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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| Veröffentlicht in: | Physical review letters 2021-08, Vol.127 (8), p.1-081802, Article 081802 |
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| creator | Alkhatib, I. Amaral, D. W. P. Aralis, T. Aramaki, T. Arnquist, I. J. Ataee Langroudy, I. Azadbakht, E. Banik, S. Barker, D. Bathurst, C. Bauer, D. A. Bezerra, L. V. S. Bhattacharyya, R. Bowles, M. A. Brink, P. L. Bunker, R. Cabrera, B. Calkins, R. Cameron, R. A. Cartaro, C. Cerdeño, D. G. Chang, Y.-Y. Chaudhuri, M. Chen, R. Chott, N. Cooley, J. Coombes, H. Corbett, J. Cushman, P. De Brienne, F. di Vacri, M. L. Diamond, M. D. Fascione, E. Figueroa-Feliciano, E. Fink, C. W. Fouts, K. 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. Kashyap, V. K. S. Kelsey, M. H. Kubik, A. Kurinsky, N. A. Lawrence, R. E. Li, A. Loer, B. Lopez Asamar, E. Lukens, P. MacFarlane, D. B. Mahapatra, R. Mandic, V. Mast, N. Mayer, A. J. Meyer zu Theenhausen, H. 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. Pyle, M. Rau, W. Reid, E. Ren, R. Reynolds, T. Roberts, A. Robinson, A. E. Saab, T. Sadoulet, B. Sander, J. Sattari, A. Schnee, R. W. Scorza, S. Serfass, B. Sincavage, D. J. Stanford, C. Street, J. |
| 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 × 105), as well as the strongest limits for charge ≤ e / 160 , with a minimum vertical intensity of 1.36 × 10−7 cm−2 s−1 sr−1 at charge e / 160 . These results apply over a wide range of LIP masses ( 5 MeV / c2 to 100 TeV / c2) and cover a wide range of β γ values ( 0.1 – 106), thus excluding nonrelativistic LIPs with β γ as small as 0.1 for the first time. |
| doi_str_mv | 10.1103/PhysRevLett.127.081802 |
| format | Article |
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W. P. ; Aralis, T. ; Aramaki, T. ; Arnquist, I. J. ; Ataee Langroudy, I. ; Azadbakht, E. ; Banik, S. ; Barker, D. ; Bathurst, C. ; Bauer, D. A. ; Bezerra, L. V. S. ; Bhattacharyya, R. ; Bowles, M. A. ; Brink, P. L. ; Bunker, R. ; Cabrera, B. ; Calkins, R. ; Cameron, R. A. ; Cartaro, C. ; Cerdeño, D. G. ; Chang, Y.-Y. ; Chaudhuri, M. ; Chen, R. ; Chott, N. ; Cooley, J. ; Coombes, H. ; Corbett, J. ; Cushman, P. ; De Brienne, F. ; di Vacri, M. L. ; Diamond, M. D. ; Fascione, E. ; Figueroa-Feliciano, E. ; Fink, C. W. ; Fouts, K. ; 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. ; Kashyap, V. K. S. ; Kelsey, M. H. ; Kubik, A. ; Kurinsky, N. A. ; Lawrence, R. E. ; Li, A. ; Loer, B. ; Lopez Asamar, E. ; Lukens, P. ; MacFarlane, D. B. ; Mahapatra, R. ; Mandic, V. ; Mast, N. ; Mayer, A. J. ; Meyer zu Theenhausen, H. ; Michaud, É. 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D. ; Fascione, E. ; Figueroa-Feliciano, E. ; Fink, C. W. ; Fouts, K. ; 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. ; Kashyap, V. K. S. ; Kelsey, M. H. ; Kubik, A. ; Kurinsky, N. A. ; Lawrence, R. E. ; Li, A. ; Loer, B. ; Lopez Asamar, E. ; Lukens, P. ; MacFarlane, D. B. ; Mahapatra, R. ; Mandic, V. ; Mast, N. ; Mayer, A. J. ; Meyer zu Theenhausen, H. ; 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. ; Pyle, M. ; Rau, W. ; Reid, E. ; Ren, R. ; Reynolds, T. ; Roberts, A. ; Robinson, A. E. ; Saab, T. ; Sadoulet, B. ; Sander, J. ; Sattari, A. ; Schnee, R. W. ; Scorza, S. ; Serfass, B. ; Sincavage, D. J. ; Stanford, C. ; Street, J. ; SuperCDMS Collaboration</creatorcontrib><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 × 105), as well as the strongest limits for charge ≤ e / 160 , with a minimum vertical intensity of 1.36 × 10−7 cm−2 s−1 sr−1 at charge e / 160 . 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J.</creatorcontrib><creatorcontrib>Stanford, C.</creatorcontrib><creatorcontrib>Street, J.</creatorcontrib><creatorcontrib>SuperCDMS Collaboration</creatorcontrib><title>Constraints on Lightly Ionizing Particles from CDMSlite</title><title>Physical review letters</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 × 105), as well as the strongest limits for charge ≤ e / 160 , with a minimum vertical intensity of 1.36 × 10−7 cm−2 s−1 sr−1 at charge e / 160 . These results apply over a wide range of LIP masses ( 5 MeV / c2 to 100 TeV / c2) and cover a wide range of β γ values ( 0.1 – 106), thus excluding nonrelativistic LIPs with β γ as small as 0.1 for the first time.</description><subject>Dark matter</subject><subject>Germanium</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNpd0E1LAzEQgOEgCtbqX5BFL162TjbZTXKU9atQsfhxDtt0tk3ZJpqkQv31bqkH8ZTLQ2bmJeScwohSYNfT5Ta-4NcEUxrRQoxAUgnFARlQECoXlPJDMgBgNFcA4picxLgCAFpUckBE7V1MobEuxcy7bGIXy9Rts7F39tu6RTZtQrKmw5i1wa-z-vbptbMJT8lR23QRz37fIXm_v3urH_PJ88O4vpnkhimaciXLoqkEVxLnMKuwKdqKFablApAaVlYMzBxRcTMzqMRMzlW_WKs4R1GqsmVDcrH_18dkdTT9aLM03jk0SVNJOXDo0dUefQT_ucGY9NpGg13XOPSbqIuyUkwyWbKeXv6jK78Jrj9hp8pKipLLXlV7ZYKPMWCrP4JdN2GrKehddP0nuu6j63109gP4tXZq</recordid><startdate>20210820</startdate><enddate>20210820</enddate><creator>Alkhatib, I.</creator><creator>Amaral, D. W. 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E.</creator><creator>Saab, T.</creator><creator>Sadoulet, B.</creator><creator>Sander, J.</creator><creator>Sattari, A.</creator><creator>Schnee, R. W.</creator><creator>Scorza, S.</creator><creator>Serfass, B.</creator><creator>Sincavage, D. J.</creator><creator>Stanford, C.</creator><creator>Street, J.</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7X8</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0003-1925-0088</orcidid><orcidid>https://orcid.org/0000000319250088</orcidid></search><sort><creationdate>20210820</creationdate><title>Constraints on Lightly Ionizing Particles from CDMSlite</title><author>Alkhatib, I. ; Amaral, D. W. P. ; Aralis, T. ; Aramaki, T. ; Arnquist, I. J. ; Ataee Langroudy, I. ; Azadbakht, E. ; Banik, S. ; Barker, D. ; Bathurst, C. ; Bauer, D. A. ; Bezerra, L. V. S. ; Bhattacharyya, R. ; Bowles, M. A. ; Brink, P. L. ; Bunker, R. ; Cabrera, B. ; Calkins, R. ; Cameron, R. A. ; Cartaro, C. ; Cerdeño, D. G. ; Chang, Y.-Y. ; Chaudhuri, M. ; Chen, R. ; Chott, N. ; Cooley, J. ; Coombes, H. ; Corbett, J. ; Cushman, P. ; De Brienne, F. ; di Vacri, M. L. ; Diamond, M. D. ; Fascione, E. ; Figueroa-Feliciano, E. ; Fink, C. W. ; Fouts, K. ; 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. ; Kashyap, V. K. S. ; Kelsey, M. H. ; Kubik, A. ; Kurinsky, N. A. ; Lawrence, R. E. ; Li, A. ; Loer, B. ; Lopez Asamar, E. ; Lukens, P. ; MacFarlane, D. B. ; Mahapatra, R. ; Mandic, V. ; Mast, N. ; Mayer, A. J. ; Meyer zu Theenhausen, H. ; 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. ; Pyle, M. ; Rau, W. ; Reid, E. ; Ren, R. ; Reynolds, T. ; Roberts, A. ; Robinson, A. E. ; Saab, T. ; Sadoulet, B. ; Sander, J. ; Sattari, A. ; Schnee, R. W. ; Scorza, S. ; Serfass, B. ; Sincavage, D. J. ; Stanford, C. ; Street, J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c391t-9852a67498ed0b6ea2f632cf470e1c35630cdee94cbce97b8d9012f944e7595f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Dark matter</topic><topic>Germanium</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Alkhatib, I.</creatorcontrib><creatorcontrib>Amaral, D. W. P.</creatorcontrib><creatorcontrib>Aralis, T.</creatorcontrib><creatorcontrib>Aramaki, T.</creatorcontrib><creatorcontrib>Arnquist, I. J.</creatorcontrib><creatorcontrib>Ataee Langroudy, I.</creatorcontrib><creatorcontrib>Azadbakht, E.</creatorcontrib><creatorcontrib>Banik, S.</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>Bunker, R.</creatorcontrib><creatorcontrib>Cabrera, B.</creatorcontrib><creatorcontrib>Calkins, R.</creatorcontrib><creatorcontrib>Cameron, R. A.</creatorcontrib><creatorcontrib>Cartaro, C.</creatorcontrib><creatorcontrib>Cerdeño, D. G.</creatorcontrib><creatorcontrib>Chang, Y.-Y.</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>Cushman, P.</creatorcontrib><creatorcontrib>De Brienne, F.</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>Fouts, K.</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>Kashyap, V. K. S.</creatorcontrib><creatorcontrib>Kelsey, M. H.</creatorcontrib><creatorcontrib>Kubik, A.</creatorcontrib><creatorcontrib>Kurinsky, N. A.</creatorcontrib><creatorcontrib>Lawrence, R. E.</creatorcontrib><creatorcontrib>Li, A.</creatorcontrib><creatorcontrib>Loer, B.</creatorcontrib><creatorcontrib>Lopez Asamar, E.</creatorcontrib><creatorcontrib>Lukens, P.</creatorcontrib><creatorcontrib>MacFarlane, D. B.</creatorcontrib><creatorcontrib>Mahapatra, R.</creatorcontrib><creatorcontrib>Mandic, V.</creatorcontrib><creatorcontrib>Mast, N.</creatorcontrib><creatorcontrib>Mayer, A. J.</creatorcontrib><creatorcontrib>Meyer zu Theenhausen, H.</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>Pyle, M.</creatorcontrib><creatorcontrib>Rau, W.</creatorcontrib><creatorcontrib>Reid, E.</creatorcontrib><creatorcontrib>Ren, R.</creatorcontrib><creatorcontrib>Reynolds, T.</creatorcontrib><creatorcontrib>Roberts, A.</creatorcontrib><creatorcontrib>Robinson, A. E.</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>Stanford, C.</creatorcontrib><creatorcontrib>Street, J.</creatorcontrib><creatorcontrib>SuperCDMS Collaboration</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Alkhatib, I.</au><au>Amaral, D. W. P.</au><au>Aralis, T.</au><au>Aramaki, T.</au><au>Arnquist, I. J.</au><au>Ataee Langroudy, I.</au><au>Azadbakht, E.</au><au>Banik, S.</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>Bunker, R.</au><au>Cabrera, B.</au><au>Calkins, R.</au><au>Cameron, R. A.</au><au>Cartaro, C.</au><au>Cerdeño, D. G.</au><au>Chang, Y.-Y.</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>Cushman, P.</au><au>De Brienne, F.</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>Fouts, K.</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>Kashyap, V. K. S.</au><au>Kelsey, M. H.</au><au>Kubik, A.</au><au>Kurinsky, N. A.</au><au>Lawrence, R. E.</au><au>Li, A.</au><au>Loer, B.</au><au>Lopez Asamar, E.</au><au>Lukens, P.</au><au>MacFarlane, D. B.</au><au>Mahapatra, R.</au><au>Mandic, V.</au><au>Mast, N.</au><au>Mayer, A. J.</au><au>Meyer zu Theenhausen, H.</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>Pyle, M.</au><au>Rau, W.</au><au>Reid, E.</au><au>Ren, R.</au><au>Reynolds, T.</au><au>Roberts, A.</au><au>Robinson, A. E.</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>Stanford, C.</au><au>Street, J.</au><aucorp>SuperCDMS Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Constraints on Lightly Ionizing Particles from CDMSlite</atitle><jtitle>Physical review letters</jtitle><date>2021-08-20</date><risdate>2021</risdate><volume>127</volume><issue>8</issue><spage>1</spage><epage>081802</epage><pages>1-081802</pages><artnum>081802</artnum><issn>0031-9007</issn><eissn>1079-7114</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 × 105), as well as the strongest limits for charge ≤ e / 160 , with a minimum vertical intensity of 1.36 × 10−7 cm−2 s−1 sr−1 at charge e / 160 . These results apply over a wide range of LIP masses ( 5 MeV / c2 to 100 TeV / c2) and cover a wide range of β γ values ( 0.1 – 106), thus excluding nonrelativistic LIPs with β γ as small as 0.1 for the first time.</abstract><cop>College Park</cop><pub>American Physical Society</pub><doi>10.1103/PhysRevLett.127.081802</doi><orcidid>https://orcid.org/0000-0003-1925-0088</orcidid><orcidid>https://orcid.org/0000000319250088</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0031-9007 |
| ispartof | Physical review letters, 2021-08, Vol.127 (8), p.1-081802, Article 081802 |
| issn | 0031-9007 1079-7114 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1814040 |
| source | American Physical Society Journals; EZB-FREE-00999 freely available EZB journals |
| subjects | Dark matter Germanium |
| title | Constraints on Lightly Ionizing Particles from CDMSlite |
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