HOME

TheInfoList



OR:

Chooz () was a short baseline neutrino oscillation experiment in
Chooz Chooz () can denote several things: * Chooz, Ardennes is a French commune ** The Chooz Nuclear Power Plant ** Chooz (experiment) was a physics experiment using the reactor as a neutrino source ** Double Chooz Double Chooz was a short-baseline ne ...
,
France France (), officially the French Republic ( ), is a country primarily located in Western Europe. It also comprises of overseas regions and territories in the Americas and the Atlantic, Pacific and Indian Oceans. Its metropolitan area ...
. Its major result was setting limits on the neutrino oscillation parameters responsible for changing
electron neutrino The electron neutrino () is an elementary particle which has zero electric charge and a spin of . Together with the electron, it forms the first generation of leptons, hence the name electron neutrino. It was first hypothesized by Wolfgang Pauli ...
s into other neutrinos. Specifically, it found that for large δm2 and for maximal mixing. Results were published in 1999. The
Double Chooz Double Chooz was a short-baseline neutrino oscillation experiment in Chooz, France. Its goal was to measure or set a limit on the ''θ''13 mixing angle, a neutrino oscillation parameter responsible for changing electron neutrinos into other neut ...
experiment continues to take data using the same lab space.


Neutrino source

Chooz used neutrinos from two
pressurized water reactor A pressurized water reactor (PWR) is a type of light-water nuclear reactor. PWRs constitute the large majority of the world's nuclear power plants (with notable exceptions being the UK, Japan and Canada). In a PWR, the primary coolant (water) i ...
s, which provide a >99.999% source. The average neutrino energy was approximately 3
MeV In physics, an electronvolt (symbol eV, also written electron-volt and electron volt) is the measure of an amount of kinetic energy gained by a single electron accelerating from rest through an electric potential difference of one volt in vacu ...
, and the detector was roughly 1000 m from the reactor. The intensity was measured using both the heat balance and neutron output of the reactor, and was known to better than 2%. Detailed modeling of the reactor cores was used to predict both the intensity and energy spectrum of the neutrinos as a function of time. Neutrinos were observed via the
inverse beta decay Inverse beta decay, commonly abbreviated to IBD, is a nuclear reaction involving an electron antineutrino scattering off a proton, creating a positron and a neutron. This process is commonly used in the detection of electron antineutrinos in ...
reaction ( + → + ).


Detector

The Chooz detector was underground, with a 300 meter water equivalent overburden to reduce cosmic ray backgrounds. The detector itself was a cylinder 5.5 m in diameter and 5.5 m tall. The detector was composed of three regions. The innermost region (region I) contained 5 tons of scintillator doped with
gadolinium Gadolinium is a chemical element with the symbol Gd and atomic number 64. Gadolinium is a silvery-white metal when oxidation is removed. It is only slightly malleable and is a ductile rare-earth element. Gadolinium reacts with atmospheric oxygen ...
in a Plexiglas container. The gadolinium quickly captured the neutrons produced in the inverse beta decay. The second region (region II) contained 17 tons of undoped scintillator to capture the electromagnetic energy from the inverse beta decay (≈99%) and the photons from the neutron capture in the Gd (>95%). The outer surface of region II contained 192 inward facing
photomultiplier A photomultiplier is a device that converts incident photons into an electrical signal. Kinds of photomultiplier include: * Photomultiplier tube, a vacuum tube converting incident photons into an electric signal. Photomultiplier tubes (PMTs for sh ...
tubes (PMT) held in an opaque plastic structure. The outermost region (region III) contained ninety tons of the same undoped scintillator as region II and vetoed cosmic ray events using 48 PMTs. The Plexiglas layer between regions I and II was clear, to allow scintillation light from region I to be observed by the PMTs in region II. The inner surface of the region II container was painted black to avoid reflections, which would degrade position measurements. The outer surface of the region II container and the inner surface of the region III container were painted white to maximize the veto signals.


Data sample

Chooz collected data for a total of 8210 hours: 3420 hours with neither reactor running, 3250 hours with one reactor running, and 1540 hours with both reactors running. A total of 2991 neutrino candidates were observed during this period, with 287 of the candidates occurring during the reactor off periods. The correlated background was 1.01 events per day, and the uncorrelated background was 0.42 events per day. The neutrino yield was also studied as a function of reactor power, fuel burnup, and for each reactor separately. The energy spectrum of the positrons and the calculated direction of the incoming neutrino were also calculated. All distributions agreed with predictions.


Neutrino oscillation searches

Three analysis techniques were used to search for neutrino oscillations. The most powerful method used a global ''χ''2 fit of seven positron energy bins for each reactor, for a total of fourteen bins. The ''χ''2 was calculated for various (''θ'', ''δm''2) combinations. The full covariance matrix was used to account for correlations among the bins. The ''χ''2 statistic also includes a term for the overall neutrino normalization (with an uncertainty of 2.7%) and a term for the energy calibration (with an uncertainty of 1.1%). The global minimum, with a ''χ''2 probability of 96%, corresponds to , overall neutrino normalization = 1.012, and energy scale = 1.006. The no-oscillation hypothesis is also has a high ''χ''2 probability of 93%, corresponding to an overall neutrino normalization = 1.008 and energy scale = 1.011.


Interpretation of results

The Chooz results place limits on the PMNS matrix element ''U''e32. Two possibilities exist, or . The
solar neutrino problem The solar neutrino problem concerned a large discrepancy between the flux of solar neutrinos as predicted from the Sun's luminosity and as measured directly. The discrepancy was first observed in the mid-1960s and was resolved around 2002. The fl ...
excludes the second inequality, therefore ''U''e32 is restricted to small values. The CHOOZ data also indicate a strong preference for the maximum mixing hypothesis.


Note on naming

The Chooz collaboration is not consistent in its capitalization. The experiment sometimes appears as ''Chooz'' and sometimes as ''CHOOZ''. However, it is not an
acronym An acronym is a word or name formed from the initial components of a longer name or phrase. Acronyms are usually formed from the initial letters of words, as in ''NATO'' (''North Atlantic Treaty Organization''), but sometimes use syllables, as ...
.


References


External links


Chooz's home page
{{Neutrino detectors Reactor neutrino experiments