subgrid models of active galactic nuclei in clusters of galaxies
description
Transcript of subgrid models of active galactic nuclei in clusters of galaxies
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subgrid modelsof
active galactic nuclei
inclusters of galaxies
Paul Matthew Sutter Paul M. Ricker
Univ. of Illinois at Urbana-Champaign
Frontiers in Computational AstrophysicsLyon, France 10/14/2010
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clusters and cosmology
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why bother?
next-gen surveys will get ~10,000 clusters
significance will be reduced by systematics
must understand cluster astrophysics to constrain these systematics
magnetic fields play large role in cluster physics, but are poorly understood...
DES 500 Megapixel
camera at Blanco 4-meter telescope
5000 square-degree survey
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radio halosAbell 2163
1.4Ghz Radio Contours (GMRT, India) and ROSAT X-ray emission
(Feretti et al. 2001)
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radio mini-halos
(Burns et al. 1992, Sibring 1993)
(Fabian et al. 2000)
Perseus Cluster
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radio relicsAbell 2163
1.4Ghz Radio Contours (GMRT, India) and ROSAT X-ray emission
(Bagchi et al. 2006)
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seeding magnetic fields
seeds via Biermann battery
amplification via stellar or AGN accretion disks
ejection via winds or AGN
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agn
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jet injection
Cattaneo & Teyssier (2007)
jet energy linked to accretion rate
assume entrainment factor
cylindrical feedback region
kinetic, thermal, and mass injection
jets point along axis
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magnetic field injection
Li et al. (2006)
appropriate for jets and bubbles
poloidal and toroidal components
assumes underlying dynamo-like system
free to choose scale radius, magnetic field strength
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FLASH
oct-tree adaptive mesh refinement
Gravity: N-body particle-mesh multigrid+pFFT
Hydro: PPM MHD: Constrained-
Transport SM sutherland & dopita
radiative cooling fast on-the-fly halo finding scales well to >200,000
processors
(Fryxell et al. 2000)
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test setup
mock 1014 Mʘ halo fixed NFW potential
(rs = 165 kpc) rcool core = 40kpc tcool ~ 6 Gyr Mbh = 107 Mʘ
~0.5 kpc resolution
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injected magnetic field
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accretion rate
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magnetized cluster
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preliminary conclusions
magnetizing jets severely lowers accretion rates
magnetic energy much less than Liu et al. (2007), Xu et al. (2008)can weakly magnetize entire cluster with jets, strong fields in cores (mini-halos?)
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outro
clusters offer unique window on universe
must understand astrophysics to understand cosmology
magnetic fields impact cluster physics
simulations can help us understand magnetic fields