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INITIUM SIGNED

an Innovative Negative Ion TIme projection chamber for Underground dark Matter searches

Total Cost €

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EC-Contrib. €

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Partnership

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 INITIUM project word cloud

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

optical    galactic    put    neutrinos    experiment    fiducialization    mature    pis    chamber    sasso    m3    coherent    techniques    wimp    versatility    space    compelling    generating    recoil    mass    cmos    am    tpc    precisely    scattering    environmental    cygnus    ion    cameras    nucleon    superior    material    international    active    innovative    gaseous    operation    neutron    dark    pattern    searches    nowadays    cm2    directional    underground    lngs    physics    todays    spokespersons    coupling    laboratori    detector    negative    gran    unexplored    days    thanks    electron    pmts    discrimination    projection    detection    region    first    energies    rare    spin    constraints    independent    neutrino    detectors    thermal    time    consequently    capability    fundamental    sensitivity    gev    events    gathered    boost    42    amplification    floor    readout    context    flux    fast    remarkable    43    believe    simultaneously    tpcs    dm    scalability    multipliers    initium    hypothesis    location    scatter    nazionali    gas    supplying    proof    del    ton    micro    observatory   

Project "INITIUM" data sheet

The following table provides information about the project.

Coordinator
GRAN SASSO SCIENCE INSTITUTE 

Organization address
address: VIA FRANCESCO CRISPI 7
city: L'AQUILA
postcode: 67100
website: n.a.

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 Italy [IT]
 Total cost 1˙995˙719 €
 EC max contribution 1˙995˙719 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2018-COG
 Funding Scheme ERC-COG
 Starting year 2019
 Duration (year-month-day) from 2019-03-01   to  2024-02-29

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    GRAN SASSO SCIENCE INSTITUTE IT (L'AQUILA) coordinator 1˙109˙705.00
2    ISTITUTO NAZIONALE DI FISICA NUCLEARE IT (FRASCATI) participant 886˙014.00

Map

 Project objective

INITIUM: an Innovative Negative Ion TIme projection chamber for Underground dark Matter searches. INITIUM goal is to boost the advancement of gaseous Time Projection Chamber detectors in the Dark Matter (DM) searches field, one of the most compelling issues of todays fundamental physics. I believe this approach to be superior because of its active neutron/electron discrimination, directional and fiducialization capability down to low energies and versatility in terms of target material. Thanks to recent advances in Micro Pattern Gas Detectors amplification and improved readout techniques, TPCs are nowadays mature detectors to aim at developing a ton-scale experiment. INITIUM focuses on the development and operation of the first 1 m3 Negative Ion TPC with Gas Electron Multipliers amplification and optical readout with CMOS-based cameras and PMTs for directional DM searches at Laboratori Nazionali del Gran Sasso (LNGS). INITIUM will put new significant constraints in a DM WIMP-nucleon scattering parameter space still unexplored to these days, with a remarkable sensitivity down to 10-42-10-43 cm2 for Spin Independent coupling in the 1-10 GeV WIMP mass region. As a by-product, INITIUM will also precisely and simultaneously measure environmental fast and thermal neutron flux at LNGS, supplying crucial information for any present and future experiment in this location. Consequently, I will demonstrate the proof-of-principle and scalability of INITIUM approach towards the development of a ton-scale detector in the context of CYGNUS, an international collaboration (of which I am one of the Spokespersons and PIs) recently gathered together with the aim to establish a Galactic Directional Recoil Observatory, that can test the DM hypothesis beyond the Neutrino Floor and measure the coherent scatter of galactic neutrinos, generating a significant long-term impact on detection techniques for rare events searches.

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