Recent Progress in Modeling the Macro- and Micro-Physics of Radio Jet Feedback in Galaxy Clusters

Radio jets and the lobes they inflate are common in cool-core clusters and are known to play a critical role in regulating the heating and cooling of the intracluster medium (ICM). This is an inherently multi-scale problem, and much effort has been made to understand the processes governing the infl...

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Published inGalaxies Vol. 11; no. 3; p. 73
Main Authors Bourne, Martin A., Yang, Hsiang-Yi Karen
Format Journal Article
LanguageEnglish
Published Basel MDPI AG 01.06.2023
Subjects
active galactic nuclei
Analysis
Astrophysics
Cosmic ray showers
Cosmic rays
Environmental impact
Feedback
Galactic clusters
Galaxies
galaxy clusters
Heating and cooling
Inflation (Finance)
Kao Tsu, Emperor of China
Large scale structure of the universe
Lobes
Magnetic effects
Magnetic fields
Mathematical models
Microphysics
Numerical analysis
numerical modeling
Numerical simulations
Physics
Plasma physics
Power
Questions
Radiation
radio jets
Radio jets (astronomy)
Simulation
simulation techniques
Star & galaxy formation
Stars & galaxies
United Kingdom
Viscosity
X-rays
United Kingdom
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Abstract Radio jets and the lobes they inflate are common in cool-core clusters and are known to play a critical role in regulating the heating and cooling of the intracluster medium (ICM). This is an inherently multi-scale problem, and much effort has been made to understand the processes governing the inflation of lobes and their impact on the cluster, as well as the impact of the environment on the jet–ICM interaction, on both macro- and microphysical scales. The developments of new numerical techniques and improving computational resources have seen simulations of jet feedback in galaxy clusters become ever more sophisticated. This ranges from modeling ICM plasma physics processes such as the effects of magnetic fields, cosmic rays, and viscosity to including jet feedback in cosmologically evolved cluster environments in which the ICM thermal and dynamic properties are shaped by large-scale structure formation. In this review, we discuss the progress made over the last ∼decade in capturing both the macro- and microphysical processes in numerical simulations, highlighting both the current state of the field, as well as the open questions and potential ways in which these questions can be addressed in the future.
AbstractList Radio jets and the lobes they inflate are common in cool-core clusters and are known to play a critical role in regulating the heating and cooling of the intracluster medium (ICM). This is an inherently multi-scale problem, and much effort has been made to understand the processes governing the inflation of lobes and their impact on the cluster, as well as the impact of the environment on the jet–ICM interaction, on both macro- and microphysical scales. The developments of new numerical techniques and improving computational resources have seen simulations of jet feedback in galaxy clusters become ever more sophisticated. This ranges from modeling ICM plasma physics processes such as the effects of magnetic fields, cosmic rays, and viscosity to including jet feedback in cosmologically evolved cluster environments in which the ICM thermal and dynamic properties are shaped by large-scale structure formation. In this review, we discuss the progress made over the last ∼decade in capturing both the macro- and microphysical processes in numerical simulations, highlighting both the current state of the field, as well as the open questions and potential ways in which these questions can be addressed in the future.
Audience Academic
Author Bourne, Martin A.
Yang, Hsiang-Yi Karen
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  fullname: Bourne, Martin A.
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  givenname: Hsiang-Yi Karen
  orcidid: 0000-0003-3269-4660
  surname: Yang
  fullname: Yang, Hsiang-Yi Karen
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RelatedPersons Kao Tsu, Emperor of China
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SubjectTerms active galactic nuclei
Analysis
Astrophysics
Cosmic ray showers
Cosmic rays
Environmental impact
Feedback
Galactic clusters
Galaxies
galaxy clusters
Heating and cooling
Inflation (Finance)
Kao Tsu, Emperor of China
Large scale structure of the universe
Lobes
Magnetic effects
Magnetic fields
Mathematical models
Microphysics
Numerical analysis
numerical modeling
Numerical simulations
Physics
Plasma physics
Power
Questions
Radiation
radio jets
Radio jets (astronomy)
Simulation
simulation techniques
Star & galaxy formation
Stars & galaxies
United Kingdom
Viscosity
X-rays
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Title Recent Progress in Modeling the Macro- and Micro-Physics of Radio Jet Feedback in Galaxy Clusters
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