CERN Neutrinos to Gran Sasso

CERN Neutrinos to Gran Sasso Underground Structures

The CERN Neutrinos to Gran Sasso (CNGS) project was a physics project of the European Organization for Nuclear Research (CERN). The aim of the project was to analyse the hypothesis of neutrino oscillation by directing a beam of neutrinos from CERN's facilities to the detector of the OPERA experiment at the Gran Sasso National Laboratory (LNGS), located in the Gran Sasso mountain in Italy. The CNGS facility was housed in a tunnel which diverged from one of the SPS–LHC transfer tunnels, at the France –Switzerland border near Geneva.[1] It used the Super Proton Synchrotron (SPS) accelerator as a source of high-energy protons.

## Contents

* 1 History
* 2 Function
* 3 Results
* 4 References
* 5 External links

## History

The magnetic horn being installed in the CNGS target chamber

Approval for the CNGS project was signed by the CERN Council in December 1999,[2] with civil engineering on the project starting the following September.[3] Construction of the tunnels and service caverns was completed in mid-2004, with equipment installation completed in summer 2005 and commissioning being carried out throughout spring 2006. The first proton beam was sent to the target on 11 July 2006, with the CNGS facility being approved for physics operations on 18 August 2006. CNGS ceased operation in 2012. The tunnel was then repurposed for the AWAKE experiment, which became operational in 2016.

## Function

A proton beam was taken from the SPS at 400 GeV and is made to collide with a graphite target within the CNGS tunnel. The resulting particles, most importantly kaons and pions among many other particles, were then focused by magnetic lensing and travelled 1 kilometre (0.62 mi) down the CNGS tunnel in a vacuum tube. These particles are naturally unstable, and their decay products include muons and muon neutrinos. All particles except neutrinos (protons, muons, pion, kaon...) stop near the end of the tunnel. The neutrinos continue their flight unaffected, as they rarely interact with matter. The number of muons was measured at this point, which gave an indication of the beam's profile and intensity. This beam then passed 732 kilometres (455 mi) through the crust of the Earth and it is expected that during flight some of the muon neutrinos convert into other neutrino types such as tau neutrinos.[1] Once the beam arrived at Gran Sasso, the OPERA and ICARUS experiments were used to detect the neutrinos.

## Results

The first candidates for neutrino oscillation to tau neutrinos were announced in May 2010 by the OPERA experiment.[4] In total five tau neutrinos were observed,[5] consistent with the expectations from the theory of neutrino oscillation.

On 22 September 2011, the OPERA collaboration garnered international attention when they released a preprint[6] reporting the Faster-than-light neutrino anomaly, wherein neutrinos were measured to be travelling, on average, at faster-than-light speed.[7] On 24 February 2012, the team said they had discovered two problems with their previous test, muddying the validity of the previous result.[8] The preprint has been modified to account for these facts, and indeed the measurement of the neutrino speed, there reported, agrees with the velocity of the light.

## References

1. ↑ 1.0 1.1 "General Description of the CERN Project for a Neutrino Beam". http://proj-cngs.web.cern.ch/proj-cngs/Download/CNGSDGVE/cngsdgve.pdf.
2. ↑ "CNGS project Overview". http://proj-cngs.web.cern.ch/proj-cngs/ProjetOverview/projetoverview2002.htm.
3. ↑ "CERN Neutrinos to Gran Sasso (CNGS): First Beam". http://proj-cngs.web.cern.ch/proj-cngs/PDF_files/IEEE06_CNGS.pdf.
4. ↑ "Tau Neutrino embargo". http://www.lngs.infn.it/lngs_infn/contents/lngs_en/public/educational/physics/NEWS_docs/OPERA_press_rel_May_2010.pdf.
5. ↑ O'Luanaigh, C. (6 October 2015). "OPERA detects its fifth tau neutrino". https://home.cern/about/updates/2015/06/opera-detects-its-fifth-tau-neutrino.
6. ↑ T. Adam et al. (OPERA Collaboration) (22 September 2011). "Measurement of the neutrino velocity with the OPERA detector in the CNGS beam". Journal of High Energy Physics 2012 (10): 93. doi:10.1007/JHEP10(2012)093. Bibcode: 2012JHEP...10..093A.
7. ↑ "Speed-of-light experiments give baffling result at Cern". BBC. 22 September 2011. https://www.bbc.co.uk/news/science-environment-15017484.
8. ↑ "Faster-than-light neutrinos could be down to bad wiring". BBC News. 23 February 2012. https://www.bbc.co.uk/news/science-environment-17139635.

## External links

* Official CNGS project website
* Official OPERA experiment website
* Official ICARUS experiment website

* v
* t
* e

Neutrino detectors, experiments, and facilities

Discoveries|

* Cowan–Reines (νe)
* Lederman–Schwartz–Steinberger (νμ)
* DONUT (ντ)
* Neutrino oscillation
* SN 1987 neutrino burst

Operating
(divided by
primary
neutrino
source)|

| Astronomical|

* ANITA
* ANTARES
* BDUNT
* Borexino
* BUST
* HALO
* IceCube
* LVD
* NEVOD
* SAGE
* Super-Kamiokande
* SNEWS

|

Reactor|

* Daya Bay
* Double Chooz
* KamLAND
* RENO
* STEREO

Accelerator|

* ICARUS (Fermilab)
* MicroBooNE
* MINERνA
* MiniBooNE
* NA61/SHINE
* NOνA
* NuMI
* T2K
* COHERENT

0νββ|

* AMoRE
* COBRA
* CUORE
* EXO
* GERDA
* KamLAND-Zen
* MAJORANA
* NEXT
* PandaX
* XMASS

Other|

* KATRIN
* WITCH

Construction|

* ANNIE
* ARA
* ARIANNA
* BEST
* DUNE
* JUNO
* KM3NeT
* SNO+
* SuperNEMO

Retired|

* AMANDA
* CDHS
* Chooz
* CNGS
* Cuoricino
* DONUT
* ERPM
* GALLEX
* Gargamelle
* GNO
* Heidelberg-Moscow
* Homestake
* ICARUS
* IGEX
* IMB
* K2K
* Kamiokande
* KARMEN
* KGF
* LSND
* MACRO
* MINOS
* MINOS+
* NARC
* NEMO
* OPERA
* RICE
* SciBooNE
* SNO
* Soudan 2
* Utah

Proposed|

* CUPID
* GRAND
* Hyper-Kamiokande
* INO
* LAGUNA
* LEGEND
* LENA
* Neutrino Factory
* nEXO
* Nucifer
* SBND
* UNO
* JEM-EUSO
* WATCHMAN

Cancelled|

* DUMAND Project
* Long Baseline Neutrino Experiment
* NEMO Project
* NESTOR Project
* SOX
* BOREX

See also|

* BNO
* Kamioka Observatory
* LNGS
* SNOLAB
* List of neutrino experiments

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