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ClusterWeb SIGNED

Unravelling the physics of particle acceleration and feedback in galaxy clusters and the cosmic web

Total Cost €

0

EC-Contrib. €

0

Partnership

0

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 ClusterWeb project word cloud

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

intergalactic    magnetic    heat    window    rays    unknown    enormous    obtain    medium    feedback    sensitivity    speed    fossil    reside    sequence    nature    scales    accelerate    poorly    giant    construct    elusive    images    physics    extreme    size    frequency    breakthroughs    energies    cosmic    generating    nbsp    telescopes    ionosphere    understand    grow    accelerators    content    correct    total    emitting       turbulence    dilute    plasmas    heated       episodes    earth    universe    galaxies    survey    particles    mass    acceleration    budget    emission    combined    shocks    carry    time    evolution    waves    distorting    arrays    origin    unravel    mergers    epoch    big    associated    energy    mpc    cluster    web    structures    ray    phased    baryons    input    shock    radio    studies    filaments    particle    galaxy    agn    gains    sources    resolution    warm    clusters    plasma    accretion    hot    deepest    quantify    measurements    producing    synchrotron    first    constraints    opening    accelerated    diffuse   

Project "ClusterWeb" data sheet

The following table provides information about the project.

Coordinator
UNIVERSITEIT LEIDEN 

Organization address
address: RAPENBURG 70
city: LEIDEN
postcode: 2311 EZ
website: www.universiteitleiden.nl

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 Netherlands [NL]
 Total cost 1˙487˙755 €
 EC max contribution 1˙487˙755 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2018-STG
 Funding Scheme ERC-STG
 Starting year 2019
 Duration (year-month-day) from 2019-09-01   to  2024-08-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITEIT LEIDEN NL (LEIDEN) coordinator 1˙487˙755.00

Map

 Project objective

We will unravel the origin of cosmic magnetic fields, the physics of particle acceleration in dilute plasmas, and the nature of AGN feedback with state-of-the-art radio telescopes. With the enormous gains in sensitivity, survey speed, and resolution of these telescopes – combined with recent breakthroughs that correct for phased-arrays and the Earth’s distorting ionosphere – we can now take the next big step in this field.

Cosmic web filaments and galaxy clusters are the Universe’s largest structures. Clusters grow by a sequence of mergers, generating shock waves and turbulence which heat the cluster plasma. In merging clusters, cosmic rays are accelerated to extreme energies, producing Mpc-size diffuse synchrotron emitting sources. However, these acceleration processes are still poorly understood. Clusters are also heated by AGN feedback from radio galaxies, but the total energy input by feedback and its evolution over cosmic time are unknown. We will construct the largest low-frequency sample of galaxy clusters to (1) establish how particles are accelerated in cluster plasmas, (2) quantify how the cosmic ray content scales with cluster mass, (3) determine the importance of AGN fossil plasma in the acceleration processes, (4) characterize current and past episodes of AGN feedback, and (5) determine the evolution of feedback up to the epoch of cluster formation (z=1-2). These results will be essential to understand cluster formation and its associated energy budget.

As in clusters, cosmic web accretion shocks should also accelerate particles producing radio emission. Based on the deepest low-frequency images ever produced, we will (5) carry out the first studies of these giant accelerators, opening up a new window on the elusive warm-hot intergalactic medium, where many of the cosmic baryons reside. Even more important, (6) we aim to obtain measurements of the intergalactic magnetic field, providing key constraints on the origin of our Universe’s magnetic fields.

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

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lastchecktime (2021-04-22 3:09:59) correctly updated