Zobrazeno 1 - 10
of 45
pro vyhledávání: '"Loer, Ben"'
Autor:
Fowler, Joseph W., Szypryt, Paul, Bunker, Raymond, Edwards, Ellen R., Florang, Ian Fogarty, Gao, Jiansong, Giachero, Andrea, Hoogerheide, Shannon F., Loer, Ben, Mumm, H. Pieter, Nakamura, Nathan, O'Neil, Galen C., Orrell, John L., Scott, Elizabeth M., Stevens, Jason, Swetz, Daniel S., VanDevender, Brent A., Vissers, Michael, Ullom, Joel N.
Naturally occurring background radiation is a source of correlated decoherence events in superconducting qubits that will challenge error-correction schemes. To characterize the radiation environment in an unshielded laboratory, we performed broadban
Externí odkaz:
http://arxiv.org/abs/2404.10866
Autor:
Chou, Aaron, Irwin, Kent, Maruyama, Reina H., Baker, Oliver K., Bartram, Chelsea, Berggren, Karl K., Cancelo, Gustavo, Carney, Daniel, Chang, Clarence L., Cho, Hsiao-Mei, Garcia-Sciveres, Maurice, Graham, Peter W., Habib, Salman, Harnik, Roni, Harris, J. G. E., Hertel, Scott A., Hume, David B., Khatiwada, Rakshya, Kovachy, Timothy L., Kurinsky, Noah, Lamoreaux, Steve K., Lehnert, Konrad W., Leibrandt, David R., Li, Dale, Loer, Ben, Martínez-Rincón, Julián, McCuller, Lee, Moore, David C., Mueller, Holger, Pena, Cristian, Pooser, Raphael C., Pyle, Matt, Rajendran, Surjeet, Safronova, Marianna S., Schuster, David I., Shaw, Matthew D., Spiropulu, Maria, Stankus, Paul, Sushkov, Alexander O., Winslow, Lindley, Xie, Si, Zurek, Kathryn M.
Strong motivation for investing in quantum sensing arises from the need to investigate phenomena that are very weakly coupled to the matter and fields well described by the Standard Model. These can be related to the problems of dark matter, dark sec
Externí odkaz:
http://arxiv.org/abs/2311.01930
Radioactive decays from ^{42}Ar and its progeny ^{42}K are potential background sources in large-scale liquid-argon-based neutrino and dark matter experiments. In the atmosphere, ^{42}Ar is produced primarily by cosmogenic activation on ^{40}Ar. The
Externí odkaz:
http://arxiv.org/abs/2309.16169
Autor:
Perez, Santiago, Rodrigues, Dario, Estrada, Juan, Harnik, Roni, Liu, Zhen, Cervantes-Vergara, Brenda A., D'Olivo, Juan Carlos, Plestid, Ryan D., Tiffenberg, Javier, Yu, Tien-Tien, Aguilar-Arevalo, Alexis, Alcalde-Bessia, Fabricio, Avalos, Nicolas, Baez, Oscar, Baxter, Daniel, Bertou, Xavier, Bonifazi, Carla, Botti, Ana, Cancelo, Gustavo, Castelló-Mor, Nuria, Chavarria, Alvaro E., Chavez, Claudio R., Chierchie, Fernando, De Egea, Juan Manuel, 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, Saffold, Nathan, Saldanha, Richard, Singal, Aman, Smida, Radomir, Sofo-Haro, Miguel, Stalder, Diego, Stefanazzi, Leandro, Traina, Michelangelo, Tsai, Yu-Dai, Uemura, Sho, Ventura, Pedro, Cortabitarte, Rocío Vilar, Yajur, Rachana
Oscura is a planned light-dark matter search experiment using Skipper-CCDs with a total active mass of 10 kg. As part of the detector development, the collaboration plans to build the Oscura Integration Test (OIT), an engineering test with 10% of the
Externí odkaz:
http://arxiv.org/abs/2304.08625
Autor:
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
Publikováno v:
Journal of Instrumentation, Volume 18, August 2023
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
Externí odkaz:
http://arxiv.org/abs/2304.04401
Autor:
Beck, Douglas, Carlson, Joseph, Davoudi, Zohreh, Formaggio, Joseph, Quaglioni, Sofia, Savage, Martin, Barata, Joao, Bhattacharya, Tanmoy, Bishof, Michael, Cloet, Ian, Delgado, Andrea, DeMarco, Michael, Fink, Caleb, Florio, Adrien, Francois, Marianne, Grabowska, Dorota, Hoogerheide, Shannon, Huang, Mengyao, Ikeda, Kazuki, Illa, Marc, Joo, Kyungseon, Kharzeev, Dmitri, Kowalski, Karol, Lai, Wai Kin, Leach, Kyle, Loer, Ben, Low, Ian, Martin, Joshua, Moore, David, Mehen, Thomas, Mueller, Niklas, Mulligan, James, Mumm, Pieter, Pederiva, Francesco, Pisarski, Rob, Ploskon, Mateusz, Reddy, Sanjay, Rupak, Gautam, Singh, Hersh, Singh, Maninder, Stetcu, Ionel, Stryker, Jesse, Szypryt, Paul, Valgushev, Semeon, VanDevender, Brent, Watkins, Samuel, Wilson, Christopher, Yao, Xiaojun, Afanasev, Andrei, Balantekin, Akif Baha, Baroni, Alessandro, Bunker, Raymond, Chakraborty, Bipasha, Chernyshev, Ivan, Cirigliano, Vincenzo, Clark, Benjamin, Dhiman, Shashi Kumar, Du, Weijie, Dutta, Dipangkar, Edwards, Robert, Flores, Abraham, Galindo-Uribarri, Alfredo, Ruiz, Ronald Fernando Garcia, Gueorguiev, Vesselin, Guo, Fanqing, Hansen, Erin, Hernandez, Hector, Hattori, Koichi, Hauke, Philipp, Hjorth-Jensen, Morten, Jankowski, Keith, Johnson, Calvin, Lacroix, Denis, Lee, Dean, Lin, Huey-Wen, Liu, Xiaohui, Llanes-Estrada, Felipe J., Looney, John, Lukin, Misha, Mercenne, Alexis, Miller, Jeff, Mottola, Emil, Mueller, Berndt, Nachman, Benjamin, Negele, John, Orrell, John, Patwardhan, Amol, Phillips, Daniel, Poole, Stephen, Qualters, Irene, Rumore, Mike, Schaefer, Thomas, Scott, Jeremy, Singh, Rajeev, Vary, James, Galvez-Viruet, Juan-Jose, Wendt, Kyle, Xing, Hongxi, Yang, Liang, Young, Glenn, Zhao, Fanyi
In preparation for the 2023 NSAC Long Range Plan (LRP), members of the Nuclear Science community gathered to discuss the current state of, and plans for further leveraging opportunities in, QIST in NP research at the Quantum Information Science for U
Externí odkaz:
http://arxiv.org/abs/2303.00113
Autor:
Cooley, Jodi, Lin, Tongyan, Lippincott, W. Hugh, Slatyer, Tracy R., Yu, Tien-Tien, Akerib, Daniel S., Aramaki, Tsuguo, Baxter, Daniel, Bringmann, Torsten, Bunker, Ray, Carney, Daniel, Cebrián, Susana, Chen, Thomas Y., Cushman, Priscilla, Dahl, C. E., Essig, Rouven, Fan, Alden, Gaitskell, Richard, Galbiati, Cristano, Gelmini, Graciela B., Giovanetti, Graham K., Giroux, Guillaume, Grandi, Luca, Harding, J. Patrick, Haselschwardt, Scott, Hsu, Lauren, Horiuchi, Shunsaku, Kahn, Yonatan, Kim, Doojin, Kim, Geon-Bo, Kravitz, Scott, Kudryavtsev, V. A., Kurinsky, Noah, Lang, Rafael F., Leane, Rebecca K., Lehmann, Benjamin V., Levy, Cecilia, Li, Shengchao, Loer, Ben, Manalaysay, Aaron, Martoff, C. J, Mohlabeng, Gopolang, Monzani, M. E., Murphy, Alexander St J., Neilson, Russell, Nelson, Harry N., O'Hare, Ciaran A. J., Palladino, K. J., Parikh, Aditya, Park, Jong-Chul, Perez, Kerstin, Profumo, Stefano, Raj, Nirmal, Roach, Brandon M., Saab, Tarek, Sarsa, Maria Luísa, Schnee, Richard, Shaw, Sally, Shin, Seodong, Sinha, Kuver, Stifter, Kelly, Suzuki, Aritoki, Szydagis, M., Tait, Tim M. P., Takhistov, Volodymyr, Tsai, Yu-Dai, Vahsen, S. E., Vitagliano, Edoardo, von Doetinchem, Philip, Wang, Gensheng, Westerdale, Shawn, Williams, David A., Xiang, Xin, Yang, Liang
This report summarizes the findings of the CF1 Topical Subgroup to Snowmass 2021, which was focused on particle dark matter. One of the most important scientific goals of the next decade is to reveal the nature of dark matter (DM). To accomplish this
Externí odkaz:
http://arxiv.org/abs/2209.07426
Autor:
Wilson, Jonathan S., Theenhausen, Hanno Meyer zu, von Krosigk, Belina, Azadbakht, Elham, Bunker, Ray, Hall, Jeter, Hansen, Sten, Hines, Bruce, Loer, Ben, Olsen, Jamieson T., Oser, Scott M., Partridge, Richard, Pyle, Matthew, Sander, Joel, Serfass, Bruno, Toback, David, Watkins, Samuel L., Zhao, Xuji
Publikováno v:
2022 JINST 17 P07010
The SuperCDMS SNOLAB dark matter search experiment aims to be sensitive to energy depositions down to O(1 eV). This imposes requirements on the resolution, signal efficiency, and noise rejection of the trigger system. To accomplish this, the SuperCDM
Externí odkaz:
http://arxiv.org/abs/2204.13002
Autor:
SuperCDMS Collaboration, Al-Bakry, Musaab, Alkhatib, Imran, Amaral, Dorian Praia do, Aralis, Taylor, Aramaki, Tsuguo, Arnquist, Isaac, Langroudy, Iman Ataee, Azadbakht, Elham, Banik, Samir, Bathurst, Corey, Bauer, Dan, Bezerra, Lucas, Bhattacharyya, Rik, Brink, Paul, Bunker, Ray, Cabrera, Blas, Calkins, Robert, Cameron, Robert, Cartaro, Concetta, Cerdeno, David, Chang, Yen-Yung, Chaudhuri, Mouli, Chen, Ran, Chott, Nicholas, Cooley, Jodi, Coombes, Harrison, Corbett, Jonathan, Cushman, Priscilla, De Brienne, François, Dharani, Sukeerthi, di Vacri, Maria Laura, Diamond, Miriam, Fascione, Eleanor, Figueroa, Enectali, Fink, Caleb, Fouts, Ken, Fritts, Matt, Gerbier, Gilles, Germond, Richard, Ghaith, Muad, Golwala, Sunil, Hall, Jeter, Hassan, Noah, Hines, Bruce, Hollister, Matt, Hong, Ziqing, Hoppe, Eric, Hsu, Lauren, Huber, Martin, Iyer, Vijay, Jardin, Daniel, Jastram, Andrew, Kashyap, Varchaswi, Kelsey, Michael, Kubik, Andrew, Kurinsky, Noah, Lawrence, Richard, Lee, Matthew, Li, Ashley, Liu, Jasmine, Liu, Yan, Loer, Ben, Lukens, Pat, MacFarlane, David, Mahapatra, Rupak, Mandic, Vuk, Mast, Nicholas, Mayer, Adam, Theenhausen, Hanno Meyer zu, Michaud, Émile, Michielin, Emanuele, Mirabolfathi, Nader, Mohanty, Bedangadas, Nagorny, Serge, Nelson, Jack, Neog, Himangshu, Novati, Valentina, Orrell, John, Osborne, McKay, Oser, Scott, Page, William, Partridge, Richard, Pedreros, David S., Podviianiuk, Ruslan, Ponce, Francisco, Poudel, Sudip, Pradeep, Aditi, Pyle, Matt, Rau, Wolfgang, Reid, Elliott, Ren, Tom, Reynolds, Tyler, Roberts, Amy, Robinson, Alan, Saab, Tarek, Sadoulet, Bernard, Saikia, Ishwita, Sander, Joel, Sattari, Ata, Schmidt, Benjamin, Schnee, Richard, Scorza, Silvia, Serfass, Bruno, Poudel, Sagar Sharma, Sincavage, Derek, Stanford, Chris, Street, Joseph, Sun, Huanbo, Thasrawala, Fatema, Toback, David, Underwood, Ryan, Verma, Shubham, Villano, Anthony, von Krosigk, Belina, Watkins, Samuel, Wen, Osmond, Williams, Zachary, Wilson, Matthew, Winchell, Joshua, Wu, Chih-pan, Wykoff, Kevin, Yellin, Steve, Young, Betty, Yu, To Chin, Zatschler, Birgit, Zatschler, Stefan, Zaytsev, Alexander, Zhang, Enze, Zheng, Lei, Zuber, Summer
In this paper, we present a re-analysis of SuperCDMS data using a profile likelihood approach to search for sub-GeV dark matter particles (DM) through two inelastic scattering channels: bremsstrahlung radiation and the Migdal effect. By considering p
Externí odkaz:
http://arxiv.org/abs/2203.02594
Autor:
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
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
Externí odkaz:
http://arxiv.org/abs/2202.10518