KM3NeT: Difference between revisions
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[[File:KM3NeT logo.jpg|thumb|KM3NeT logo]] |
[[File:KM3NeT logo.jpg|thumb|KM3NeT logo]] |
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The '''Cubic Kilometre Neutrino Telescope''', or '''KM3NeT''', is a |
The '''Cubic Kilometre Neutrino Telescope''', or '''KM3NeT''', is a European [[research]] infrastructure located at the bottom of the [[Mediterranean Sea]]. It hosts the next-generation [[neutrino astronomy|neutrino telescope]] in the form of water [[Cherenkov]] detectors with, when completed, a total instrumented volume of several cubic kilometres distributed over three locations in the Mediterranean: KM3NeT-Fr (offshore [[Toulon]], France), KM3NeT-It (offshore [[Portopalo di Capo Passero]], Sicily, Italy) and KM3NeT-Gr (offshore [[Pylos]], Peloponnese, Greece). The KM3NeT project continues work done for the neutrino telescope [[ANTARES|ANTARES]] operated offshore the coast of France between 2008 and 2022 and the research and development projects [[Neutrino Mediterranean Observatory|NEMO]] offshore the coast of Italy and [[NESTOR |NESTOR]] offshore the coast of Greece. |
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KM3NeT |
Using KM3NeT, scientists search for [[neutrino]]s from distant astrophysical sources like [[supernova remnant]]s, [[gamma-ray burst]]s, [[supernova]]e or colliding stars. The telescope is a powerful tool in the search for [[dark matter]] in the universe. Arrays of thousands of optical sensor modules will detect the faint [[Cherenkov]] light in the deep sea from charged particles originating from collisions of the neutrinos and the water or rock in the vicinity of the detector. The research infrastructure will also house instrumentation for other sciences like [[marine biology]], [[oceanography]] and [[geophysics]] for long-term and on-line monitoring of the deep-sea environment and the sea bottom at depth of several kilometres. |
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Once fully completed, the KM3NeT research infrastructure will consist of several large subdetectors. At first, two of these - together forming the ARCA detector - will indeed form a telescope searching for distant neutrino-sources. Another subdetector - ORCA - will be optimised to measure the properties of the neutrino itself. In that sense, ORCA is a neutrino particle physics detector. Details can be found in the Letter of Intent |
Once fully completed, the KM3NeT research infrastructure will consist of several large subdetectors. At first, two of these - together forming the ARCA detector - will indeed form a telescope searching for distant neutrino-sources. Another subdetector - ORCA - will be optimised to measure the properties of the neutrino itself. In that sense, ORCA is a neutrino particle physics detector. Details can be found in the Letter of Intent.<ref>{{Cite journal|year=2016|title=KM3NeT 2.0 – Letter of Intent for ARCA and ORCA |url=https://iopscience.iop.org/article/10.1088/0954-3899/43/8/084001 |doi=10.1088/0954-3899/43/8/084001|last1=The KM3NeT Collaboration |journal=J. Phys. G: Nucl. Part. Phys. |
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|volume=43 |pages=084001}}</ref> |
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The oversight, governance and management of the implementation and operation of KM3NeT is conducted by an international collaboration. The |
The oversight, governance and management of the implementation and operation of KM3NeT is conducted by an international collaboration. The KM3NeT Collaboration brings together a large diversity of people, from many research institutes in different countries and at different continents. The KM3NeT community consists of about 250 scientists, along with engineers and technicians. |
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== Design == |
== Design == |
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[[File:KM3NeT DOM in the lab.jpg|thumb|KM3NeT Digital Optical Module (DOM) in the laboratory]] |
[[File:KM3NeT DOM in the lab.jpg|thumb|KM3NeT Digital Optical Module (DOM) in the laboratory]] |
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In the future and pending funding, the full neutrino telescope will contain |
In the future and pending funding, the full neutrino telescope will contain in the order of 12000 pressure-resistant glass spheres attached to about 600 flexible vertical strings. In the current phase of construction, the telescope will comprise 345 strings, 230 in the ARCA detector and 115 in the ORCA detector. The strings - or detection units - support 18 sensor spheres each, anchored to the sea floor and supported by floats. Each sphere, called a "digital optical module" (DOM), is about {{convert|44|cm|in}} in diameter, contains 31 three-inch [[photomultiplier]] tubes with supporting electronics, and is connected to shore via a high-bandwidth optical network.<ref>{{Cite journal|year=2022 |title=The KM3NeT multi-PMT optical module |url=https://iopscience.iop.org/article/10.1088/1748-0221/17/07/P07038 |doi=10.1088/1748-0221/17/07/P07038|arxiv=2203.10048 |last1=The KM3NeT Collaboration |journal=Journal of Instrumentation |volume=17 |issue=7 |pages=P07038}}</ref> Together, the ARCA and ORCA detectors contain 6210 DOMs. Via an electro-optical network of cables and subsea junction boxes the optical modules are connected to control stations on shore for electrical power, for detector control and for data transmission.<ref>{{Cite journal|year=2023 |title=KM3NeT Broadcast Optical Data Transport System |url=https://iopscience.iop.org/article/10.1088/1748-0221/18/02/T02001 |doi=10.1088/1748-0221/18/02/T02001 |last1=The KM3NeT Collaboration |journal=Journal of Instrumentation |volume=18 |pages=T02001}}</ref> |
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Since the strings with optical modules moves with the currents in the deep sea, the position and orientation of the modules and thus of the photomultoplier tubes inside is monitored using an acoustic system and a compass system, respectively. |
Since the strings with optical modules moves with the currents in the deep sea, the position and orientation of the modules and thus of the photomultoplier tubes inside is dynamically monitored using an acoustic system and a compass system, respectively.<ref>{{Cite journal|year=2023 |title=Dynamical position and orientation calibration of the KM3NeT telescope |url=https://pos.sissa.it/444/1033/pdf|last1=The KM3NeT Collaboration |journal=PoS (ICRC2023)|pages=1033}}</ref>. Nanobeacons at the string are used for time calibration.<ref>{{Cite journal|year=2022 |title=Nanobeacon: A time calibration device for the KM3NeT neutrino telescope |url=https://www.sciencedirect.com/science/article/pii/S0168900222005174?via%3Dihub |doi=10.1016/j.nima.2022.167132 |last1=The KM3NeT Collaboration | journal=NIMA |volume=1040 |pages=167132}}</ref> |
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At the shore of each KM3NeT installation site, a farm of computers will perform the first data filter in the search for the signal of cosmic neutrinos, prior to streaming the data to a central KM3NeT data centre for storage and further analysis by the KM3NeT scientists. |
At the shore of each KM3NeT installation site, a farm of computers will perform the first data filter in the search for the signal of cosmic neutrinos, prior to streaming the data to a central KM3NeT data centre for storage and further analysis by the KM3NeT scientists. |
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The KM3NeT-It site, at a depth of 3400 m, hosts the ARCA (''Astroparticle Research with Cosmics in the Abyss'') detector, which with more widely spaced DOMs is optimised for the detection of high-energy cosmic neutrinos in the TeV–PeV range. Its strings are 650 m long, spaced 90 m apart. |
The KM3NeT-It site, at a depth of 3400 m, hosts the ARCA (''Astroparticle Research with Cosmics in the Abyss'') detector, which with more widely spaced DOMs is optimised for the detection of high-energy cosmic neutrinos in the TeV–PeV range. Its strings are 650 m long, spaced 90 m apart. |
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The KM3NeT-Fr site, at a depth of 2475 m, hosts the ORCA (''Oscillation Research with Cosmics in the Abyss'') detector, a more compact array with more closely spaced sensors optimised for the detection of atmospheric neutrinos in the GeV range. ORCA will consist of 115 strings in a 20 m triangular grid, with a 9 m spacing between the DOMs in a string. Overall, the array is about 210 m in diameter, and the strings are 200 m long. |
The KM3NeT-Fr site, at a depth of 2475 m, hosts the ORCA (''Oscillation Research with Cosmics in the Abyss'') detector, a more compact array with more closely spaced sensors optimised for the detection of atmospheric neutrinos in the GeV range. ORCA will consist of 115 strings in a 20 m triangular grid, with a 9 m spacing between the DOMs in a string. Overall, the array is about 210 m in diameter, and the strings are 200 m long. |
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== Construction == |
== Construction == |
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The design of the KM3NeT neutrino telescope is very modular and construction can be phased in time. In 2012, the first phase of the implementation of the KM3NeT research facility started with the construction of the seabed infrastructures at the KM3NeT-Fr and KM3NeT-It sites. A prototype KM3NeT Digital Optical Module (KM3NeT-DOM) took data successfully in 2014-2015 |
The design of the KM3NeT neutrino telescope is very modular and construction can be phased in time. In 2012, the first phase of the implementation of the KM3NeT research facility started with the construction of the seabed infrastructures at the KM3NeT-Fr and KM3NeT-It sites. A prototype KM3NeT Digital Optical Module (KM3NeT-DOM) took data successfully in 2014-2015 |
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<ref>{{Cite journal|year=2014 |title=Nanobeacon: Deep sea tests of a prototype of the KM3NeT digital optical module |url=https://link.springer.com/article/10.1140/epjc/s10052-014-3056-3 |doi=10.1140/epjc/s10052-014-3056-3 |last1=The KM3NeT Collaboration | journal=Eur.Phys.J. C |volume=74 |pages=3056}}</ref> |
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as part of the [[ANTARES (telescope)|ANTARES]] telescope. |
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At the KM3NeT-It site a prototype string took data, also during about one year<ref>{{Cite journal|year=2016 |title=The prototype detection unit of the KM3NeT detector|url=https://link.springer.com/article/10.1140/epjc/s10052-015-3868-9?wt_mc=internal.event.1.SEM.ArticleAuthorIncrementalIssue |doi=10.1140/epjc/s10052-015-3868-9 |last1=The KM3NeT Collaboration | journal=Eur.Phys.J. C |volume=76 |pages=54}}</ref>. |
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The first phase of construction has been successfully terminated. The second phase of construction has begun and complies the completion of the ARCA and ORCA detectors at the KM3NeT-It and KM3NeT-Fr sites, respectively. |
The first phase of construction has been successfully terminated. The second phase of construction has begun and complies the completion of the ARCA and ORCA detectors at the KM3NeT-It and KM3NeT-Fr sites, respectively. |
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==Further reading== |
==Further reading== |
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* {{cite journal |title=Letter of intent for KM3NeT 2.0 |last=Adrián-Martínez |first=S. |display-authors=etal |date=24 June 2016 |journal=[[Journal of Physics G]] |volume=43 |issue=8 |page=084001 |arxiv=1601.07459 |bibcode=2016JPhG...43h4001A |doi=10.1088/0954-3899/43/8/084001 |doi-access=free}} |
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* {{cite web |last=Adcock |first=C. |date=24 June 2016 |title=KM3NeT: The next big thing in neutrino physics |url=https://jphysplus.iop.org/2016/06/24/km3net-the-next-big-thing-in-neutrino-physics/ |work=[[Journal of Physics G|JPhys+]] }} |
* {{cite web |last=Adcock |first=C. |date=24 June 2016 |title=KM3NeT: The next big thing in neutrino physics |url=https://jphysplus.iop.org/2016/06/24/km3net-the-next-big-thing-in-neutrino-physics/ |work=[[Journal of Physics G|JPhys+]] }} |
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Revision as of 22:17, 22 September 2023
The Cubic Kilometre Neutrino Telescope, or KM3NeT, is a European research infrastructure located at the bottom of the Mediterranean Sea. It hosts the next-generation neutrino telescope in the form of water Cherenkov detectors with, when completed, a total instrumented volume of several cubic kilometres distributed over three locations in the Mediterranean: KM3NeT-Fr (offshore Toulon, France), KM3NeT-It (offshore Portopalo di Capo Passero, Sicily, Italy) and KM3NeT-Gr (offshore Pylos, Peloponnese, Greece). The KM3NeT project continues work done for the neutrino telescope ANTARES operated offshore the coast of France between 2008 and 2022 and the research and development projects NEMO offshore the coast of Italy and NESTOR offshore the coast of Greece.
Using KM3NeT, scientists search for neutrinos from distant astrophysical sources like supernova remnants, gamma-ray bursts, supernovae or colliding stars. The telescope is a powerful tool in the search for dark matter in the universe. Arrays of thousands of optical sensor modules will detect the faint Cherenkov light in the deep sea from charged particles originating from collisions of the neutrinos and the water or rock in the vicinity of the detector. The research infrastructure will also house instrumentation for other sciences like marine biology, oceanography and geophysics for long-term and on-line monitoring of the deep-sea environment and the sea bottom at depth of several kilometres.
Once fully completed, the KM3NeT research infrastructure will consist of several large subdetectors. At first, two of these - together forming the ARCA detector - will indeed form a telescope searching for distant neutrino-sources. Another subdetector - ORCA - will be optimised to measure the properties of the neutrino itself. In that sense, ORCA is a neutrino particle physics detector. Details can be found in the Letter of Intent.[1]
The oversight, governance and management of the implementation and operation of KM3NeT is conducted by an international collaboration. The KM3NeT Collaboration brings together a large diversity of people, from many research institutes in different countries and at different continents. The KM3NeT community consists of about 250 scientists, along with engineers and technicians.
Design
In the future and pending funding, the full neutrino telescope will contain in the order of 12000 pressure-resistant glass spheres attached to about 600 flexible vertical strings. In the current phase of construction, the telescope will comprise 345 strings, 230 in the ARCA detector and 115 in the ORCA detector. The strings - or detection units - support 18 sensor spheres each, anchored to the sea floor and supported by floats. Each sphere, called a "digital optical module" (DOM), is about 44 centimetres (17 in) in diameter, contains 31 three-inch photomultiplier tubes with supporting electronics, and is connected to shore via a high-bandwidth optical network.[2] Together, the ARCA and ORCA detectors contain 6210 DOMs. Via an electro-optical network of cables and subsea junction boxes the optical modules are connected to control stations on shore for electrical power, for detector control and for data transmission.[3]
Since the strings with optical modules moves with the currents in the deep sea, the position and orientation of the modules and thus of the photomultoplier tubes inside is dynamically monitored using an acoustic system and a compass system, respectively.[4]. Nanobeacons at the string are used for time calibration.[5]
At the shore of each KM3NeT installation site, a farm of computers will perform the first data filter in the search for the signal of cosmic neutrinos, prior to streaming the data to a central KM3NeT data centre for storage and further analysis by the KM3NeT scientists.
The KM3NeT-It site, at a depth of 3400 m, hosts the ARCA (Astroparticle Research with Cosmics in the Abyss) detector, which with more widely spaced DOMs is optimised for the detection of high-energy cosmic neutrinos in the TeV–PeV range. Its strings are 650 m long, spaced 90 m apart.
The KM3NeT-Fr site, at a depth of 2475 m, hosts the ORCA (Oscillation Research with Cosmics in the Abyss) detector, a more compact array with more closely spaced sensors optimised for the detection of atmospheric neutrinos in the GeV range. ORCA will consist of 115 strings in a 20 m triangular grid, with a 9 m spacing between the DOMs in a string. Overall, the array is about 210 m in diameter, and the strings are 200 m long.
Construction
The design of the KM3NeT neutrino telescope is very modular and construction can be phased in time. In 2012, the first phase of the implementation of the KM3NeT research facility started with the construction of the seabed infrastructures at the KM3NeT-Fr and KM3NeT-It sites. A prototype KM3NeT Digital Optical Module (KM3NeT-DOM) took data successfully in 2014-2015 [6] as part of the ANTARES telescope. At the KM3NeT-It site a prototype string took data, also during about one year[7].
The first phase of construction has been successfully terminated. The second phase of construction has begun and complies the completion of the ARCA and ORCA detectors at the KM3NeT-It and KM3NeT-Fr sites, respectively.
Relation to other neutrino telescopes
For the design of the neutrino detector, KM3NeT builds on the experience of three pilot projects in the Mediterranean Sea: the ANTARES detector, the Neutrino Mediterranean Observatory (NEMO) project and the NESTOR Project. NEMO and NESTOR were both research and development projects only. The ANTARES telescope was completed on 30 May 2008, and was the largest neutrino telescope in the Northern Hemisphere. In the southern hemisphere, at Antarctica, the IceCube Neutrino Observatory is already operational. In Lake Baikal a gigaton volume neutrino telescope is being built. Together, the three telescopes view the full sky and form a global neutrino observatory.
Relation with the European institutions
As a unique experiment in Europe and thanks to the success of its predecessor ANTARES, KM3NeT has a special position within the European context. Throughout its history KM3NeT has received support from the European Union, via the participation in several European projects, but also thanks to the acknowledgement of the value of KM3NeT by the European institutions.
Indeed, in 2006 KM3NeT was included in the European Strategy Forum on Research Infrastructure (ESFRI) roadmap, which recognises as a priority the KM3NeT research infrastructure for Europe’s scientific needs for the next 10-20 years. The support was renewed by the Council of the European Union for the 2019-2026 period. While the first phase of the project led to the engineering of the modular detector and the construction of prototypes, the objective of KM3NeT 2.0 is to adapt to the scientific and technological progress made in the field of neutrino astroparticle physics. Therefore, the second inscription in the ESFRI roadmap reaffirms the interest of KM3NeT during its effective construction phase.
Along with the Council, the implementation of KM3NeT installation sites also benefitted from funding through the European Regional Development Fund (ERDF), confirming the economic, social and territorial potential of KM3NeT at regional level.
In addition, the experiment also benefited from different funding through European research and innovation programmes:
- From 2006 to 2009, the Design Study was supported by the European Sixth Framework Programme (EU FP6). The objective was to address the scientific and technical design issues related to the installation of the telescope.
- From 2008 to 2012, the Preparatory Phase for the KM3NeT infrastructure was funded by the European Seventh Framework Programme (EU FP7) in order to bring the telescope to its construction stage.
- From 2017 to 2020, KM3NeT benefited from the Horizon 2020 programme through the implementation of the KM3NeT-INFRADEV project, which objective was to support the development of the legal and governance aspects of the experiment, as well as to explore sustainable solution for the operation of the research infrastructure.
- From 2023 to 2026, these objectives are being taken up as part of the KM3NeT-INFRADEV2 project, funded by Horizon Europe, that should lead to the full implementation of the KM3NeT Research Infrastructure.
Finally, KM3NeT participated in many European projects, led by partners of the Collaboration. For example, KM3NeT takes part in the EMSO network, by providing long-term access for Earth and Sea sciences research. KM3NeT participated in the ASTERICS project, and is still participating in the EOSC European initiative for Open Science as well as in the related ESCAPE project[8]. Last but not least, KM3NeT is also engaged in citizen science, notably through the REINFORCE project[9].
Socio-economic and environmental impact of KM3NeT
Most of these EU projects have been the means of financing and implementing the KM3NeT Collaboration's commitment to deliver a positive experiment in terms of socio-economic and environmental impacts[10]. In particular:
- Education and training: Via its participating research institutes and university groups, KM3NeT contributes to the education of the next generation of undergraduate and graduate students and to postdoctoral training. Students are given the opportunity to participate in all activities of the Collaboration, ranging from presentations in Collaboration meetings to participation in "shifts" monitoring the operation of the detectors. Also, regarding the training of younger people, KM3NeT strongly engages in citizen science.
- Economic benefit: The funding authorities of the participating Parties in the Collaboration support investments in the construction and operation of the detectors and the involvement of scientists, engineers, students and administrative staff. Relevant companies profit from the licence-free cutting-edge technologies and from orders for innovative products. Finally, by working with locally-based companies, KM3NeT contributes to local economic development on sites.
- Diversity and inclusion: The KM3NeT Collaboration is committed to creating an inclusive working environment with equal opportunities for all talents. Recognising the importance of diverse teams for the successful realisation of the experiment, the Collaboration has adopted a policy strategy, which includes measures taken to provide a welcoming and inclusive working environment to all talents, regardless of characteristics such as, but not limited to gender, age, disability, ethnicity, religion or sexual orientation and to support the professional advancement of all. The diversity policy also includes measurable goals for the number of women and early-career scientists in all positions, but in particular in leadership positions in the Collaboration[11].
- Environmental awareness: One of the objectives of the Collaboration is to demonstrate KM3NeT as a role model for a research infrastructure with high sustainability standards and societal and environmental awareness. In order to reach this ambition, a number of initiatives have been taken to ensure a sustainable future for the experiment. For example, a plan for making the three sites of KM3NeT carbon-neutral facilities using renewable energy sources was established, solutions and procedures for transforming the daily activities of the KM3NeT community to a sustainable configuration are being identified under the INFRADEV2 project and studies are being conducted regarding potential impact of the KM3NeT decommissioning on the environment, with the objective to define recycling schemes[12]. Finally, KM3NeT deploys a number of citizen science initiatives in order to raise environmental awareness among the general public.
Image gallery
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Electronics to read out the photomultiplier tubes and calibration instrumentation inside the KM3NeT DOM -
The KM3NeT LOM – the launching vehicle of Optical Modules – being loaded onto the RV Pelagia deployment vessel. A full string detection is rolled onto the LOM. After arrival at the seabed the string is unrolled to its full length. -
A prototype KM3NeT DOM installed in the instrumentation line of the ANTARES neutrino telescope. The DOM is operational since April 2013.
References
- ^ The KM3NeT Collaboration (2016). "KM3NeT 2.0 – Letter of Intent for ARCA and ORCA". J. Phys. G: Nucl. Part. Phys. 43: 084001. doi:10.1088/0954-3899/43/8/084001.
{{cite journal}}: CS1 maint: numeric names: authors list (link) - ^ The KM3NeT Collaboration (2022). "The KM3NeT multi-PMT optical module". Journal of Instrumentation. 17 (7): P07038. arXiv:2203.10048. doi:10.1088/1748-0221/17/07/P07038.
{{cite journal}}: CS1 maint: numeric names: authors list (link) - ^ The KM3NeT Collaboration (2023). "KM3NeT Broadcast Optical Data Transport System". Journal of Instrumentation. 18: T02001. doi:10.1088/1748-0221/18/02/T02001.
{{cite journal}}: CS1 maint: numeric names: authors list (link) - ^ The KM3NeT Collaboration (2023). "Dynamical position and orientation calibration of the KM3NeT telescope". PoS (ICRC2023): 1033.
{{cite journal}}: CS1 maint: numeric names: authors list (link) - ^ The KM3NeT Collaboration (2022). "Nanobeacon: A time calibration device for the KM3NeT neutrino telescope". NIMA. 1040: 167132. doi:10.1016/j.nima.2022.167132.
{{cite journal}}: CS1 maint: numeric names: authors list (link) - ^ The KM3NeT Collaboration (2014). "Nanobeacon: Deep sea tests of a prototype of the KM3NeT digital optical module". Eur.Phys.J. C. 74: 3056. doi:10.1140/epjc/s10052-014-3056-3.
{{cite journal}}: CS1 maint: numeric names: authors list (link) - ^ The KM3NeT Collaboration (2016). "The prototype detection unit of the KM3NeT detector". Eur.Phys.J. C. 76: 54. doi:10.1140/epjc/s10052-015-3868-9.
{{cite journal}}: CS1 maint: numeric names: authors list (link) - ^ "ESCAPE project".
- ^ "REINFORCE project".
- ^ "KM3NeT Impact".
- ^ "Diversity and Inclusion in KM3NeT".
- ^ "KM3NeT-INFRADEV2".
Further reading
- Adcock, C. (24 June 2016). "KM3NeT: The next big thing in neutrino physics". JPhys+.
