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Welcome to CPH Theory Siteبه سایت نظریه سی پی اچ خوش آمدید

 

   

C reative

      Particle

           Higgs

  CPH Theory is based  on  Generalized light velocity from energy  into mass.

 

CPH Theory in Journals

   

 

Neutrinos and the Speed of Light — A Primer on the CERN Study

 

 

 


Neutrinos and the Speed of Light — A Primer on the CERN Study

 

 

 

Cross section of the CNGS experiment through the Earth. (Image: CERN)

 

 

 

Recently, a group of physicists have been working to measure the neutrinos generated from a particle accelerator at CERN. This group discovered neutrinos arriving faster than would have been expected and they appear to be traveling faster than the speed of light itself, but they draw no definitive conclusions. This has been widely reported as being the end of Relativity, but this is not the case at all. Let’s take a look at what is going on in the experiment and what was reported in the journal article.

First, it might help the reader to gain an understanding of the neutrino. Neutrinos are interesting little neutral particles that have almost zero mass. Due to their nature, they can pass through matter without being absorbed. There are three known types of neutrinos: the electron neutrino, the muon neutrino, and the tau neutrino. The experiment in the journal article is referred to as CERN neutrinos to Gran Sasso, or CNGS. The CNGS team is searching for a phenomenon known as neutrino oscillation where muon neutrinos may change into tau neutrinos. A secondary goal of the experiment is to measure neutrino velocity to a great accuracy.

In the experiment, neutrinos are generated at the Super Proton Synchrotron (SPS) particle accelerator at the CERN LHC complex in Geneva and further accelerated down a 1 km beam line toward the Gran Sasso National Laboratory in Italy. At Gran Sasso, a detector instrument called OPERA measures the neutrinos. The distance from CERN to Gran Sasso is 732 km straight through the Earth, traveling up to 11.4 km below the Earth’s surface. Remember, neutrinos don’t interact with matter so the Earth is invisible to the tiny particles.

The distance between the two systems is known to within 20 cm. Time is also measured with extreme precision utilizing GPS timing signals and a cesium atomic clock. The GPS used in timing also allows the team to track any small movements in the Earth itself. This even allowed consideration of the effect of the L’Aquila Earthquake that moved the OPERA detector 7 cm. Due to the nature of the experiment, the time is not calculated with a simple, stopwatch style, start to finish measurement. It instead relies on measurements and comparisons of probability distribution functions at the source and the detector. In other words, there is a lot of math involved. In addition to understanding the timing and position variations in the experiment, the physicists also took into account many other variables, such as day versus night and seasonal changes. The sensitivity of this experiment is roughly an order of magnitude better than previous experiments.

The speed of neutrinos is measured and compared to the speed of light by subtracting the expected time for light to travel the distance from the time for the neutrinos to travel the same distance. One would normally expect this to be zero for neutrinos traveling at the speed of light or negative for any value below the speed of light. The case presented in the article shows a positive value of 60.7 nanoseconds with statistical and systematic errors providing not nearly enough potential difference to account for the positive value. This value has six-sigma significance. This is, obviously, a stunning finding.

The final paragraph is what appears to be overlooked all too often in the reporting on this finding:

Despite the large significance of the measurement reported here and the stability of the analysis, the potential great impact of the results motivates the continuation of our studies in order to investigate possible still unknown systematic effects that could explain the observed anomaly. We deliberately do not attempt any theoretical or phenomenological interpretation of the results.

This is an important paragraph. This is the group of physicists, together, stating that they don’t know how they came to a result that shows neutrinos apparently exceeding the speed of light. They are not drawing any conclusions in this article and are simply providing the finding and the methods used to obtain the finding. They are trying to find where there could be errors in their measurements. They do not claim that the neutrinos are actually exceeding the speed of light, only that the measurements to date show something unexpected. They are reaching out to the high-energy physics community to improve the experiment and data analysis. They are not looking to fundamentally change physics but to ensure that they are producing sound data. We may find that nothing comes of this. We may find that there is an effect known in physics that accounts for the difference. We may find that neutrinos are capable of moving slightly faster than the speed of light. It is simply too early to make definitive, wide-reaching conclusions.

The conclusion that can be drawn from this article is that a group of experimenters found an unexpected result using some of the most amazing and precise instruments and techniques ever created. No matter what is found to be the actual cause of this 60.7 nanosecond variation, the conclusion you can draw is that it is an amazing time in history where such measurements can be made and an exciting time to be a practitioner or admirer of science. Imagine the findings that will be made by the next couple generations of scientists who are sitting in elementary classrooms right now and just learning that a rainbow is the spectrum of sunlight. Einstein wouldn’t be disappointed by these findings; he would be intrigued and proud to see the legacy of great science continuing forward.

Source: WIRED

OPERA experiment reports anomaly in flight time of neutrinos from CERN to Gran Sasso

 

23.09.2011

UPDATE 18 November 2011

Following the OPERA collaboration's presentation at CERN on 23 September, inviting scrutiny of their neutrino time-of-flight measurement from the broader particle physics community, the collaboration has rechecked many aspects of its analysis and taken into account valuable suggestions from a wide range of sources. One key test was to repeat the measurement with very short beam pulses from CERN. This allowed the extraction time of the protons, that ultimately lead to the neutrino beam, to be measured more precisely.

The beam sent from CERN consisted of pulses three nanoseconds long separated by up to 524 nanoseconds. Some 20 clean neutrino events were measured at the Gran Sasso Laboratory, and precisely associated with the pulse leaving CERN. This test confirms the accuracy of OPERA's timing measurement, ruling out one potential source of systematic error. The new measurements do not change the initial conclusion. Nevertheless, the observed anomaly in the neutrinos' time of flight from CERN to Gran Sasso still needs further scrutiny and independent measurement before it can be refuted or confirmed.

On 17 November, the collaboration submitted a paper on this measurement to the peer reviewed Journal of High Energy Physics (JHEP). This paper is also available on the Inspire website.

Geneva, 23 September 2011. The OPERA1 experiment, which observes a neutrino beam from CERN2 730 km away at Italy’s INFN Gran Sasso Laboratory, will present new results in a seminar at CERN this afternoon at 16:00 CEST. The seminar will be webcast at http://webcast.cern.ch. Journalists wishing to ask questions may do so via twitter using the hash tag #nuquestions, or via the usual CERN press office channels.

 

The OPERA result is based on the observation of over 15000 neutrino events measured at Gran Sasso, and appears to indicate that the neutrinos travel at a velocity 20 parts per million above the speed of light, nature’s cosmic speed limit. Given the potential far-reaching consequences of such a result, independent measurements are needed before the effect can either be refuted or firmly established. This is why the OPERA collaboration has decided to open the result to broader scrutiny. The collaboration’s result is available on the preprint server arxiv.org: http://arxiv.org/abs/1109.4897.

The OPERA measurement is at odds with well-established laws of nature, though science frequently progresses by overthrowing the established paradigms. For this reason, many searches have been made for deviations from Einstein’s theory of relativity, so far not finding any such evidence. The strong constraints arising from these observations makes an interpretation of the OPERA measurement in terms of modification of Einstein’s theory unlikely, and give further strong reason to seek new independent measurements.

 

" This result comes as a complete surprise,” said OPERA spokesperson, Antonio Ereditato of the University of Bern. “After many months of studies and cross checks we have not found any instrumental effect that could explain the result of the measurement. While OPERA researchers will continue their studies, we are also looking forward to independent measurements to fully assess the nature of this observation.” 

"When an experiment finds an apparently unbelievable result and can find no artefact of the measurement to account for it, it’s normal procedure to invite broader scrutiny, and this is exactly what the OPERA collaboration is doing, it’s good scientific practice,” said CERN Research Director Sergio Bertolucci. “If this measurement is confirmed, it might change our view of physics, but we need to be sure that there are no other, more mundane, explanations. That will require independent measurements.”

 

In order to perform this study, the OPERA Collaboration teamed up with experts in metrology from CERN and other institutions to perform a series of high precision measurements of the distance between the source and the detector, and of the neutrinos’ time of flight. The distance between the origin of the neutrino beam and OPERA was measured with an uncertainty of 20 cm over the 730 km travel path. The neutrinos’ time of flight was determined with an accuracy of less than 10 nanoseconds by using sophisticated instruments including advanced GPS systems and atomic clocks. The time response of all elements of the CNGS beam line and of the OPERA detector has also been measured with great precision.

 

"We have established synchronization between CERN and Gran Sasso that gives us nanosecond accuracy, and we’ve measured the distance between the two sites to 20 centimetres,” said Dario Autiero, the CNRS researcher who will give this afternoon’s seminar. “Although our measurements have low systematic uncertainty and high statistical accuracy, and we place great confidence in our results, we’re looking forward to comparing them with those from other experiments."

 

" The potential impact on science is too large to draw immediate conclusions or attempt physics interpretations. My first reaction is that the neutrino is still surprising us with its mysteries.” said Ereditato. “Today’s seminar is intended to invite scrutiny from the broader particle physics community.”

The OPERA experiment was inaugurated in 2006, with the main goal of studying the rare transformation (oscillation) of muon neutrinos into tau neutrinos. One first such event was observed in 2010, proving the unique ability of the experiment in the detection of the elusive signal of tau neutrinos.

Further information:

OPERA website

Quantum diaries blog post: Elementary, my dear neutrino...

Photos from the OPERA collaboration:

http://www.infn.it/comunicazione/scambio/

CNRS

Photos of the seminar on OPERA Results

Contact:

CERN Press Office, press.office@cern.ch
+41 22 767 34 32
+41 22 767 21 41

Follow CERN at:

www.cern.ch

http://twitter.com/cern/

http://www.youtube.com/user/CERNTV

http://www.quantumdiaries.org/

 

1. OPERA has been designed and is being conducted by a team of researchers from Belgium, Croatia, France, Germany, Israel, Italy, Japan, Korea, Russia, Switzerland and Turkey. The experiment constitutes a complex scientific enterprise that has been realised thanks to the skill of a large number of scientists, engineers, technicians and students, and with the strong commitment of the various actors of the project. In particular we mention the LNGS/INFN and CERN laboratories, and the major financial support of Italy and Japan with substantial contributions from Belgium, France, Germany and Switzerland. The OPERA Collaboration presently includes about 160 researchers from 30 institutions and 11 countries:
IIHE-ULB Brussels, Belgium; IRB Zagreb, Croatia; LAPP Annecy, France; IPNL Lyon, France; IPHC Strasbourg, France; Hamburg, Germany; Technion Haifa, Israel; Bari, Italy; Bologna, Italy; LNF, Italy, L’Aquila, Italy; LNGS, Italy; Naples, Italy; Padova, Italy; Rome, Italy; Salerno, Italy; Aichi, Japan; Toho, Japan; Kobe, Japan; Nagoya, Japan; Utsunomiya, Japan; GNU Jinju, Korea; INR RAS Moscow, Russia; LPI RAS Moscow, Russia; ITEP Moscow, Russia; SINP MSU Moscow, Russia; JINR Dubna, Russia; Bern, Switzerland; ETH Zurich, Switzerland; METU Ankara, Turkey.

2. CERN, the European Organization for Nuclear Research, is the world's leading laboratory for particle physics. It has its headquarters in Geneva. At present, its Member States are Austria, Belgium, Bulgaria, the Czech Republic, Denmark, Finland, France, Germany, Greece, Hungary, Italy, the Netherlands, Norway, Poland, Portugal, Slovakia, Spain, Sweden, Switzerland and the United Kingdom. Romania is a candidate for accession. India, Israel, Japan, the Russian Federation, the United States of America, Turkey, the European Commission and UNESCO have Observer status.


Source: Public Cern Web

 

 
 
 

What to expect from the LHC in 2012

 

Engineers at work on the ATLAS calorimeter during last year's maintenance shutdown. Image: CERN

The Large Hadron Collider (LHC), the world's largest particle accelerator, is currently shut down for annual maintenance. In February CERN will decide whether to run the LHC at a total energy of 8 TeV this year, instead of 7 TeV as in 2011. Higher energy should increase the chances of finding heavy particles. By early March, all the magnets around the 27-kilometre accelerator will have been cooled down to their operating temperatures of -271.3°C, ready to guide beams of particles through the LHC.

The LHC will resume colliding protons in late March. The goal is to deliver about 1600 trillion proton-proton collisions (16 "inverse femtobarns" of data) to the experiments, compared to the 500 trillion collisions delivered in 2011. More collisions will help the LHC experiments to improve the precision of their measurements and push searches for new physics further.

The CMS and ATLAS experiments will continue to look for new particles this year, of which the Higgs boson is the most publicized. Data taken in 2012 will allow them either to confirm a Higgs discovery or to rule out its existence conclusively.

The LHCb experiment will carry on with its precise measurements of quarks, in the search for weak points in the current Standard Model of particle physics. Meanwhile, ALICE is analyzing lead-ion collision data taken in November 2011 in the quest to understand how quark-gluon plasma formed after the Big Bang. More heavy-ion collisions are scheduled for November this year.

Stay tuned for more from CERN in 2012!

MORE INFORMATION:

Source: Cern WEb
 

 

 

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Biography

Since 1962 I doubted on Newton's laws. I did not accept the infinitive speed and I found un-vivid the laws of gravity and time.

I learned the Einstein's Relativity, thus I found some answers for my questions. But, I had another doubt of Infinitive Mass-Energy. And I wanted to know why light has stable speed?

 


 

 


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22 December, 2013 13:27

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