Coordinatore | ISTITUTO NAZIONALE DI FISICA NUCLEARE
Spiacenti, non ci sono informazioni su questo coordinatore. Contattare Fabio per maggiori infomrazioni, grazie. |
Nazionalità Coordinatore | Italy [IT] |
Totale costo | 1˙176˙758 € |
EC contributo | 1˙176˙758 € |
Programma | FP7-IDEAS-ERC
Specific programme: "Ideas" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013) |
Code Call | ERC-2013-StG |
Funding Scheme | ERC-SG |
Anno di inizio | 2014 |
Periodo (anno-mese-giorno) | 2014-03-01 - 2018-02-28 |
# | ||||
---|---|---|---|---|
1 |
UNIVERSITA DEGLI STUDI DI ROMA LA SAPIENZA
Organization address
address: Piazzale Aldo Moro 5 contact info |
IT (ROMA) | beneficiary | 419˙960.00 |
2 |
CONSIGLIO NAZIONALE DELLE RICERCHE
Organization address
address: Piazzale Aldo Moro 7 contact info |
IT (ROMA) | beneficiary | 159˙720.00 |
3 |
ISTITUTO NAZIONALE DI FISICA NUCLEARE
Organization address
address: Via Enrico Fermi 40 contact info |
IT (FRASCATI) | hostInstitution | 597˙078.40 |
4 |
ISTITUTO NAZIONALE DI FISICA NUCLEARE
Organization address
address: Via Enrico Fermi 40 contact info |
IT (FRASCATI) | hostInstitution | 597˙078.40 |
Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.
'In the comprehension of fundamental laws of nature, particle physics is now facing two important questions: 1) What is the nature of the neutrino, is it a standard (Dirac) particle or a Majorana particle? The nature of the neutrino plays a crucial role in the global framework of particle interactions and in cosmology. The only practicable way to answer this question is to search for a nuclear process called 'neutrinoless double beta decay' (0nuDBD). 2) What is the so called 'dark matter' made of? Astrophysical observations suggest that the largest part of the mass of the Universe is composed by a form of matter other than atoms and known matter constituents. We still do not know what dark matter is made of because its rate of interaction with ordinary matter is really low, thus making the direct experimental detection extremely difficult. Both 0nuDBD and dark matter interactions are rare processes and can be detected using the same experimental technique. Bolometers are promising devices and their combination with light detectors provides the identification of interacting particles, a powerful tool to reduce the background. 

The goal of CALDER is to realize a new type of light detectors to improve the upcoming generation of bolometric experiments. The detectors will be designed to feature unprecedented energy resolution and reliability, to ensure an almost complete particle identification. In case of success, CUORE, a 0nuDBD experiment in construction, would gain in sensitivity by up to a factor 6. LUCIFER, a 0nuDBD experiment already implementing the light detection, could be sensitive also to dark matter interactions, thus increasing its research potential. The light detectors will be based on Kinetic Inductance Detectors (KIDs), a new technology that proved its potential in astrophysical applications but that is still new in the field of particle physics and rare event searches.'
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