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The Oscura Experiment

Authors :
Aguilar-Arevalo, Alexis
Bessia, Fabricio Alcalde
Avalos, Nicolas
Baxter, Daniel
Bertou, Xavier
Bonifazi, Carla
Botti, Ana
Cababie, Mariano
Cancelo, Gustavo
Cervantes-Vergara, Brenda Aurea
Castello-Mor, Nuria
Chavarria, Alvaro
Chavez, Claudio R.
Chierchie, Fernando
De Egea, Juan Manuel
D`Olivo, Juan Carlos
Dreyer, Cyrus E.
Drlica-Wagner, Alex
Essig, Rouven
Estrada, Juan
Estrada, Ezequiel
Etzion, Erez
Fernandez-Moroni, Guillermo
Fernandez-Serra, Marivi
Holland, Steve
Barreda, Agustin Lantero
Lathrop, Andrew
Lipovetzky, Jose
Loer, Ben
Villalpando, Edgar Marrufo
Molina, Jorge
Perez, Santiago
Privitera, Paolo
Rodrigues, Dario
Saldanha, Richard
Cruz, Diego Santa
Singal, Aman
Saffold, Nathan
Stefanazzi, Leandro
Sofo-Haro, Miguel
Tiffenberg, Javier
Torres, Christian
Uemura, Sho
Vilar, Rocio
Aguilar-Arevalo, Alexis
Bessia, Fabricio Alcalde
Avalos, Nicolas
Baxter, Daniel
Bertou, Xavier
Bonifazi, Carla
Botti, Ana
Cababie, Mariano
Cancelo, Gustavo
Cervantes-Vergara, Brenda Aurea
Castello-Mor, Nuria
Chavarria, Alvaro
Chavez, Claudio R.
Chierchie, Fernando
De Egea, Juan Manuel
D`Olivo, Juan Carlos
Dreyer, Cyrus E.
Drlica-Wagner, Alex
Essig, Rouven
Estrada, Juan
Estrada, Ezequiel
Etzion, Erez
Fernandez-Moroni, Guillermo
Fernandez-Serra, Marivi
Holland, Steve
Barreda, Agustin Lantero
Lathrop, Andrew
Lipovetzky, Jose
Loer, Ben
Villalpando, Edgar Marrufo
Molina, Jorge
Perez, Santiago
Privitera, Paolo
Rodrigues, Dario
Saldanha, Richard
Cruz, Diego Santa
Singal, Aman
Saffold, Nathan
Stefanazzi, Leandro
Sofo-Haro, Miguel
Tiffenberg, Javier
Torres, Christian
Uemura, Sho
Vilar, Rocio
Publication Year :
2022

Abstract

The Oscura experiment will lead the search for low-mass dark matter particles using a very large array of novel silicon Charge Coupled Devices (CCDs) with a threshold of two electrons and with a total exposure of 30 kg-yr. The R&D effort, which began in FY20, is currently entering the design phase with the goal of being ready to start construction in late 2024. Oscura will have unprecedented sensitivity to sub-GeV dark matter particles that interact with electrons, probing dark matter-electron scattering for masses down to 500 keV and dark matter being absorbed by electrons for masses down to 1 eV. The Oscura R&D effort has made some significant progress on the main technical challenges of the experiment, of which the most significant are engaging new foundries for the fabrication of the CCD sensors, developing a cold readout solution, and understanding the experimental backgrounds.

Details

Database :
OAIster
Publication Type :
Electronic Resource
Accession number :
edsoai.on1312096540
Document Type :
Electronic Resource