scholarly journals Numerical Simulations of Buoyancy Instabilities in Galaxy Cluster Plasmas with Cosmic Rays and Anisotropic Thermal Conduction

2008 ◽  
Vol 685 (1) ◽  
pp. 105-117 ◽  
Author(s):  
Y. Rasera ◽  
B. Chandran
2012 ◽  
Vol 541 ◽  
pp. A99 ◽  
Author(s):  
J. Aleksić ◽  
E. A. Alvarez ◽  
L. A. Antonelli ◽  
P. Antoranz ◽  
M. Asensio ◽  
...  

2020 ◽  
Vol 500 (3) ◽  
pp. 3151-3161
Author(s):  
Jacob Svensmark ◽  
Steen H Hansen ◽  
Davide Martizzi ◽  
Ben Moore ◽  
Romaine Tessier

ABSTRACT Dark matter (DM) dominates the properties of large cosmological structures such as galaxy clusters, and the mass profiles of the DM have been inferred for these equilibrated structures for years by using cluster X-ray surface brightnesses and temperatures. A new method has been proposed, which should allow us to infer a dynamical property of the DM, namely the velocity anisotropy. For the gas, a similar velocity anisotropy is zero due to frequent collisions; however, the collisionless nature of DM allows it to be non-trivial. Numerical simulations have for years found non-zero and radially varying DM velocity anisotropies. Here we employ the method proposed by Hansen & Piffaretti, and developed by Høst et al. to infer the DM velocity anisotropy in the bright galaxy cluster Perseus, to near five times the radii previously obtained. We find the DM velocity anisotropy to be consistent with the results of numerical simulations, however, still with large error bars. At half the virial radius, we find the DM velocity anisotropy to be non-zero at 1.7$\, \sigma$, lending support to the collisionless nature of DM.


2019 ◽  
Vol 15 (S341) ◽  
pp. 271-272
Author(s):  
Yutaka Fujita ◽  
Keiichi Umetsu ◽  
Elena Rasia ◽  
Massimo Meneghetti ◽  
Megan Donahue ◽  
...  

AbstractIn this study, we show that the characteristic radius rs, mass Ms, and the X-ray temperature, TX, of galaxy clusters form a thin plane in the space of (log rs, log Ms, log TX). This tight correlation indicates that the cluster structure including the temperature is affected by the formation time of individual clusters. Numerical simulations show that clusters move along the fundamental plane as they evolve. The plane and the cluster evolution within the plane can be explained by a similarity solution of structure formation. The angle of the plane shows that clusters have not achieved “virial equilibrium”. The details of this study are written in Fujita et al. (2018a,b).


2021 ◽  
Author(s):  
Jinyu Tang ◽  
William R. Rossen

<p>Well-logging data show that geothermal formations typically feature layered heterogeneities. This imposes a challenge in numerical simulations, in particular in the upscaling of geothermal processes. The goal of our study is to develop an approach to (1) simplify the description of heterogeneous geothermal formations and (2) provide an accurate representation of convection/dispersion processes for simulating the up-scaled system.</p><p>In geothermal processes, transverse thermal conduction causes extra spreading of the cooling front: thermal Taylor dispersion. We derive a model from an energy balance for effective thermal diffusivity, α<sub>eff</sub>, to represent this phenomenon in layered media. α<sub>eff</sub>, accounting for transverse heat conduction, is much greater than the longitudinal thermal diffusivity, leading to a remarkably larger effective dispersion. A ratio of times is defined for longitudinal thermal convection and transverse thermal conduction, referred to as transverse thermal-conduction number N<sub>TC</sub>. The value of N<sub>TC</sub> is an indicator of thermal equilibrium in the vertical cross-section. Both N<sub>TC</sub> and α<sub>eff</sub> equations are verified by a match with numerical solutions for convection/conduction in a two-layer system. For N<sub>TC</sub> > 5, the system behaves as a single layer with thermal diffusivity α<sub>eff</sub>.</p><p>When N<sub>TC</sub> > 5, a two-layer system can be combined and represented with α<sub>eff</sub> and average properties of the two layers. We illustrate upscaling approach for simulation of geothermal processes in stratified formations, by grouping layers based on the condition of N<sub>TC</sub> > 5 and the α<sub>eff</sub> model. Specifically, N<sub>TC</sub> is calculated for every adjacent two layers, and the paired layers with a maximum value of N<sub>TC</sub> are grouped first. This procedure repeats on the grouped system until no adjacent layers meet the criterion N<sub>TC</sub> > 5. The upscaled layer properties of the grouped system are used as new inputs in the numerical simulations. The effectiveness of the upscaling approach is validated by a good agreement in numerical solutions for thermal convection/dispersion using original and average layer properties, respectively (Figs. 1 and 2 in the Supplementary Data File). The upscaling approach is applied to well-log data of a geothermal reservoir in Copenhagen featuring many interspersed layers. After upscaling, the formation with 93 layers of thickness 1 – 3 meters is upscaled to 12 layers (Fig. 3 in the Supplementary Data File). The effective thermal diffusivity α<sub>eff</sub> in the flow direction is about a factor of 10 times greater than original thermal diffusivity of the rock. Thus, α<sub>eff</sub> should be used as simulation inputs for representing more accurately geothermal processes in the up-scaled system.</p><p> </p><p> </p>


2008 ◽  
Vol 679 (2) ◽  
pp. 1173-1180 ◽  
Author(s):  
Scott W. Randall ◽  
Maxim Markevitch ◽  
Douglas Clowe ◽  
Anthony H. Gonzalez ◽  
Marusa Bradač

2009 ◽  
Vol 699 (1) ◽  
pp. 348-361 ◽  
Author(s):  
Prateek Sharma ◽  
Benjamin D. G. Chandran ◽  
Eliot Quataert ◽  
Ian J. Parrish

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