Opendata, web and dolomites

DISKtoHALO SIGNED

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

Total Cost €

0

EC-Contrib. €

0

Partnership

0

Views

0

 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.

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

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.

Are you the coordinator (or a participant) of this project? Plaese send me more information about the "DISKTOHALO" project.

For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.

Send me an  email (fabio@fabiodisconzi.com) and I put them in your project's page as son as possible.

Thanks. And then put a link of this page into your project's website.

The information about "DISKTOHALO" are provided by the European Opendata Portal: CORDIS opendata.

More projects from the same programme (H2020-EU.1.1.)

NanoPD_P (2020)

High throughput multiplexed trace-analyte screening for diagnostics applications

Read More  

TOROS (2019)

A Theory-Oriented Real-Time Operating System for Temporally Sound Cyber-Physical Systems

Read More  

PROGRESS (2019)

The Enemy of the Good: Towards a Theory of Moral Progress

Read More