s(-1) to simultaneously reproduce its morphology and its high X-ray luminosity and temperature. We therefore conclude that El Gordo still poses a significant challenge to.CDM cosmology. Whether the properties of El Gordo can be reconciled with a lower Vinfall should be tested with new hydrodynamical simulations that explore different configurations of the interaction.

引用

页数：6

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