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ICARUS (Imaging Cosmic And Rare Underground Signals) is a physics experiment aimed at studying neutrinos. It was located at the Laboratori Nazionali del Gran Sasso (LNGS). After completion of its operations there, it was refurbished at CERN for re-use in the same neutrino beam from Fermilab as the MiniBooNE, MicroBooNE and SBND experiments.[1] The ICARUS detector was then broken down for transport and reassembled at Fermilab. In February 2020, scientists at Fermilab began cooling down ICARUS and filling it with 760 tons of liquid argon. Scientists hope to take the first measurements with the refurbished ICARUS later in 2020.[2]

The ICARUS program was initiated by Carlo Rubbia in 1977, who proposed a new type of neutrino detector.[3] These are called Liquid Argon Time Projection Chambers (LAr-TPC), which should combine the advantages of bubble chambers and electronic detectors, evolving previous detectors.[4] In the course of the ICARUS program, such detectors of considerable capacity were proposed. After first runs at Pavia in 2001, the ICARUS T600 detector at Gran Sasso, filled with 760 tons of liquid argon, started operation in 2010. In order to study neutrino oscillations and various fundamental topics of modern physics, neutrinos of astronomic or solar sources, and CERN Neutrinos to Gran Sasso (CNGS) beam produced 730 km away by the Super Proton Synchrotron from CERN, have been detected through the reaction:[5]

\( {}^{40}Ar + \nu \rightarrow {}^{40}K + e^{-} \,. \)

The CNGS neutrinos are also studied by the OPERA experiment, therefore those experiments are also called CNGS1 (OPERA) and CNGS2 (ICARUS).[6]

The CNGS measurements also became important when the OPERA group announced in September and November 2011, that they have measured superluminal neutrinos (see faster-than-light neutrino anomaly). Shortly afterwards, the ICARUS collaboration published a paper in which they argued, that the energy distribution of the neutrinos is not compatible with superluminal particles. This conclusion was based on a theory of Cohen and Sheldon Lee Glashow.[7] In March 2012, they published a direct neutrino velocity measurement based on seven neutrinos events. The result was in agreement with the speed of light and thus special relativity, and contradicts the OPERA result.[6] In August 2012, another neutrino velocity measurement based on 25 neutrino events was published with increased accuracy and statistics, again in agreement with the speed of light,[8] see measurements of neutrino speed.

The ICARUS detector moved to Fermilab in July 2017 for a new neutrino experiment.[9] [10]

As of February 2020, ICARUS is expected to start operations later in 2020. [2]
References

Jepsen, Kathryn (22 April 2015). "Italian neutrino experiment to move to the US". Symmetry Magazine. Retrieved 2015-05-08.
Steffel, Catherine N. (March 2, 2020). "ICARUS prepares to chase a fourth neutrino". symmetrymagazine.org. Retrieved March 3, 2020.
Rubbia, C. (16 May 1977). "The liquid-Argon time projection chamber: a new concept for neutrino detector" (PDF). CERN. CERN-EP/77-08.
Cerri, Claudio; Sergiampietri, Franco (March 1977). "Test of a liquid argon calorimeter with very thin sampling". Nuclear Instruments and Methods. 141 (2): 207–218. Bibcode:1977NucIM.141..207C. doi:10.1016/0029-554X(77)90769-8.
ICARUS-Collaboration (2011). "Underground operation of the ICARUS T600 LAr-TPC: first results". Journal of Instrumentation. 6 (7): 7011.arXiv:1106.0975. Bibcode:2011JInst...6.7011R. doi:10.1088/1748-0221/6/07/P07011.
ICARUS Collaboration (2012). "Measurement of the neutrino velocity with the ICARUS detector at the CNGS beam". Physics Letters B. 713 (1): 17–22.arXiv:1203.3433. Bibcode:2012PhLB..713...17A. doi:10.1016/j.physletb.2012.05.033.
ICARUS Collaboration (2012). "A search for the analogue to Cherenkov radiation by high energy neutrinos at superluminal speeds in ICARUS". Physics Letters B. 711 (3–4): 270–275.arXiv:1110.3763. Bibcode:2012PhLB..711..270I. doi:10.1016/j.physletb.2012.04.014.
ICARUS collaboration (2012). "Precision measurement of the neutrino velocity with the ICARUS detector in the CNGS beam". Journal of High Energy Physics. 2012 (11): 49.arXiv:1208.2629. Bibcode:2012JHEP...11..049A. doi:10.1007/JHEP11(2012)049.
"Fermilab | Newsroom | Press Releases | April 22, 2015: ICARUS neutrino experiment to move to Fermilab". www.fnal.gov. Retrieved 2015-08-11.

"ICARUS arrives at Fermilab | News". news.fnal.gov.

External links

ICARUS webpage

vte

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 ASD BDUNT Borexino BUST HALO IceCube LVD NEVOD SAGE Super-Kamiokande SNEWS

Reactor

Daya Bay Double Chooz KamLAND RENO STEREO

Accelerator

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

0νββ

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

Other

KATRIN WITCH

Construction

ARA ARIANNA Baikal-GVD BEST DUNE Hyper-Kamiokande JUNO KM3NeT SuperNEMO FASERν

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 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 (Baksan or Baxan Neutrino Observatory) Kamioka Observatory LNGS SNOLAB List of neutrino experiments

Physics Encyclopedia

World

Index

Hellenica World - Scientific Library

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