Turbulence, plasma instabilities, transport and magnetogenesis in galaxy clusters

Lead Research Organisation: University of Oxford
Department Name: Oxford Physics

Abstract

The clusters of galaxies are the largest structured objects in the Universe. Most of the luminous matter contained in clusters is in the form of ionised gas, or plasma (called the intracluster medium, or ICM). This plasma is believed to be in a turbulent state, i.e., it is moving in a disordered fashion. It is also permeated by tangled magnetic fields, which impart a certain elasticity to the plasma motions and also alter the motion of individual particles. All large scale processes in clusters - such as, for example, the propagation of waves and shocks, formation and movement of 'bubbles' blown by the active galaxies in cluster cores etc. - occur in this turbulent magnetised medium and are profoundly affected by it. This proposal is for an investigation of the fundamental physical properties of the ICM: what kind of turbulent motions and electromagnetic fluctuations exist in it? how is the energy of ICM motions dissipated into heat? how is heat trnasported across clusters? what is the origin and structure of magnetic fields in clusters? All these questions must be faced in order for us to be able to make sense of the rapidly increasing amount of observational evidence (obtained with radiotelescopes and with X-ray satellite observatories) and also to develop correct numerical models of clusters. More broadly, the problem of turbulence, which is at the centre of this research, is an exciting and formidable intellectual challenge, sometimes referred to as the last great unsolvedx problem of classical physics. Intertwined with the problem of magnetogenesis (the origin of cosmic magnetism), it continues to inspire both theoretical physicists and astronomers.

Publications

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Chandran B (2015) INTERMITTENCY AND ALIGNMENT IN STRONG RMHD TURBULENCE in The Astrophysical Journal

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Chen C (2010) INTERPRETING POWER ANISOTROPY MEASUREMENTS IN PLASMA TURBULENCE in The Astrophysical Journal

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Chen C (2012) THREE-DIMENSIONAL STRUCTURE OF SOLAR WIND TURBULENCE in The Astrophysical Journal

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Churazov E (2013) Powering of cool filaments in cluster cores by buoyant bubbles - I. Qualitative model in Monthly Notices of the Royal Astronomical Society

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En (2009) Magnetic turbulence in clusters of galaxies in Revista Mexicana de Astronomia y Astrofisica Conference Series

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Enßlin T (2010) Magnetic turbulence in clusters of galaxies in Proceedings of the International Astronomical Union

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Forest C (2015) The Wisconsin Plasma Astrophysics Laboratory in Journal of Plasma Physics

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Heinemann T (2011) Large-scale magnetic field generation by randomly forced shearing waves. in Physical review letters

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Komarov S (2016) Polarization of thermal bremsstrahlung emission due to electron pressure anisotropy in Monthly Notices of the Royal Astronomical Society

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Komarov S (2016) Thermal conduction in a mirror-unstable plasma in Monthly Notices of the Royal Astronomical Society

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Komarov S (2014) Suppression of local heat flux in a turbulent magnetized intracluster medium in Monthly Notices of the Royal Astronomical Society

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Kunz M (2012) BUOYANCY INSTABILITIES IN A WEAKLY COLLISIONAL INTRACLUSTER MEDIUM in The Astrophysical Journal

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Loureiro N (2009) Turbulent magnetic reconnection in two dimensions in Monthly Notices of the Royal Astronomical Society: Letters

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Loureiro NF (2013) Plasmoid and Kelvin-Helmholtz instabilities in Sweet-Parker current sheets. in Physical review. E, Statistical, nonlinear, and soft matter physics

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Mallet A (2015) Refined critical balance in strong Alfvénic turbulence in Monthly Notices of the Royal Astronomical Society: Letters

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Mallet A (2016) Measures of three-dimensional anisotropy and intermittency in strong Alfvénic turbulence in Monthly Notices of the Royal Astronomical Society

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Meinecke J (2015) Developed turbulence and nonlinear amplification of magnetic fields in laboratory and astrophysical plasmas. in Proceedings of the National Academy of Sciences of the United States of America

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Melville S (2016) Pressure-anisotropy-driven microturbulence and magnetic-field evolution in shearing, collisionless plasma in Monthly Notices of the Royal Astronomical Society

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Mogavero F (2014) Models of magnetic field evolution and effective viscosity in weakly collisional extragalactic plasmas in Monthly Notices of the Royal Astronomical Society

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Oliver M (2017) Magneto-optic probe measurements in low density-supersonic jets in Journal of Instrumentation

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PLUNK G (2010) Two-dimensional gyrokinetic turbulence in Journal of Fluid Mechanics

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Rincon F (2016) Turbulent dynamo in a collisionless plasma. in Proceedings of the National Academy of Sciences of the United States of America

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Rincon F (2015) Non-linear mirror instability in Monthly Notices of the Royal Astronomical Society: Letters

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Samtaney R (2009) Formation of plasmoid chains in magnetic reconnection. in Physical review letters

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Samtaney R. (2012) Plasmoid dynamics in 3D resistive MHD simulations of magnetic reconnection in EGU General Assembly Conference Abstracts

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Sanders JS (2013) Linear structures in the core of the Coma cluster of galaxies. in Science (New York, N.Y.)

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Schekochihin A (2009) ASTROPHYSICAL GYROKINETICS: KINETIC AND FLUID TURBULENT CASCADES IN MAGNETIZED WEAKLY COLLISIONAL PLASMAS in The Astrophysical Journal Supplement Series

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Schekochihin A (2010) Magnetofluid dynamics of magnetized cosmic plasma: firehose and gyrothermal instabilities in Monthly Notices of the Royal Astronomical Society

 
Description The publication list reflects the key findings.
Exploitation Route Some theories and methods that were developed carry over to bordering disciplines and areas of activity, most importantly magnetic fusion research.
Sectors Energy