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DISKtoHALO SIGNED

From the accretion disk to the cluster halo: the multi-scale physics of black hole feedback

Total Cost €

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EC-Contrib. €

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Partnership

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 DISKtoHALO project word cloud

Explore the words cloud of the DISKtoHALO project. It provides you a very rough idea of what is the project "DISKtoHALO" about.

multiscale    rate    smbh    proceeds    determines    plasma    unclear    data    magnetohydrodynamic    influence    smbhs    smaller    couples    holes    machinery    dictated    incorporating    ineffective    intracluster    medium    relativistic    evolution    accretion    supermassive    partitioning    scales    winds    regulate    cosmic    truly    icm    balance    group    fundamental    time    10    torrent    observations    questions    radiation    black    physics    galaxy    disks    realization    efficiency    interpreting    cgm    baryons    closely    function    thermalization    microphysics    nucleus    groups    explore    environment    massive    active    accreting    models    cluster    redshifts    push    agn    au    it    jets    heating    cooling    epoch    phenomenon    clusters    calibrate    mode    energy    requiring    halo    galaxies    profound    observatories    instabilities    mass    first    firmly    hot    9pc    surroundings    maintenance    microphysical    feedback    theoretical    constructed    disk    proxies    prescriptions    nature    galactic    energetic    appear    releases    almost    times    back    injected    circumgalactic   

Project "DISKtoHALO" data sheet

The following table provides information about the project.

Coordinator		 THE CHANCELLOR MASTERS AND SCHOLARSOF THE UNIVERSITY OF CAMBRIDGE 

Organization address
address: TRINITY LANE THE OLD SCHOOLS
city: CAMBRIDGE
postcode: CB2 1TN
website: www.cam.ac.uk

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.
 Coordinator Country United Kingdom [UK]
 Total cost 2˙489˙918 €
 EC max contribution 2˙489˙918 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2018-ADG
 Funding Scheme ERC-ADG
 Starting year 2019
 Duration (year-month-day) from 2019-10-01   to  2024-09-30

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    THE CHANCELLOR MASTERS AND SCHOLARSOF THE UNIVERSITY OF CAMBRIDGE UK (CAMBRIDGE) coordinator 2˙489˙918.00

Map

 Project objective

It is firmly established that supermassive black holes (SMBHs) have a profound influence on the evolution of galaxies and galaxy groups/clusters. Yet, almost 20 years after this realization, fundamental questions remain. What determines the efficiency with which an active galactic nucleus (AGN) couples to its surroundings? Why does AGN feedback appear to be ineffective in low-mass galaxies? In maintenance-mode feedback, how does the AGN regulate to closely balance cooling? How does the nature of AGN feedback change as we consider higher redshifts and push back to the epoch of the first galaxies? AGN feedback is a truly multi-scale phenomenon. Observations show that AGN have an energetic impact on galactic-, group-, and cluster-halo scales. Yet the efficiency with which an accreting SMBH releases energy, and the partitioning of that energy into radiation, winds, and relativistic jets, is dictated by complex processes in the accretion disk on AU scales, 10^10 times smaller than the halo. Furthermore, especially in massive systems where feedback proceeds via the heating of a hot circumgalactic or intracluster medium (CGM/ICM), the relevant microphysics of the hot baryons is unclear, requiring an understanding of plasma instabilities on 10^-9pc scales. We propose a set of projects that explore the multiscale physics of AGN feedback. Magnetohydrodynamic models of accretion disks will be constructed to study the AGN radiation/winds/jets and calibrate observable proxies of SMBH mass and accretion rate. We will use the machinery of plasma physics to characterize the CGM/ICM microphysics relevant to the thermalization of AGN-injected energy. Finally, we will produce new galaxy-, group- and cluster-scale models incorporating the new microphysical prescriptions and AGN models. Our new theoretical understanding of AGN feedback as a function of halo mass, environment, and cosmic time is essential for interpreting the torrent of data from current and future observatories

 Deliverables

List of deliverables.
Data Management Plan Open Research Data Pilot 2020-04-09 20:18:58

Take a look to the deliverables list in detail:  detailed list of DISKtoHALO deliverables.

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