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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.

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

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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