Operation of an Archaeological Lead PbWO4 Crystal to Search for Neutrinos from Astrophysical Sources with a Transition Edge Sensor
The experimental detection of the CE ν NS allows the investigation of neutrinos and neutrino sources with all-flavor sensitivity. Given its large content in neutrons and stability, Pb is a very appealing choice as target element. The presence of the radioisotope 210 Pb (T 1 / 2 ∼ 22 yrs) makes natur...
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| Veröffentlicht in: | Journal of low temperature physics 2022, Vol.209 (5-6), p.872-878 |
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| creator | Ferreiro Iachellini, N. Pattavina, L. Abdelhameed, A. H. Bento, A. Canonica, L. Danevich, F. Dubovik, O. M. Fuchs, D. Garai, A. Mancuso, M. Petricca, F. Tupitsyna, I. A. |
| description | The experimental detection of the CE
ν
NS allows the investigation of neutrinos and neutrino sources with all-flavor sensitivity. Given its large content in neutrons and stability, Pb is a very appealing choice as target element. The presence of the radioisotope
210
Pb (T
1
/
2
∼
22 yrs) makes natural Pb unsuitable for low-background, low-energy event searches. This limitation can be overcome employing Pb of archaeological origin, where several half-lives of
210
Pb have gone by. We present results of a cryogenic measurement of a 15 g PbWO
4
crystal, grown with archaeological Pb (older than
∼
2000 yrs) that achieved a sub-keV nuclear recoil detection threshold. A ton-scale experiment employing such material, with a detection threshold for nuclear recoils of just 1 keV would probe the entire Milky Way for SuperNovae, with equal sensitivity for all neutrino flavors, allowing the study of the core of such exceptional events. |
| doi_str_mv | 10.1007/s10909-022-02823-8 |
| format | Article |
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ν
NS allows the investigation of neutrinos and neutrino sources with all-flavor sensitivity. Given its large content in neutrons and stability, Pb is a very appealing choice as target element. The presence of the radioisotope
210
Pb (T
1
/
2
∼
22 yrs) makes natural Pb unsuitable for low-background, low-energy event searches. This limitation can be overcome employing Pb of archaeological origin, where several half-lives of
210
Pb have gone by. We present results of a cryogenic measurement of a 15 g PbWO
4
crystal, grown with archaeological Pb (older than
∼
2000 yrs) that achieved a sub-keV nuclear recoil detection threshold. A ton-scale experiment employing such material, with a detection threshold for nuclear recoils of just 1 keV would probe the entire Milky Way for SuperNovae, with equal sensitivity for all neutrino flavors, allowing the study of the core of such exceptional events.</description><identifier>ISSN: 0022-2291</identifier><identifier>EISSN: 1573-7357</identifier><identifier>DOI: 10.1007/s10909-022-02823-8</identifier><language>eng</language><publisher>New York: Springer US</publisher><subject>Archaeology ; Characterization and Evaluation of Materials ; Condensed Matter Physics ; Crystal growth ; Flavors ; Lead isotopes ; Low temperature physics ; Magnetic Materials ; Magnetism ; Neutrinos ; Physics ; Physics and Astronomy ; Radioisotopes ; Sensitivity ; Supernovae</subject><ispartof>Journal of low temperature physics, 2022, Vol.209 (5-6), p.872-878</ispartof><rights>The Author(s) 2022</rights><rights>The Author(s) 2022. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-p157t-60b4d83107ff2f36e2e2a1239590852400066773d73677b5d0469de2b3ff2a4f3</cites><orcidid>0000-0001-5226-6626</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s10909-022-02823-8$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s10909-022-02823-8$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>315,782,786,27933,27934,41497,42566,51328</link.rule.ids></links><search><creatorcontrib>Ferreiro Iachellini, N.</creatorcontrib><creatorcontrib>Pattavina, L.</creatorcontrib><creatorcontrib>Abdelhameed, A. H.</creatorcontrib><creatorcontrib>Bento, A.</creatorcontrib><creatorcontrib>Canonica, L.</creatorcontrib><creatorcontrib>Danevich, F.</creatorcontrib><creatorcontrib>Dubovik, O. M.</creatorcontrib><creatorcontrib>Fuchs, D.</creatorcontrib><creatorcontrib>Garai, A.</creatorcontrib><creatorcontrib>Mancuso, M.</creatorcontrib><creatorcontrib>Petricca, F.</creatorcontrib><creatorcontrib>Tupitsyna, I. A.</creatorcontrib><title>Operation of an Archaeological Lead PbWO4 Crystal to Search for Neutrinos from Astrophysical Sources with a Transition Edge Sensor</title><title>Journal of low temperature physics</title><addtitle>J Low Temp Phys</addtitle><description>The experimental detection of the CE
ν
NS allows the investigation of neutrinos and neutrino sources with all-flavor sensitivity. Given its large content in neutrons and stability, Pb is a very appealing choice as target element. The presence of the radioisotope
210
Pb (T
1
/
2
∼
22 yrs) makes natural Pb unsuitable for low-background, low-energy event searches. This limitation can be overcome employing Pb of archaeological origin, where several half-lives of
210
Pb have gone by. We present results of a cryogenic measurement of a 15 g PbWO
4
crystal, grown with archaeological Pb (older than
∼
2000 yrs) that achieved a sub-keV nuclear recoil detection threshold. A ton-scale experiment employing such material, with a detection threshold for nuclear recoils of just 1 keV would probe the entire Milky Way for SuperNovae, with equal sensitivity for all neutrino flavors, allowing the study of the core of such exceptional events.</description><subject>Archaeology</subject><subject>Characterization and Evaluation of Materials</subject><subject>Condensed Matter Physics</subject><subject>Crystal growth</subject><subject>Flavors</subject><subject>Lead isotopes</subject><subject>Low temperature physics</subject><subject>Magnetic Materials</subject><subject>Magnetism</subject><subject>Neutrinos</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Radioisotopes</subject><subject>Sensitivity</subject><subject>Supernovae</subject><issn>0022-2291</issn><issn>1573-7357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><recordid>eNpFkE1LAzEQhoMoWKt_wFPA8-oks9nsHkupH1Cs0IrHkO0m7Za6WZMU6dVfbtoKHoaBmWc-3peQWwb3DEA-BAYVVBlwnqLkmJVnZMCExEyikOdkAIcW5xW7JFchbACgKgsckJ9Zb7yOreuos1R3dOSXa23c1q3apd7SqdENfas_Zjkd-32IqRQdnRudMGqdp69mF33buUCtd590FKJ3_XofjtNzt_NLE-h3G9dU04XXXWiPxybNyqQ1XXD-mlxYvQ3m5i8PyfvjZDF-zqazp5fxaJr1SUjMCqjzpkQG0lpusTDccM04VqKCUvA8SSoKKbGRmFItGsiLqjG8xsTr3OKQ3J329t597UyIapPe69JJxWWOgpcIIlF4okKfZK2M_6cYqIPZ6mS2So6qo9mqxF_9oHIc</recordid><startdate>2022</startdate><enddate>2022</enddate><creator>Ferreiro Iachellini, N.</creator><creator>Pattavina, L.</creator><creator>Abdelhameed, A. H.</creator><creator>Bento, A.</creator><creator>Canonica, L.</creator><creator>Danevich, F.</creator><creator>Dubovik, O. M.</creator><creator>Fuchs, D.</creator><creator>Garai, A.</creator><creator>Mancuso, M.</creator><creator>Petricca, F.</creator><creator>Tupitsyna, I. A.</creator><general>Springer US</general><general>Springer Nature B.V</general><scope>C6C</scope><orcidid>https://orcid.org/0000-0001-5226-6626</orcidid></search><sort><creationdate>2022</creationdate><title>Operation of an Archaeological Lead PbWO4 Crystal to Search for Neutrinos from Astrophysical Sources with a Transition Edge Sensor</title><author>Ferreiro Iachellini, N. ; Pattavina, L. ; Abdelhameed, A. H. ; Bento, A. ; Canonica, L. ; Danevich, F. ; Dubovik, O. M. ; Fuchs, D. ; Garai, A. ; Mancuso, M. ; Petricca, F. ; Tupitsyna, I. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p157t-60b4d83107ff2f36e2e2a1239590852400066773d73677b5d0469de2b3ff2a4f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Archaeology</topic><topic>Characterization and Evaluation of Materials</topic><topic>Condensed Matter Physics</topic><topic>Crystal growth</topic><topic>Flavors</topic><topic>Lead isotopes</topic><topic>Low temperature physics</topic><topic>Magnetic Materials</topic><topic>Magnetism</topic><topic>Neutrinos</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Radioisotopes</topic><topic>Sensitivity</topic><topic>Supernovae</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ferreiro Iachellini, N.</creatorcontrib><creatorcontrib>Pattavina, L.</creatorcontrib><creatorcontrib>Abdelhameed, A. H.</creatorcontrib><creatorcontrib>Bento, A.</creatorcontrib><creatorcontrib>Canonica, L.</creatorcontrib><creatorcontrib>Danevich, F.</creatorcontrib><creatorcontrib>Dubovik, O. M.</creatorcontrib><creatorcontrib>Fuchs, D.</creatorcontrib><creatorcontrib>Garai, A.</creatorcontrib><creatorcontrib>Mancuso, M.</creatorcontrib><creatorcontrib>Petricca, F.</creatorcontrib><creatorcontrib>Tupitsyna, I. A.</creatorcontrib><collection>Springer Nature OA Free Journals</collection><jtitle>Journal of low temperature physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ferreiro Iachellini, N.</au><au>Pattavina, L.</au><au>Abdelhameed, A. H.</au><au>Bento, A.</au><au>Canonica, L.</au><au>Danevich, F.</au><au>Dubovik, O. M.</au><au>Fuchs, D.</au><au>Garai, A.</au><au>Mancuso, M.</au><au>Petricca, F.</au><au>Tupitsyna, I. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Operation of an Archaeological Lead PbWO4 Crystal to Search for Neutrinos from Astrophysical Sources with a Transition Edge Sensor</atitle><jtitle>Journal of low temperature physics</jtitle><stitle>J Low Temp Phys</stitle><date>2022</date><risdate>2022</risdate><volume>209</volume><issue>5-6</issue><spage>872</spage><epage>878</epage><pages>872-878</pages><issn>0022-2291</issn><eissn>1573-7357</eissn><abstract>The experimental detection of the CE
ν
NS allows the investigation of neutrinos and neutrino sources with all-flavor sensitivity. Given its large content in neutrons and stability, Pb is a very appealing choice as target element. The presence of the radioisotope
210
Pb (T
1
/
2
∼
22 yrs) makes natural Pb unsuitable for low-background, low-energy event searches. This limitation can be overcome employing Pb of archaeological origin, where several half-lives of
210
Pb have gone by. We present results of a cryogenic measurement of a 15 g PbWO
4
crystal, grown with archaeological Pb (older than
∼
2000 yrs) that achieved a sub-keV nuclear recoil detection threshold. A ton-scale experiment employing such material, with a detection threshold for nuclear recoils of just 1 keV would probe the entire Milky Way for SuperNovae, with equal sensitivity for all neutrino flavors, allowing the study of the core of such exceptional events.</abstract><cop>New York</cop><pub>Springer US</pub><doi>10.1007/s10909-022-02823-8</doi><tpages>7</tpages><orcidid>https://orcid.org/0000-0001-5226-6626</orcidid><oa>free_for_read</oa></addata></record> |
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| subjects | Archaeology Characterization and Evaluation of Materials Condensed Matter Physics Crystal growth Flavors Lead isotopes Low temperature physics Magnetic Materials Magnetism Neutrinos Physics Physics and Astronomy Radioisotopes Sensitivity Supernovae |
| title | Operation of an Archaeological Lead PbWO4 Crystal to Search for Neutrinos from Astrophysical Sources with a Transition Edge Sensor |
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