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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.

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

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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