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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.

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

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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