Do Neutrinos have Mass?
Posted by lahar9jhadav on November 10, 2011
First result from a new generation of reactor neutrino experiments
Physicists of the Double Chooz experiment detected a short-range disappearance of electron antineutrinos. They presented this result on Wednesday 9 November 2011 at the LowNu conference in Seoul, Korea. It helps determine the so-far unknown third neutrino mixing angle which is a fundamental property with important consequences for particle and astro-particle physics. The Double Chooz experiment is looking for neutrinos produced in the nearby nuclear power plant. A measurement of this third angle would complete our picture of neutrino oscillations as reported by other experiments and will open new perspectives in understanding why we find matter and no antimatter in our today’s Universe.
Neutrinos are the most common particles existing in the Universe, but they are the least visible. They exist in three kinds called “flavours” and they have been known since the late 90’s for their special ability to transform from one type into another. This phenomenon is called neutrino oscillation and it implies that neutrinos do have a mass. Neutrino oscillations are currently an intensive field of research with several experiments aiming at a full description of the mechanism.
Neutrinos are produced in various ways such as by fusion processes inside the Sun and by cosmic rays bombarding the atmosphere. The Double Chooz experiment is dedicated to measure neutrino oscillations with unprecedented precision, by looking at anti-neutrinos being produced in the nearby nuclear reactor at Chooz in the French Ardennes. Double Chooz started taking data six months ago. At the 2011 LowNu conference in Korea the collaboration just announced its first results, reporting new data consistent with short-range oscillations. This result is based on the observation of the “disappearance” of (anti-)neutrinos in the expected flux observed from the nuclear reactor.
The three different flavours of neutrinos are related to their charged lepton counterparts: electron, muon and tau. Oscillations depend on three mixing parameters, of which two are large and have been measured before. The third mixing angle called θ13 (theta13) was not well measured up to now and restricted by an upper limit. The Double Chooz collaboration, by measuring the “disappearance” of electron antineutrinos, presents hints for oscillation also involving the third angle with the following value: sin2(2θ13) = 0.085 ± 0.051. The probability given by preliminary results that there is no oscillation is only 7.9%.
The measurement of the last mixing angle “θ13” (theta13) is crucial for future experiments aimed at measuring the difference between neutrino and anti-neutrino oscillations (leptonic CP violation). Furthermore, it relates indirectly to the origin of the asymmetry between matter and antimatter in the Universe.
“The third mixing angle is currently the missing link of neutrino physics. Measuring it precisely is the key to open the door to new physics beyond the standard model of particle physics and we are now very close to it” said Herve de Kerret from CNRS in France, and spokesman of the Double Chooz collaboration.
In June 2011, first hints of oscillation of neutrino muon neutrinos to neutrino electron neutrinos, involving this third angle, have been reported by accelerator experiments. The Double Chooz collaboration, by measuring the “disappearance” of electron antineutrinos, presents complementary and important evidence of oscillation also involving the third angle.
Double Chooz uses currently a detector located at a distance of about 1000 m from the reactor cores. The precision of the measurement will further increase over time and after the start of operation in 2012, of a second or “near” detector located at a distance of 400 m from the reactor. At these distances, no significant transformation into another neutrino species is expected. But by combining the results from both detectors, sin2(2θ13) can be determined with even higher precision.
The detector target is composed of 10m3 of liquid scintillator developed specifically for this experiment. The scintillator is doped with gadolinium in order to tag neutrons from inverse beta decays induced by the reactor anti-neutrinos. The target is surrounded by layers of other liquids protecting against other particles and environmental radioactivity. The target is observed by 390 immersed photomultipliers, converting the interactions into electronic signals. These signals are processed in a data acquisition system, which is ready to take data over the next five years. The new detectors will ensure that neutrino physics will stay one of the most fruitful areas of particle physics, as it has been for the past 50 years.
The Double Chooz collaboration is composed of universities and research institutes from Brazil, England, France, Germany, Japan, Russia, Spain and the USA.
Double Chooz website: http://www.doublechooz.org
and they did it again….
18 November 2011
The team which found that neutrinos may travel faster than light has carried out an improved version of their experiment – and confirmed the result.
If confirmed by other experiments, the find could undermine one of the basic principles of modern physics.
Critics of the first report in September had said that the long bunches of neutrinos (tiny particles) used could introduce an error into the test.
The new work used much shorter bunches.
It has been posted to the Arxiv repositoryand submitted to the Journal of High Energy Physics, but has not yet been reviewed by the scientific community.
The experiments have been carried out by the Opera collaboration – short for Oscillation Project with Emulsion (T)racking Apparatus.
It hinges on sending bunches of neutrinos created at the Cern facility (actually produced as decays within a long bunch of protons produced at Cern) through 730km (454 miles) of rock to a giant detector at the INFN-Gran Sasso laboratory in Italy.
The initial series of experiments, comprising 15,000 separate measurements spread out over three years, found that the neutrinos arrived 60 billionths of a second faster than light would have, travelling unimpeded over the same distance.
The idea that nothing can exceed the speed of light in a vacuum forms a cornerstone in physics – first laid out by James Clerk Maxwell and later incorporated into Albert Einstein’s theory of special relativity.
Timing is everything
Initial analysis of the work by the wider scientific community argued that the relatively long-lasting bunches of neutrinos could introduce a significant error into the measurement.
Those bunches lasted 10 millionths of a second – 160 times longer than the discrepancy the team initially reported in the neutrinos’ travel time.
To address that, scientists at Cern adjusted the way in which the proton beams were produced, resulting in bunches just three billionths of a second long.
When the Opera team ran the improved experiment 20 times, they found almost exactly the same result.
“This is reinforcing the previous finding and ruling out some possible systematic errors which could have in principle been affecting it,” said Antonio Ereditato of the Opera collaboration.
“We didn’t think they were, and now we have the proof,” he told BBC News. “This is reassuring that it’s not the end of the story.”
The first announcement of evidently faster-than-light neutrinos caused a stir worldwide; the Opera collaboration is very aware of its implications if eventually proved correct.
The error in the length of the bunches, however, is just the largest among several potential sources of uncertainty in the measurement, which must all now be addressed in turn; these mostly centre on the precise departure and arrival times of the bunches.
“So far no arguments have been put forward that rule out our effect,” Dr Ereditato said.
“This additional test we made is confirming our original finding, but still we have to be very prudent, still we have to look forward to independent confirmation. But this is a positive result.”
That confirmation may be much longer in coming, as only a few facilities worldwide have the detectors needed to catch the notoriously flighty neutrinos – which interact with matter so rarely as to have earned the nickname “ghost particles”.
Next year, teams working on two other experiments at Gran Sasso experiments – Borexino and Icarus – will begin independent cross-checks of Opera’s results.
The US Minos experiment and Japan’s T2K experiment will also test the observations. It is likely to be several months before they report back.