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'''ICARUS''' ('''I'''maging '''C'''osmic '''A'''nd '''R'''are '''U'''nderground '''S'''ignals) is a [[physics]] experiment aimed at studying [[neutrino]]s. It is located at the [[Laboratori Nazionali del Gran Sasso]] (LNGS).
'''ICARUS''' ('''I'''maging '''C'''osmic '''A'''nd '''R'''are '''U'''nderground '''S'''ignals) is a [[physics]] experiment aimed at studying [[neutrino]]s. It was located at the [[Laboratori Nazionali del Gran Sasso]] (LNGS) where it started operations in 2010. After completion of its operations there, it was refurbished at [[CERN]] for re-use at [[Fermilab]], in the same neutrino beam as the [[MiniBooNE]], [[MicroBooNE]] and [[Short Baseline Near Detector]] (SBND) experiments.<ref>{{cite news |url=http://www.symmetrymagazine.org/article/april-2015/italian-neutrino-experiment-to-move-to-the-us |title=Italian neutrino experiment to move to the US |date=22 April 2015 |first=Kathryn |last=Jepsen |journal=Symmetry Magazine |access-date=2015-05-08}}</ref> The ICARUS detector was then taken apart for transport and reassembled at Fermilab, where data collection is expected to begin in fall 2021.


It was initiated by a proposal of a new type of [[neutrino detector]]s by [[Carlo Rubbia]] in 1977.<ref>{{Cite journal|author=Rubbia, C.|year=1977|title=The liquid-Argon time projection chamber: a new concept for neutrino detector
The ICARUS program was initiated by [[Carlo Rubbia]] in 1977, who proposed a new type of [[neutrino detector]].<ref>{{Cite web|author=Rubbia, C.|date=16 May 1977|title=The liquid-Argon time projection chamber: a new concept for neutrino detector |url=https://cds.cern.ch/record/117852/files/CERN-EP-INT-77-8.pdf |publisher=CERN |id=CERN-EP/77-08}}</ref>
These are called Liquid Argon Time Projection Chambers (LAr-TPC), which should combine the advantages of [[bubble chamber]]s and electronic detectors, evolving previous detectors.<ref>{{Cite journal|last1=Cerri|first1=Claudio|last2=Sergiampietri|first2=Franco|date=March 1977|title=Test of a liquid argon calorimeter with very thin sampling|journal=Nuclear Instruments and Methods|language=en|volume=141|issue=2|pages=207–218|doi=10.1016/0029-554X(77)90769-8|bibcode=1977NucIM.141..207C}}</ref> They detect neutrinos through the reaction:<ref>{{Cite journal|author=ICARUS-Collaboration|date=2011|title=Underground operation of the ICARUS T600 LAr-TPC: first results|journal=Journal of Instrumentation|volume=6|issue=7|pages=7011|arxiv=1106.0975|bibcode=2011JInst...6.7011R|doi=10.1088/1748-0221/6/07/P07011|s2cid=53398494}}</ref>
|journal=CERN-
EP/77-08}}</ref>
⚫
These are called Liquid Argon Time Projection Chambers (LAr-TPC), which should combine the advantages of [[bubble chamber]]s and electronic detectors. 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 oscillation]]s and various fundamental topics of [[modern physics]], neutrinos of astronomic or solar sources, and [[CERN Neutrinos to Gran Sasso]] (CNGS) produced 730km away by the [[Super Proton Synchrotron]] from [[CERN]] have been detected through the reaction:<ref>{{Cite journal|author=ICARUS-Collaboration|year=2011|title=Underground operation of the ICARUS T600 LAr-TPC: first results|journal=Journal of Instrumentation|volume=6|issue=07|pages=7011|doi=10.1088/1748-0221/6/07/P07011|arxiv=1106.0975}}</ref>


:<math>{}^{40}Ar + \nu \rightarrow {}^{40}K + e^{-} \,.</math>
:<math>{}^{40}Ar + \nu \rightarrow {}^{40}K + e^{-} \,</math>


(a neutrino combining with an atom of argon-40 to yield an atom of [[potassium]]-40 and an electron.)
⚫
The CNGS neutrinos are also studied by the [[OPERA experiment]], therefore those experiments are also called CNGS1 (OPERA) and CNGS2 (ICARUS).<ref name=icarus12>{{cite journal|author=ICARUS collaboration|title=Measurement of the neutrino velocity with the ICARUS detector at the CNGS beam|arxiv=1203.3433|year=2012}}.</ref>


⚫
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 oscillation]]s and various fundamental topics of [[modern physics]], neutrinos of astronomic or solar sources, and [[CERN Neutrinos to Gran Sasso]] (CNGS) [[Accelerator neutrino|beam]] produced 730&nbsp;km away by the [[Super Proton Synchrotron]] from [[CERN]], have been detected.
⚫
The CNGS measurements also became important when the OPERA group announced in September and November 2011, that they have measured [[faster than light|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]].<ref>{{Cite journal|author=ICARUS-Collaboration|year=2011|title=A search for the analogue to Cherenkov radiation by high energy neutrinos at superluminal speeds in ICARUS|arxiv=1110.3763}}</ref>

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. Concluding measurements should be available in May 2012.<ref name=icarus12 />
⚫
The CNGS neutrinos are also studied by the [[OPERA experiment]], therefore those experiments are also called [[CNGS1 experiment|CNGS1]] (OPERA) and CNGS2 (ICARUS).<ref name=icarus12>{{Cite journal|author=ICARUS Collaboration|title=Measurement of the neutrino velocity with the ICARUS detector at the CNGS beam|journal=Physics Letters B|volume=713|issue=1|pages=17–22|doi=10.1016/j.physletb.2012.05.033|arxiv=1203.3433|date=2012|bibcode = 2012PhLB..713...17A |s2cid=55397067}}</ref>

⚫
The CNGS measurements also became important when the OPERA group announced in September and November 2011 that they had measured [[faster than light|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 Glashow]].<ref>{{Cite journal|author=ICARUS Collaboration|title=A search for the analogue to Cherenkov radiation by high energy neutrinos at superluminal speeds in ICARUS |journal=Physics Letters B|volume=711|issue=3–4|pages=270–275|doi=10.1016/j.physletb.2012.04.014|arxiv=1110.3763|date=2012|bibcode = 2012PhLB..711..270I |s2cid=118357662 }}</ref>
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.<ref name=icarus12 /> 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.<ref>{{Cite journal|author=ICARUS collaboration|title=Precision measurement of the neutrino velocity with the ICARUS detector in the CNGS beam |journal=Journal of High Energy Physics|volume=2012 |issue=11|pages=49|date=2012|doi=10.1007/JHEP11(2012)049|arxiv=1208.2629|bibcode =2012JHEP...11..049A|s2cid=51160473 }}</ref> (See ''[[measurements of neutrino speed]]''.)

The ICARUS detector moved to Fermilab in July 2017 for a new neutrino experiment.<ref>{{Cite web|title = Fermilab {{!}} Newsroom {{!}} Press Releases {{!}} April 22, 2015: ICARUS neutrino experiment to move to Fermilab|url = http://www.fnal.gov/pub/presspass/press_releases/2015/ICARUS-20150422.html|website = www.fnal.gov| date=22 April 2015 |access-date = 2015-08-11}}</ref><ref>{{cite web|title=ICARUS arrives at Fermilab {{!}} News|url=http://news.fnal.gov/2017/07/icarus-arrives-fermilab/|website=news.fnal.gov|date=31 July 2017 }}</ref> 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.<ref name="symmertry">{{cite web|last=Steffel|first=Catherine N.|date=March 2, 2020|title=ICARUS prepares to chase a fourth neutrino|url=https://www.symmetrymagazine.org/article/icarus-prepares-to-chase-a-fourth-neutrino|access-date=March 3, 2020|publisher=symmetrymagazine.org}}</ref> In May 2021, Fermilab announced that ICARUS would begin data collection in the fall of 2021.<ref>{{cite web |last1=Barbu |first1=Brianna |title=ICARUS gets ready to fly |url=https://news.fnal.gov/2021/05/icarus-gets-ready-to-fly/ |website=Fermilab |date=20 May 2021 |access-date=23 September 2021}}</ref>


==References==
==References==
<references />
<references />


== External link ==
== External links ==
*[http://icarus.lngs.infn.it/ ICARUS webpage]
*[http://icarus.lngs.infn.it/ ICARUS webpage] {{Webarchive|url=https://web.archive.org/web/20120307052611/http://icarus.lngs.infn.it/ |date=2012-03-07 }}


[[Category:Neutrino experiments]]
{{Neutrino detectors}}


[[Category:Neutrino experiments]]
[[de:ICARUS]]
[[Category:CERN experiments]]

Latest revision as of 23:30, 20 October 2024

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) where it started operations in 2010. After completion of its operations there, it was refurbished at CERN for re-use at Fermilab, in the same neutrino beam as the MiniBooNE, MicroBooNE and Short Baseline Near Detector (SBND) experiments.[1] The ICARUS detector was then taken apart for transport and reassembled at Fermilab, where data collection is expected to begin in fall 2021.

The ICARUS program was initiated by Carlo Rubbia in 1977, who proposed a new type of neutrino detector.[2] These are called Liquid Argon Time Projection Chambers (LAr-TPC), which should combine the advantages of bubble chambers and electronic detectors, evolving previous detectors.[3] They detect neutrinos through the reaction:[4]

(a neutrino combining with an atom of argon-40 to yield an atom of potassium-40 and an electron.)

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.

The CNGS neutrinos are also studied by the OPERA experiment, therefore those experiments are also called CNGS1 (OPERA) and CNGS2 (ICARUS).[5]

The CNGS measurements also became important when the OPERA group announced in September and November 2011 that they had 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 Glashow.[6] 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.[5] 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.[7] (See measurements of neutrino speed.)

The ICARUS detector moved to Fermilab in July 2017 for a new neutrino experiment.[8][9] 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.[10] In May 2021, Fermilab announced that ICARUS would begin data collection in the fall of 2021.[11]

References

[edit]
  1. ^ Jepsen, Kathryn (22 April 2015). "Italian neutrino experiment to move to the US". Symmetry Magazine. Retrieved 2015-05-08.
  2. ^ Rubbia, C. (16 May 1977). "The liquid-Argon time projection chamber: a new concept for neutrino detector" (PDF). CERN. CERN-EP/77-08.
  3. ^ 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.
  4. ^ 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. S2CID 53398494.
  5. ^ a b 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. S2CID 55397067.
  6. ^ 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. S2CID 118357662.
  7. ^ 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. S2CID 51160473.
  8. ^ "Fermilab | Newsroom | Press Releases | April 22, 2015: ICARUS neutrino experiment to move to Fermilab". www.fnal.gov. 22 April 2015. Retrieved 2015-08-11.
  9. ^ "ICARUS arrives at Fermilab | News". news.fnal.gov. 31 July 2017.
  10. ^ Steffel, Catherine N. (March 2, 2020). "ICARUS prepares to chase a fourth neutrino". symmetrymagazine.org. Retrieved March 3, 2020.
  11. ^ Barbu, Brianna (20 May 2021). "ICARUS gets ready to fly". Fermilab. Retrieved 23 September 2021.
[edit]
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