01.05.2013 Views

Etudes des proprietes des neutrinos dans les contextes ...

Etudes des proprietes des neutrinos dans les contextes ...

Etudes des proprietes des neutrinos dans les contextes ...

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

tel-00450051, version 1 - 25 Jan 2010<br />

Noνa<br />

Intended to be the successor to MINOS, NOνA will consist of two detectors, one<br />

at Fermilab (the near detector), and one in northern Minnesota (the far detector).<br />

Neutrinos from NuMI will pass through 810 km of Earth to reach the far detector.<br />

NOνA’s main goal is to observe the oscillation of muon to electron <strong>neutrinos</strong>. If a<br />

non-zero value of θ13 is resolvable by the experiment, it will be possible to obtain<br />

measurements of δ and the mass ordering by also observing the process νµ → νe.<br />

2.5.2 Future long-term experiments<br />

Among the future long-term projects are the Megaton detector experiments and<br />

the experiments <strong>des</strong>igned to measure the hardly reachable CP-violating phase δ.<br />

The Megaton detectors<br />

A series of experimental and theoretical studies are being conducted to assess the<br />

astro particle physics potential of future large scale particle detectors as the next<br />

generation underground observatories [18]. Three type of detection techniques<br />

have been proposed all based on the use of large mass of liquid as active media:<br />

the liquid argon (like in GLACIER), the liquid scintillator (LENA) and the water<br />

Cherenkov (MEMPHYS [46], Hyper Kamiokande, UNO). The purpose for such<br />

massive detectors, is multidisciplinary and may answer to the still remaining proton<br />

decay question. Moreover, their potentiality is enormous in neutrino physics,<br />

and more generally in the astro-particle field. It could improve the sensitivity<br />

to known neutrino parameters, investigate the solar and atmospheric neutrino<br />

more deeply, look for geo<strong>neutrinos</strong>, give tremendous information if a supernova<br />

explosion occur, and even yield information about relic neutrino fluxes. Last but<br />

not least, it would allow the exploration of a very small θ13 and the CP-violation<br />

in the leptonic sector, if used in conjunction with future long-term neutrino accelerator<br />

facilities.<br />

1. Water Cherenkov.<br />

As the cheapest available (active) target material, water is the only liquid<br />

that is realistic for extremely large detectors, up to several hundreds or 1<br />

thousand of kton. Water Cherenkov detectors have sufficiently good resolution<br />

in energy, position. The technology is well proven, as previously used<br />

e.g. in Kamiokande and Super-Kamiokande experiments.<br />

2. Liquid scintillator.<br />

Experiments using a liquid scintillator as active target provide high-energy<br />

and angle resolution and offer low-energy threshold. They are particularly<br />

attractive for low energy particle detection, as for example, supernoae, solar<br />

<strong>neutrinos</strong> and geo-<strong>neutrinos</strong>. Also liquid scintillator detectors exploits a well<br />

46

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!