Skipper-CCD Sensors for the Oscura Experiment: Requirements and Preliminary Tests

Fuente: arXiv
Salvato in:
Dettagli Bibliografici
Autori principali: Cervantes-Vergara, Brenda A., Perez, Santiago, Estrada, Juan, Botti, Ana, Chavez, Claudio R., Chierchie, Fernando, Saffold, Nathan, Aguilar-Arevalo, Alexis, Alcalde-Bessia, Fabricio, Avalos, Nicolás, Baez, Oscar, Baxter, Daniel, Bertou, Xavier, Bonifazi, Carla, Cancelo, Gustavo, Castelló-Mor, Nuria, Chavarria, Alvaro E., De Egea, Juan Manuel, D'Olivo, Juan Carlos, Dreyer, Cyrus, Drlica-Wagner, Alex, Essig, Rouven, Estrada, Ezequiel, Etzion, Erez, Grylls, Paul, Fernandez-Moroni, Guillermo, Fernández-Serra, Marivi, Ferreyra, Santiago, Holland, Stephen, Barreda, Agustín Lantero, Lathrop, Andrew, Lawson, Ian, Loer, Ben, Luoma, Steffon, Villalpando, Edgar Marrufo, Montero, Mauricio Martinez, McGuire, Kellie, Molina, Jorge, Munagavalasa, Sravan, Norcini, Danielle, Piers, Alexander, Privitera, Paolo, Rodrigues, Dario, Saldanha, Richard, Singal, Aman, Smida, Radomir, Sofo-Haro, Miguel, Stalder, Diego, Stefanazzi, Leandro, Tiffenberg, Javier, Traina, Michelangelo, Uemura, Sho, Ventura, Pedro, Cortabitarte, Rocío Vilar, Yajur, Rachana
Natura: Preprint
Pubblicazione: 2023
Soggetti:
Accesso online:
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
_version_ 1866911835124400128
author Cervantes-Vergara, Brenda A.
Perez, Santiago
Estrada, Juan
Botti, Ana
Chavez, Claudio R.
Chierchie, Fernando
Saffold, Nathan
Aguilar-Arevalo, Alexis
Alcalde-Bessia, Fabricio
Avalos, Nicolás
Baez, Oscar
Baxter, Daniel
Bertou, Xavier
Bonifazi, Carla
Cancelo, Gustavo
Castelló-Mor, Nuria
Chavarria, Alvaro E.
De Egea, Juan Manuel
D'Olivo, Juan Carlos
Dreyer, Cyrus
Drlica-Wagner, Alex
Essig, Rouven
Estrada, Ezequiel
Etzion, Erez
Grylls, Paul
Fernandez-Moroni, Guillermo
Fernández-Serra, Marivi
Ferreyra, Santiago
Holland, Stephen
Barreda, Agustín Lantero
Lathrop, Andrew
Lawson, Ian
Loer, Ben
Luoma, Steffon
Villalpando, Edgar Marrufo
Montero, Mauricio Martinez
McGuire, Kellie
Molina, Jorge
Munagavalasa, Sravan
Norcini, Danielle
Piers, Alexander
Privitera, Paolo
Rodrigues, Dario
Saldanha, Richard
Singal, Aman
Smida, Radomir
Sofo-Haro, Miguel
Stalder, Diego
Stefanazzi, Leandro
Tiffenberg, Javier
Traina, Michelangelo
Uemura, Sho
Ventura, Pedro
Cortabitarte, Rocío Vilar
Yajur, Rachana
author_facet Cervantes-Vergara, Brenda A.
Perez, Santiago
Estrada, Juan
Botti, Ana
Chavez, Claudio R.
Chierchie, Fernando
Saffold, Nathan
Aguilar-Arevalo, Alexis
Alcalde-Bessia, Fabricio
Avalos, Nicolás
Baez, Oscar
Baxter, Daniel
Bertou, Xavier
Bonifazi, Carla
Cancelo, Gustavo
Castelló-Mor, Nuria
Chavarria, Alvaro E.
De Egea, Juan Manuel
D'Olivo, Juan Carlos
Dreyer, Cyrus
Drlica-Wagner, Alex
Essig, Rouven
Estrada, Ezequiel
Etzion, Erez
Grylls, Paul
Fernandez-Moroni, Guillermo
Fernández-Serra, Marivi
Ferreyra, Santiago
Holland, Stephen
Barreda, Agustín Lantero
Lathrop, Andrew
Lawson, Ian
Loer, Ben
Luoma, Steffon
Villalpando, Edgar Marrufo
Montero, Mauricio Martinez
McGuire, Kellie
Molina, Jorge
Munagavalasa, Sravan
Norcini, Danielle
Piers, Alexander
Privitera, Paolo
Rodrigues, Dario
Saldanha, Richard
Singal, Aman
Smida, Radomir
Sofo-Haro, Miguel
Stalder, Diego
Stefanazzi, Leandro
Tiffenberg, Javier
Traina, Michelangelo
Uemura, Sho
Ventura, Pedro
Cortabitarte, Rocío Vilar
Yajur, Rachana
contents Oscura is a proposed multi-kg skipper-CCD experiment designed for a dark matter (DM) direct detection search that will reach unprecedented sensitivity to sub-GeV DM-electron interactions with its 10 kg detector array. Oscura is planning to operate at SNOLAB with 2070 m overburden, and aims to reach a background goal of less than one event in each electron bin in the 2-10 electron ionization-signal region for the full 30 kg-year exposure, with a radiation background rate of 0.01 dru. In order to achieve this goal, Oscura must address each potential source of background events, including instrumental backgrounds. In this work, we discuss the main instrumental background sources and the strategy to control them, establishing a set of constraints on the sensors' performance parameters. We present results from the tests of the first fabricated Oscura prototype sensors, evaluate their performance in the context of the established constraints and estimate the Oscura instrumental background based on these results.
format Preprint
id arxiv_https___arxiv_org_abs_2304_04401
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Skipper-CCD Sensors for the Oscura Experiment: Requirements and Preliminary Tests
Cervantes-Vergara, Brenda A.
Perez, Santiago
Estrada, Juan
Botti, Ana
Chavez, Claudio R.
Chierchie, Fernando
Saffold, Nathan
Aguilar-Arevalo, Alexis
Alcalde-Bessia, Fabricio
Avalos, Nicolás
Baez, Oscar
Baxter, Daniel
Bertou, Xavier
Bonifazi, Carla
Cancelo, Gustavo
Castelló-Mor, Nuria
Chavarria, Alvaro E.
De Egea, Juan Manuel
D'Olivo, Juan Carlos
Dreyer, Cyrus
Drlica-Wagner, Alex
Essig, Rouven
Estrada, Ezequiel
Etzion, Erez
Grylls, Paul
Fernandez-Moroni, Guillermo
Fernández-Serra, Marivi
Ferreyra, Santiago
Holland, Stephen
Barreda, Agustín Lantero
Lathrop, Andrew
Lawson, Ian
Loer, Ben
Luoma, Steffon
Villalpando, Edgar Marrufo
Montero, Mauricio Martinez
McGuire, Kellie
Molina, Jorge
Munagavalasa, Sravan
Norcini, Danielle
Piers, Alexander
Privitera, Paolo
Rodrigues, Dario
Saldanha, Richard
Singal, Aman
Smida, Radomir
Sofo-Haro, Miguel
Stalder, Diego
Stefanazzi, Leandro
Tiffenberg, Javier
Traina, Michelangelo
Uemura, Sho
Ventura, Pedro
Cortabitarte, Rocío Vilar
Yajur, Rachana
Instrumentation and Detectors
Oscura is a proposed multi-kg skipper-CCD experiment designed for a dark matter (DM) direct detection search that will reach unprecedented sensitivity to sub-GeV DM-electron interactions with its 10 kg detector array. Oscura is planning to operate at SNOLAB with 2070 m overburden, and aims to reach a background goal of less than one event in each electron bin in the 2-10 electron ionization-signal region for the full 30 kg-year exposure, with a radiation background rate of 0.01 dru. In order to achieve this goal, Oscura must address each potential source of background events, including instrumental backgrounds. In this work, we discuss the main instrumental background sources and the strategy to control them, establishing a set of constraints on the sensors' performance parameters. We present results from the tests of the first fabricated Oscura prototype sensors, evaluate their performance in the context of the established constraints and estimate the Oscura instrumental background based on these results.
title Skipper-CCD Sensors for the Oscura Experiment: Requirements and Preliminary Tests
topic Instrumentation and Detectors
url https://arxiv.org/abs/2304.04401