EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
arXiv:2210.09978 · doi:10.1093/mnras/stad342
Abstract
Recent high-resolution cosmological hydrodynamic simulations run with a variety of codes systematically predict large amounts of entropy in the intra-cluster medium at low redshift, leading to flat entropy profiles and a suppressed cool-core population. This prediction is at odds with X-ray observations of groups and clusters. We use a new implementation of the EAGLE galaxy formation model to investigate the sensitivity of the central entropy and the shape of the profiles to changes in the sub-grid model applied to a suite of zoom-in cosmological simulations of a group of mass and a cluster of mass . Using our reference model, calibrated to match the stellar mass function of field galaxies, we confirm that our simulated groups and clusters contain hot gas with too high entropy in their cores. Additional simulations run without artificial conduction, metal cooling or AGN feedback produce lower entropy levels but still fail to reproduce observed profiles. Conversely, the two objects run without supernova feedback show a significant entropy increase which can be attributed to excessive cooling and star formation. Varying the AGN heating temperature does not greatly affect the profile shape, but only the overall normalisation. Finally, we compared runs with four AGN heating schemes and obtained similar profiles, with the exception of bipolar AGN heating, which produces a higher and more uniform entropy distribution. Our study leaves open the question of whether the entropy core problem in simulations, and particularly the lack of power-law cool-core profiles, arise from incorrect physical assumptions, missing physical processes, or insufficient numerical resolution.
arXiv commentAccepted for publication in MNRAS on 2023 February 06. The code used in the analysis is publicly available on the corresponding author's GitHub repository: https://github.com/edoaltamura/entropy-core-problem
References in corpus (114)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Array Programming with NumPy
- Astropy: A Community Python Package for Astronomy
- The Global Schmidt Law in Star Forming Galaxies
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- Observational Evidence of AGN Feedback
- Simulating Galaxy Formation with the IllustrisTNG Model
- The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
- Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation
- The Co-Evolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe
- Simba: Cosmological Simulations with Black Hole Growth and Feedback
- Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
- Evolution of Buoyant Bubbles in M87
- Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
- On the relation between the Schmidt and Kennicutt-Schmidt star formation laws and its implications for numerical simulations
- Fundamental differences between SPH and grid methods
- A deep Chandra observation of the Perseus cluster: shocks and ripples
- Star formation thresholds and galaxy edges: why and where
- Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters
- Simulating galactic outflows with thermal supernova feedback
- The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology
- Galaxy evolution in groups and clusters: star formation rates, red sequence fractions, and the persistent bimodality
- The Santa Barbara cluster comparison project: a comparison of cosmological hydrodynamics solutions
- The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues
- The Evolution of X-ray Clusters and the Entropy of the Intra Cluster Medium
- Simulating galactic outflows with kinetic supernova feedback
- Cosmological simulations of black hole growth: AGN luminosities and downsizing
- Chaotic cold accretion onto black holes
- Modelling discontinuities and Kelvin-Helmholtz instabilities in SPH
- Towards a realistic population of simulated galaxy groups and clusters
- Time-Dependent Ionization in Radiatively Cooling Gas
- Gas entropy in a representative sample of nearby X-ray galaxy clusters (REXCESS): relationship to gas mass fraction
- Inviscid SPH
- The baseline intracluster entropy profile from gravitational structure formation
- The Structure and Dynamical Evolution of Dark Matter Halos
- The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end
- The case for AGN feedback in galaxy groups
- The impact of angular momentum on black hole accretion rates in simulations of galaxy formation
- Simulating the effect of AGN feedback on the metal enrichment of galaxy clusters
- Revisiting the Cosmic Cooling Crisis
- The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
- A Cosmic UV/X-ray Background Model Update
- The Hydrangea simulations: galaxy formation in and around massive clusters
- The EAGLE simulations of galaxy formation: the importance of the hydrodynamics scheme
- Gas expulsion by quasar-driven winds as a solution to the over-cooling problem in galaxy groups and clusters
- Cool Core Clusters from Cosmological Simulations
- Modified-Entropy Models for the Intracluster Medium
- Cooling, AGN Feedback and Star Formation in Simulated Cool-Core Galaxy Clusters
- How AGN Jets Heat the Intracluster Medium -- Insights from Hydrodynamic Simulations
- What Shapes the Galaxy Mass Function? Exploring the Roles of Supernova-Driven Winds and AGN
- The Effect of Cooling and Preheating on the X-ray Properties of Clusters of Galaxies
- The effect of radiative cooling on the X-ray properties of galaxy clusters
- Cool core cycles: Cold gas and AGN jet feedback in cluster cores
- Non-Equilibirum ionisation and cooling of metal-enriched gas in the presence of a photo-ionisation background
- The FABLE simulations: A feedback model for galaxies, groups and clusters
- Magnetic draping of merging cores and radio bubbles in clusters of galaxies
- On the Origin of Cores in Simulated Galaxy Clusters
- Feedback from Active Galactic Nuclei in Galaxy Groups
- Cosmological Shock Waves in the Large Scale Structure of the Universe: Non-gravitational Effects
- Introducing RomulusC: A Cosmological Simulation of a Galaxy Cluster with Unprecedented Resolution
- Blowing cold flows away: the impact of early AGN activity on the formation of a brightest cluster galaxy progenitor
- The Redshift Evolution of the Mean Temperature, Pressure, and Entropy Profiles in 80 SPT-Selected Galaxy Clusters
- A new way of setting the phases for cosmological multi-scale Gaussian initial conditions
- On viscosity, conduction and sound waves in the intracluster medium
- Second-order Lagrangian perturbation theory initial conditions for resimulations
- The redshift evolution of massive galaxy clusters in the MACSIS simulations
- The Entropy-Driven X-ray Evolution of Galaxy Clusters
- AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
- The XMM Cluster Outskirts Project (X-COP)
- Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields
- Simulating the interaction of jets with the intra-cluster medium
- A census of cool core galaxy clusters in IllustrisTNG
- Hunting for Galaxies and Halos in simulations with VELOCIraptor
- Entropy amplification from energy feedback in simulated galaxy groups and clusters
- Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration
- Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies
- The impact of mergers on relaxed X-ray clusters - III. Effects on compact cool cores
- nIFTy galaxy cluster simulations I: dark matter & non-radiative models
- A Systematic Look at the Effects of Radiative Feedback on Disc Galaxy Formation
- The rapid growth phase of supermassive black holes
- Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations
- Modelling Shock Heating in Cluster Mergers: I. Moving Beyond the Spherical Accretion Model
- The formation of the brightest cluster galaxies in cosmological simulations: the case for AGN feedback
- Rhapsody-G simulations I: the cool cores, hot gas and stellar content of massive galaxy clusters
- AGN Heating in Simulated Cool-Core Clusters
- Two Clusters with Radio-quiet Cooling Cores
- The DIANOGA simulations of galaxy clusters: characterizing star formation in proto-clusters
- Blandford-Znajek jets in galaxy formation simulations: method and implementation
- How AGN feedback and metal cooling shape cluster entropy profiles
- Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback
- nIFTy galaxy cluster simulations II: radiative models
- Black hole evolution: II. Spinning black holes in a supernova-driven turbulent interstellar medium
- The importance of black hole repositioning for galaxy formation simulations
- Simulations of Jet Heating in Galaxy Clusters: Successes and Challenges
- Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relations
- Spin-driven jet feedback in idealised simulations of galaxy groups and clusters
- AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
- Characterizing hydrostatic mass bias with Mock-X
- X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
- Efficient Production of Sound Waves by AGN Jets in the Intracluster Medium
- How baryons can significantly bias cluster count cosmology
- Fountains and storms: The role of AGN and mergers in disrupting the cool-core in the RomulusC simulation
- Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
- The Three Hundred Project: the stellar and gas profiles
- Self-regulated AGN feedback of light jets in cool-core galaxy clusters
- The X-ray Properties of Weak Lensing Selected Galaxy Clusters
- Turbulent magnetic fields in merging clusters: A case study of Abell 2146
- Inconsistencies arising from the coupling of galaxy formation sub-grid models to Pressure-Smoothed Particle Hydrodynamics
- Very Large Array observations of the mini-halo and AGN feedback in the Phoenix cluster
- Projecting SPH Particles in Adaptive Environments
- Exploring the role of cosmological shock waves in the Dianoga simulations of galaxy clusters
- The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
Cited by in corpus (10)
- SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
- The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
- The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
- Star Formation and Chemical Enrichment in Protoclusters
- How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
- CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime
- A large thermal energy reservoir in the nascent intracluster medium at a redshift of 4.3
- Core to Cosmic Edge: SIMBA-C's New Take on Abundance Profiles in the Intragroup Medium at z = 0
- Entropy plateaus can emerge from gas replacement at a characteristic halo mass in simulated groups and clusters of galaxies
- How supermassive black holes shape central entropies in galaxy clusters