Constraints on Lightly Ionizing Particles from CDMSlite
The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) achieved efficient detection of very small recoil energies in its germanium target, resulting in sensitivity to Lightly Ionizing Particles (LIPs) in a previously unexplored region of charge, mass, and velocity parameter...
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| creator | Collaboration, SuperCDMS Alkhatib, I Aralis, T Aramaki, T Arnquist, I J I Ataee Langroudy Azadbakht, E Barker, D Bathurst, C Bauer, D A Bezerra, L V S Bhattacharyya, R Bowles, M A Brink, P L Cabrera, B Calkins, R Cerdeño, D G Y -Y Chang Chaudhuri, M Chen, R Chott, N Cooley, J Coombes, H Corbett, J di Vacri, M L Diamond, M D Fascione, E Figueroa-Feliciano, E Fink, C W Fritts, M Gerbier, G Germond, R Ghaith, M Golwala, S R Harris, H R Hines, B A Hollister, M I Hong, Z Hoppe, E W Hsu, L Huber, M E Iyer, V Jardin, D Jastram, A Kelsey, M H Kubik, A Kurinsky, N A Lawrence, R E A Li Loer, B E Lopez Asamar Lukens, P Mahapatra, R Mandic, V Mast, N Mayer, A J H Meyer zu Theenhausen Michaud, É M Michielin, E Mirabolfathi, N Mohanty, B Morales Mendoza, J D Nagorny, S Nelson, J Neog, H Novati, V Orrell, J L Oser, S M Page, W A Partridge, R Podviianiuk, R Ponce, F Poudel, S Pradeep, A Reid, E Ren, R Reynolds, T Saab, T Sadoulet, B Sander, J Sattari, A Schnee, R W Scorza, S Serfass, B Sincavage, D J Street, J Verma, S Villano, A N B von Krosigk Watkins, S L Wilson, J S Wilson, M J Winchell, J Wright, D H Yellin, S Young, B A Yu, T C Zhang, E Zhang, H G Zhao, X |
| description | The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) achieved efficient detection of very small recoil energies in its germanium target, resulting in sensitivity to Lightly Ionizing Particles (LIPs) in a previously unexplored region of charge, mass, and velocity parameter space. We report first direct-detection limits calculated using the optimum interval method on the vertical intensity of cosmogenically-produced LIPs with an electric charge smaller than \(e/(3\times10^5\)), as well as the strongest limits for charge \(\leq e/160\), with a minimum vertical intensity of \(1.36\times10^{-7}\)\,cm\(^{-2}\)s\(^{-1}\)sr\(^{-1}\) at charge \(e/160\). These results apply over a wide range of LIP masses (5\,MeV/\(c^2\) to 100\,TeV/\(c^2\)) and cover a wide range of \(\beta\gamma\) values (0.1 -- \(10^6\)), thus excluding non-relativistic LIPs with \(\beta\gamma\) as small as 0.1 for the first time. |
| doi_str_mv | 10.48550/arxiv.2011.09183 |
| format | Article |
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We report first direct-detection limits calculated using the optimum interval method on the vertical intensity of cosmogenically-produced LIPs with an electric charge smaller than \(e/(3\times10^5\)), as well as the strongest limits for charge \(\leq e/160\), with a minimum vertical intensity of \(1.36\times10^{-7}\)\,cm\(^{-2}\)s\(^{-1}\)sr\(^{-1}\) at charge \(e/160\). 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Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27902</link.rule.ids><backlink>$$Uhttps://doi.org/10.1103/PhysRevLett.127.081802$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.2011.09183$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Collaboration, SuperCDMS</creatorcontrib><creatorcontrib>Alkhatib, I</creatorcontrib><creatorcontrib>Aralis, T</creatorcontrib><creatorcontrib>Aramaki, T</creatorcontrib><creatorcontrib>Arnquist, I 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B</creatorcontrib><creatorcontrib>E Lopez Asamar</creatorcontrib><creatorcontrib>Lukens, P</creatorcontrib><creatorcontrib>Mahapatra, R</creatorcontrib><creatorcontrib>Mandic, V</creatorcontrib><creatorcontrib>Mast, N</creatorcontrib><creatorcontrib>Mayer, A J</creatorcontrib><creatorcontrib>H Meyer zu Theenhausen</creatorcontrib><creatorcontrib>Michaud, É M</creatorcontrib><creatorcontrib>Michielin, E</creatorcontrib><creatorcontrib>Mirabolfathi, N</creatorcontrib><creatorcontrib>Mohanty, B</creatorcontrib><creatorcontrib>Morales Mendoza, J D</creatorcontrib><creatorcontrib>Nagorny, S</creatorcontrib><creatorcontrib>Nelson, J</creatorcontrib><creatorcontrib>Neog, H</creatorcontrib><creatorcontrib>Novati, V</creatorcontrib><creatorcontrib>Orrell, J L</creatorcontrib><creatorcontrib>Oser, S M</creatorcontrib><creatorcontrib>Page, W A</creatorcontrib><creatorcontrib>Partridge, R</creatorcontrib><creatorcontrib>Podviianiuk, R</creatorcontrib><creatorcontrib>Ponce, F</creatorcontrib><creatorcontrib>Poudel, S</creatorcontrib><creatorcontrib>Pradeep, A</creatorcontrib><creatorcontrib>Reid, E</creatorcontrib><creatorcontrib>Ren, R</creatorcontrib><creatorcontrib>Reynolds, T</creatorcontrib><creatorcontrib>Saab, T</creatorcontrib><creatorcontrib>Sadoulet, B</creatorcontrib><creatorcontrib>Sander, J</creatorcontrib><creatorcontrib>Sattari, A</creatorcontrib><creatorcontrib>Schnee, R W</creatorcontrib><creatorcontrib>Scorza, S</creatorcontrib><creatorcontrib>Serfass, B</creatorcontrib><creatorcontrib>Sincavage, D J</creatorcontrib><creatorcontrib>Street, J</creatorcontrib><creatorcontrib>Verma, S</creatorcontrib><creatorcontrib>Villano, A N</creatorcontrib><creatorcontrib>B von Krosigk</creatorcontrib><creatorcontrib>Watkins, S L</creatorcontrib><creatorcontrib>Wilson, J S</creatorcontrib><creatorcontrib>Wilson, M J</creatorcontrib><creatorcontrib>Winchell, J</creatorcontrib><creatorcontrib>Wright, D H</creatorcontrib><creatorcontrib>Yellin, S</creatorcontrib><creatorcontrib>Young, B A</creatorcontrib><creatorcontrib>Yu, T C</creatorcontrib><creatorcontrib>Zhang, E</creatorcontrib><creatorcontrib>Zhang, H G</creatorcontrib><creatorcontrib>Zhao, X</creatorcontrib><title>Constraints on Lightly Ionizing Particles from CDMSlite</title><title>arXiv.org</title><description>The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) achieved efficient detection of very small recoil energies in its germanium target, resulting in sensitivity to Lightly Ionizing Particles (LIPs) in a previously unexplored region of charge, mass, and velocity parameter space. We report first direct-detection limits calculated using the optimum interval method on the vertical intensity of cosmogenically-produced LIPs with an electric charge smaller than \(e/(3\times10^5\)), as well as the strongest limits for charge \(\leq e/160\), with a minimum vertical intensity of \(1.36\times10^{-7}\)\,cm\(^{-2}\)s\(^{-1}\)sr\(^{-1}\) at charge \(e/160\). These results apply over a wide range of LIP masses (5\,MeV/\(c^2\) to 100\,TeV/\(c^2\)) and cover a wide range of \(\beta\gamma\) values (0.1 -- \(10^6\)), thus excluding non-relativistic LIPs with \(\beta\gamma\) as small as 0.1 for the first time.</description><subject>Dark matter</subject><subject>Germanium</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - High Energy Physics - Experiment</subject><subject>Physics - High Energy Physics - Phenomenology</subject><subject>Physics - Instrumentation and Detectors</subject><subject>Recoil</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotj8tKAzEARYMgWGo_wJUB1zPmnclSxldhRMHuh8xMUlOmSU1SsX59X97N3Rwu9wBwg1HJKs7RvY6_7qckCOMSKVzRCzAhlOKiYoRcgVlKK4QQEZJwTidA1sGnHLXzOcHgYeOWX3ncwXnw7s_5JfzQMbt-NAnaGNawfnz7HF021-DS6jGZ2X9PweL5aVG_Fs37y7x-aArNCS8IYX2FRKc1V0pSJI5R2EoreU95j1knmaVImo4LwzrLNeqZHQZJhRo6Rqfg9jx7smo30a113LVHu_ZkdyDuzsQmhu-tSbldhW30h08tYYJQRJTidA8YNlDN</recordid><startdate>20220219</startdate><enddate>20220219</enddate><creator>Collaboration, SuperCDMS</creator><creator>Alkhatib, I</creator><creator>Aralis, T</creator><creator>Aramaki, T</creator><creator>Arnquist, I J</creator><creator>I Ataee Langroudy</creator><creator>Azadbakht, E</creator><creator>Barker, D</creator><creator>Bathurst, C</creator><creator>Bauer, D A</creator><creator>Bezerra, L V 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arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PHGZM</scope><scope>PHGZT</scope><scope>PIMPY</scope><scope>PKEHL</scope><scope>PQEST</scope><scope>PQGLB</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20220219</creationdate><title>Constraints on Lightly Ionizing Particles from CDMSlite</title><author>Collaboration, SuperCDMS ; Alkhatib, I ; Aralis, T ; Aramaki, T ; Arnquist, I J ; I Ataee Langroudy ; Azadbakht, E ; Barker, D ; Bathurst, C ; Bauer, D A ; Bezerra, L V S ; Bhattacharyya, R ; Bowles, M A ; Brink, P L ; Cabrera, B ; Calkins, R ; Cerdeño, D G ; Y -Y Chang ; Chaudhuri, M ; Chen, R ; Chott, N ; Cooley, J ; Coombes, H ; Corbett, J ; di Vacri, M L ; Diamond, M D ; Fascione, E ; Figueroa-Feliciano, E ; Fink, C W ; Fritts, M ; Gerbier, G ; Germond, R ; Ghaith, M ; Golwala, S R ; Harris, H R ; Hines, B A ; Hollister, M I ; Hong, Z ; Hoppe, E W ; Hsu, L ; Huber, M E ; Iyer, V ; Jardin, D ; Jastram, A ; Kelsey, M H ; Kubik, A ; Kurinsky, N A ; Lawrence, R E ; A Li ; Loer, B ; E Lopez Asamar ; Lukens, P ; Mahapatra, R ; Mandic, V ; Mast, N ; Mayer, A J ; H Meyer zu Theenhausen ; Michaud, É M ; Michielin, E ; Mirabolfathi, N ; Mohanty, B ; Morales Mendoza, J D ; Nagorny, S ; Nelson, J ; Neog, H ; Novati, V ; Orrell, J L ; Oser, S M ; Page, W A ; Partridge, R ; Podviianiuk, R ; Ponce, F ; Poudel, S ; Pradeep, A ; Reid, E ; Ren, R ; Reynolds, T ; Saab, T ; Sadoulet, B ; Sander, J ; Sattari, A ; Schnee, R W ; Scorza, S ; Serfass, B ; Sincavage, D J ; Street, J ; Verma, S ; Villano, A N ; B von Krosigk ; Watkins, S L ; Wilson, J S ; Wilson, M J ; Winchell, J ; Wright, D H ; Yellin, S ; Young, B A ; Yu, T C ; Zhang, E ; Zhang, H G ; Zhao, X</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a525-224c806baa5997306666691f7f75c35c14b74f307eb56e4bf5a0c4fdd7369db43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Dark matter</topic><topic>Germanium</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - High Energy Physics - Experiment</topic><topic>Physics - High Energy Physics - Phenomenology</topic><topic>Physics - Instrumentation and Detectors</topic><topic>Recoil</topic><toplevel>online_resources</toplevel><creatorcontrib>Collaboration, SuperCDMS</creatorcontrib><creatorcontrib>Alkhatib, I</creatorcontrib><creatorcontrib>Aralis, T</creatorcontrib><creatorcontrib>Aramaki, T</creatorcontrib><creatorcontrib>Arnquist, I J</creatorcontrib><creatorcontrib>I Ataee Langroudy</creatorcontrib><creatorcontrib>Azadbakht, E</creatorcontrib><creatorcontrib>Barker, D</creatorcontrib><creatorcontrib>Bathurst, C</creatorcontrib><creatorcontrib>Bauer, D A</creatorcontrib><creatorcontrib>Bezerra, L V S</creatorcontrib><creatorcontrib>Bhattacharyya, R</creatorcontrib><creatorcontrib>Bowles, M A</creatorcontrib><creatorcontrib>Brink, P L</creatorcontrib><creatorcontrib>Cabrera, B</creatorcontrib><creatorcontrib>Calkins, R</creatorcontrib><creatorcontrib>Cerdeño, D G</creatorcontrib><creatorcontrib>Y -Y Chang</creatorcontrib><creatorcontrib>Chaudhuri, M</creatorcontrib><creatorcontrib>Chen, R</creatorcontrib><creatorcontrib>Chott, N</creatorcontrib><creatorcontrib>Cooley, J</creatorcontrib><creatorcontrib>Coombes, H</creatorcontrib><creatorcontrib>Corbett, J</creatorcontrib><creatorcontrib>di Vacri, M L</creatorcontrib><creatorcontrib>Diamond, M D</creatorcontrib><creatorcontrib>Fascione, E</creatorcontrib><creatorcontrib>Figueroa-Feliciano, E</creatorcontrib><creatorcontrib>Fink, C W</creatorcontrib><creatorcontrib>Fritts, M</creatorcontrib><creatorcontrib>Gerbier, G</creatorcontrib><creatorcontrib>Germond, R</creatorcontrib><creatorcontrib>Ghaith, M</creatorcontrib><creatorcontrib>Golwala, S R</creatorcontrib><creatorcontrib>Harris, H R</creatorcontrib><creatorcontrib>Hines, B A</creatorcontrib><creatorcontrib>Hollister, M I</creatorcontrib><creatorcontrib>Hong, Z</creatorcontrib><creatorcontrib>Hoppe, E W</creatorcontrib><creatorcontrib>Hsu, L</creatorcontrib><creatorcontrib>Huber, M E</creatorcontrib><creatorcontrib>Iyer, V</creatorcontrib><creatorcontrib>Jardin, D</creatorcontrib><creatorcontrib>Jastram, A</creatorcontrib><creatorcontrib>Kelsey, M H</creatorcontrib><creatorcontrib>Kubik, A</creatorcontrib><creatorcontrib>Kurinsky, N A</creatorcontrib><creatorcontrib>Lawrence, R E</creatorcontrib><creatorcontrib>A Li</creatorcontrib><creatorcontrib>Loer, B</creatorcontrib><creatorcontrib>E Lopez Asamar</creatorcontrib><creatorcontrib>Lukens, P</creatorcontrib><creatorcontrib>Mahapatra, R</creatorcontrib><creatorcontrib>Mandic, V</creatorcontrib><creatorcontrib>Mast, N</creatorcontrib><creatorcontrib>Mayer, A J</creatorcontrib><creatorcontrib>H Meyer zu Theenhausen</creatorcontrib><creatorcontrib>Michaud, É M</creatorcontrib><creatorcontrib>Michielin, E</creatorcontrib><creatorcontrib>Mirabolfathi, N</creatorcontrib><creatorcontrib>Mohanty, B</creatorcontrib><creatorcontrib>Morales Mendoza, J D</creatorcontrib><creatorcontrib>Nagorny, S</creatorcontrib><creatorcontrib>Nelson, J</creatorcontrib><creatorcontrib>Neog, H</creatorcontrib><creatorcontrib>Novati, V</creatorcontrib><creatorcontrib>Orrell, J L</creatorcontrib><creatorcontrib>Oser, S M</creatorcontrib><creatorcontrib>Page, W A</creatorcontrib><creatorcontrib>Partridge, R</creatorcontrib><creatorcontrib>Podviianiuk, R</creatorcontrib><creatorcontrib>Ponce, F</creatorcontrib><creatorcontrib>Poudel, S</creatorcontrib><creatorcontrib>Pradeep, A</creatorcontrib><creatorcontrib>Reid, E</creatorcontrib><creatorcontrib>Ren, R</creatorcontrib><creatorcontrib>Reynolds, T</creatorcontrib><creatorcontrib>Saab, T</creatorcontrib><creatorcontrib>Sadoulet, B</creatorcontrib><creatorcontrib>Sander, J</creatorcontrib><creatorcontrib>Sattari, A</creatorcontrib><creatorcontrib>Schnee, R W</creatorcontrib><creatorcontrib>Scorza, S</creatorcontrib><creatorcontrib>Serfass, B</creatorcontrib><creatorcontrib>Sincavage, D J</creatorcontrib><creatorcontrib>Street, J</creatorcontrib><creatorcontrib>Verma, S</creatorcontrib><creatorcontrib>Villano, A N</creatorcontrib><creatorcontrib>B von Krosigk</creatorcontrib><creatorcontrib>Watkins, S L</creatorcontrib><creatorcontrib>Wilson, J S</creatorcontrib><creatorcontrib>Wilson, M J</creatorcontrib><creatorcontrib>Winchell, J</creatorcontrib><creatorcontrib>Wright, D H</creatorcontrib><creatorcontrib>Yellin, S</creatorcontrib><creatorcontrib>Young, B A</creatorcontrib><creatorcontrib>Yu, T C</creatorcontrib><creatorcontrib>Zhang, E</creatorcontrib><creatorcontrib>Zhang, H G</creatorcontrib><creatorcontrib>Zhao, X</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>ProQuest Central (New)</collection><collection>ProQuest One Academic (New)</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Middle East (New)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Applied & Life Sciences</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Collaboration, SuperCDMS</au><au>Alkhatib, I</au><au>Aralis, T</au><au>Aramaki, T</au><au>Arnquist, I J</au><au>I Ataee Langroudy</au><au>Azadbakht, E</au><au>Barker, D</au><au>Bathurst, C</au><au>Bauer, D A</au><au>Bezerra, L V S</au><au>Bhattacharyya, R</au><au>Bowles, M A</au><au>Brink, P L</au><au>Cabrera, B</au><au>Calkins, R</au><au>Cerdeño, D G</au><au>Y -Y Chang</au><au>Chaudhuri, M</au><au>Chen, R</au><au>Chott, N</au><au>Cooley, J</au><au>Coombes, H</au><au>Corbett, J</au><au>di Vacri, M L</au><au>Diamond, M D</au><au>Fascione, E</au><au>Figueroa-Feliciano, E</au><au>Fink, C W</au><au>Fritts, M</au><au>Gerbier, G</au><au>Germond, R</au><au>Ghaith, M</au><au>Golwala, S R</au><au>Harris, H R</au><au>Hines, B A</au><au>Hollister, M I</au><au>Hong, Z</au><au>Hoppe, E W</au><au>Hsu, L</au><au>Huber, M E</au><au>Iyer, V</au><au>Jardin, D</au><au>Jastram, A</au><au>Kelsey, M H</au><au>Kubik, A</au><au>Kurinsky, N A</au><au>Lawrence, R E</au><au>A Li</au><au>Loer, B</au><au>E Lopez Asamar</au><au>Lukens, P</au><au>Mahapatra, R</au><au>Mandic, V</au><au>Mast, N</au><au>Mayer, A J</au><au>H Meyer zu Theenhausen</au><au>Michaud, É M</au><au>Michielin, E</au><au>Mirabolfathi, N</au><au>Mohanty, B</au><au>Morales Mendoza, J D</au><au>Nagorny, S</au><au>Nelson, J</au><au>Neog, H</au><au>Novati, V</au><au>Orrell, J L</au><au>Oser, S M</au><au>Page, W A</au><au>Partridge, R</au><au>Podviianiuk, R</au><au>Ponce, F</au><au>Poudel, S</au><au>Pradeep, A</au><au>Reid, E</au><au>Ren, R</au><au>Reynolds, T</au><au>Saab, T</au><au>Sadoulet, B</au><au>Sander, J</au><au>Sattari, A</au><au>Schnee, R W</au><au>Scorza, S</au><au>Serfass, B</au><au>Sincavage, D J</au><au>Street, J</au><au>Verma, S</au><au>Villano, A N</au><au>B von Krosigk</au><au>Watkins, S L</au><au>Wilson, J S</au><au>Wilson, M J</au><au>Winchell, J</au><au>Wright, D H</au><au>Yellin, S</au><au>Young, B A</au><au>Yu, T C</au><au>Zhang, E</au><au>Zhang, H G</au><au>Zhao, X</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Constraints on Lightly Ionizing Particles from CDMSlite</atitle><jtitle>arXiv.org</jtitle><date>2022-02-19</date><risdate>2022</risdate><eissn>2331-8422</eissn><abstract>The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) achieved efficient detection of very small recoil energies in its germanium target, resulting in sensitivity to Lightly Ionizing Particles (LIPs) in a previously unexplored region of charge, mass, and velocity parameter space. We report first direct-detection limits calculated using the optimum interval method on the vertical intensity of cosmogenically-produced LIPs with an electric charge smaller than \(e/(3\times10^5\)), as well as the strongest limits for charge \(\leq e/160\), with a minimum vertical intensity of \(1.36\times10^{-7}\)\,cm\(^{-2}\)s\(^{-1}\)sr\(^{-1}\) at charge \(e/160\). These results apply over a wide range of LIP masses (5\,MeV/\(c^2\) to 100\,TeV/\(c^2\)) and cover a wide range of \(\beta\gamma\) values (0.1 -- \(10^6\)), thus excluding non-relativistic LIPs with \(\beta\gamma\) as small as 0.1 for the first time.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2011.09183</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2022-02 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_arxiv_primary_2011_09183 |
| source | arXiv.org; Free E- Journals |
| subjects | Dark matter Germanium Physics - Cosmology and Nongalactic Astrophysics Physics - High Energy Astrophysical Phenomena Physics - High Energy Physics - Experiment Physics - High Energy Physics - Phenomenology Physics - Instrumentation and Detectors Recoil |
| title | Constraints on Lightly Ionizing Particles from CDMSlite |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-20T16%3A37%3A55IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Constraints%20on%20Lightly%20Ionizing%20Particles%20from%20CDMSlite&rft.jtitle=arXiv.org&rft.au=Collaboration,%20SuperCDMS&rft.date=2022-02-19&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2011.09183&rft_dat=%3Cproquest_arxiv%3E2462302995%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2462302995&rft_id=info:pmid/&rfr_iscdi=true |