SENSEI at SNOLAB: Single-Electron Event Rate and Implications for Dark Matter

Fuente: arXiv
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Autori principali: Bloch, Itay M., Botti, Ana M., Cababie, Mariano, Cancelo, Gustavo, Cervantes-Vergara, Brenda A., Daal, Miguel, Desai, Ansh, Drlica-Wagner, Alex, Essig, Rouven, Estrada, Juan, Etzion, Erez, Moroni, Guillermo Fernandez, Holland, Stephen E., Kehat, Jonathan, Lawson, Ian, Luoma, Steffon, Orly, Aviv, Perez, Santiago E., Rodrigues, Dario, Saffold, Nathan A., Scorza, Silvia, Sofo-Haro, Miguel, Stifter, Kelly, Tiffenberg, Javier, Uemura, Sho, Villalpando, Edgar Marrufo, Volansky, Tomer, Winkel, Federico, Wu, Yikai, Yu, Tien-Tien
Natura: Preprint
Pubblicazione: 2024
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author Bloch, Itay M.
Botti, Ana M.
Cababie, Mariano
Cancelo, Gustavo
Cervantes-Vergara, Brenda A.
Daal, Miguel
Desai, Ansh
Drlica-Wagner, Alex
Essig, Rouven
Estrada, Juan
Etzion, Erez
Moroni, Guillermo Fernandez
Holland, Stephen E.
Kehat, Jonathan
Lawson, Ian
Luoma, Steffon
Orly, Aviv
Perez, Santiago E.
Rodrigues, Dario
Saffold, Nathan A.
Scorza, Silvia
Sofo-Haro, Miguel
Stifter, Kelly
Tiffenberg, Javier
Uemura, Sho
Villalpando, Edgar Marrufo
Volansky, Tomer
Winkel, Federico
Wu, Yikai
Yu, Tien-Tien
author_facet Bloch, Itay M.
Botti, Ana M.
Cababie, Mariano
Cancelo, Gustavo
Cervantes-Vergara, Brenda A.
Daal, Miguel
Desai, Ansh
Drlica-Wagner, Alex
Essig, Rouven
Estrada, Juan
Etzion, Erez
Moroni, Guillermo Fernandez
Holland, Stephen E.
Kehat, Jonathan
Lawson, Ian
Luoma, Steffon
Orly, Aviv
Perez, Santiago E.
Rodrigues, Dario
Saffold, Nathan A.
Scorza, Silvia
Sofo-Haro, Miguel
Stifter, Kelly
Tiffenberg, Javier
Uemura, Sho
Villalpando, Edgar Marrufo
Volansky, Tomer
Winkel, Federico
Wu, Yikai
Yu, Tien-Tien
contents We present results from data acquired by the SENSEI experiment at SNOLAB after a major upgrade in May 2023, which includes deploying 16 new sensors and replacing the copper trays that house the CCDs with a new light-tight design. We observe a single-electron event rate of $(1.39 \pm 0.11) \times 10^{-5}$ e$^-$/pix/day, corresponding to $(39.8 \pm 3.1)$ e$^-$/gram/day. This is an order-of-magnitude improvement compared to the previous lowest single-electron rate in a silicon detector and the lowest for any photon detector in the near-infrared-ultraviolet range. We use these data to obtain a 90% confidence level upper bound of $1.53 \times 10^{-5}$ e$^-$/pix/day and to set constraints on sub-GeV dark matter candidates that produce single-electron events. We hypothesize that the data taken at SNOLAB in the previous run, with an older tray design for the sensors, contained a larger rate of single-electron events due to light leaks. We test this hypothesis using data from the SENSEI detector located in the MINOS cavern at Fermilab.
format Preprint
id arxiv_https___arxiv_org_abs_2410_18716
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle SENSEI at SNOLAB: Single-Electron Event Rate and Implications for Dark Matter
Bloch, Itay M.
Botti, Ana M.
Cababie, Mariano
Cancelo, Gustavo
Cervantes-Vergara, Brenda A.
Daal, Miguel
Desai, Ansh
Drlica-Wagner, Alex
Essig, Rouven
Estrada, Juan
Etzion, Erez
Moroni, Guillermo Fernandez
Holland, Stephen E.
Kehat, Jonathan
Lawson, Ian
Luoma, Steffon
Orly, Aviv
Perez, Santiago E.
Rodrigues, Dario
Saffold, Nathan A.
Scorza, Silvia
Sofo-Haro, Miguel
Stifter, Kelly
Tiffenberg, Javier
Uemura, Sho
Villalpando, Edgar Marrufo
Volansky, Tomer
Winkel, Federico
Wu, Yikai
Yu, Tien-Tien
Cosmology and Nongalactic Astrophysics
High Energy Physics - Experiment
We present results from data acquired by the SENSEI experiment at SNOLAB after a major upgrade in May 2023, which includes deploying 16 new sensors and replacing the copper trays that house the CCDs with a new light-tight design. We observe a single-electron event rate of $(1.39 \pm 0.11) \times 10^{-5}$ e$^-$/pix/day, corresponding to $(39.8 \pm 3.1)$ e$^-$/gram/day. This is an order-of-magnitude improvement compared to the previous lowest single-electron rate in a silicon detector and the lowest for any photon detector in the near-infrared-ultraviolet range. We use these data to obtain a 90% confidence level upper bound of $1.53 \times 10^{-5}$ e$^-$/pix/day and to set constraints on sub-GeV dark matter candidates that produce single-electron events. We hypothesize that the data taken at SNOLAB in the previous run, with an older tray design for the sensors, contained a larger rate of single-electron events due to light leaks. We test this hypothesis using data from the SENSEI detector located in the MINOS cavern at Fermilab.
title SENSEI at SNOLAB: Single-Electron Event Rate and Implications for Dark Matter
topic Cosmology and Nongalactic Astrophysics
High Energy Physics - Experiment
url https://arxiv.org/abs/2410.18716