Zobrazeno 1 - 10
of 158
pro vyhledávání: '"Baudis, Laura"'
Autor:
Baudis, Laura
The DARWIN/XLZD experiment is a next-generation dark matter detector with a multi-ten-ton liquid xenon time projection chamber at its core. Its principal goal will be to explore the experimentally accessible parameter space for Weakly Interacting Mas
Externí odkaz:
http://arxiv.org/abs/2404.19524
Autor:
Bajpai, Dhanurdhar, Baudis, Laura, Belov, Viacheslav, Bossio, Elisabetta, Cocolios, Thomas E., Ejiri, Hiroyasu, Sushenok, Evgenii, Fomina, Maria, Hashim, Izyan H., Heines, Michael, Gusev, Konstantin, Kazartsev, Sergej, Knecht, Andreas, Mondragon, Elizabeth, Wei, Ng Zheng, Othman, Faiznur, Ostrovskiy, Igor, Araujo, Gabriela R., Rumyantseva, Nadyia, Schwarz, Mario, Schoenert, Stefan, Shirchenko, Mark, Shevchik, Egor, Shitov, Yury, Suhonen, Jouni, Vogiatzi, Stergiani M., Wiesinger, Christoph, Zhitnikov, Igor, Zinatulina, Daniya
The MONUMENT experiment measures ordinary muon capture (OMC) on isotopes relevant for neutrinoless double-beta (0$\nu\beta\beta$) decay and nuclear astrophysics. OMC is a particularly attractive tool for improving the theoretical description of 0$\nu
Externí odkaz:
http://arxiv.org/abs/2404.12686
Autor:
Baudis, Laura
Publikováno v:
Phil. Trans. R. Soc. A382 (2023) 0083
In the past decade, dual-phase xenon time projection chambers (Xe-TPCs) have emerged as some of the most powerful detectors in the fields of astroparticle physics and rare-event searches. Developed primarily towards the direct detection of dark matte
Externí odkaz:
http://arxiv.org/abs/2311.05320
Autor:
Baum, Sebastian, Stengel, Patrick, Abe, Natsue, Acevedo, Javier F., Araujo, Gabriela R., Asahara, Yoshihiro, Avignone, Frank, Balogh, Levente, Baudis, Laura, Boukhtouchen, Yilda, Bramante, Joseph, Breur, Pieter Alexander, Caccianiga, Lorenzo, Capozzi, Francesco, Collar, Juan I., Ebadi, Reza, Edwards, Thomas, Eitel, Klaus, Elykov, Alexey, Ewing, Rodney C., Freese, Katherine, Fung, Audrey, Galelli, Claudio, Glasmacher, Ulrich A., Gleason, Arianna, Hasebe, Noriko, Hirose, Shigenobu, Horiuchi, Shunsaku, Hoshino, Yasushi, Huber, Patrick, Ido, Yuki, Igami, Yohei, Ishikawa, Norito, Itow, Yoshitaka, Kamiyama, Takashi, Kato, Takenori, Kavanagh, Bradley J., Kawamura, Yoji, Kazama, Shingo, Kenney, Christopher J., Kilminster, Ben, Kouketsu, Yui, Kozaka, Yukiko, Kurinsky, Noah A., Leybourne, Matthew, Lucas, Thalles, McDonough, William F., Marshall, Mason C., Mateos, Jose Maria, Mathur, Anubhav, Michibayashi, Katsuyoshi, Mkhonto, Sharlotte, Murase, Kohta, Naka, Tatsuhiro, Oguni, Kenji, Rajendran, Surjeet, Sakane, Hitoshi, Sala, Paola, Scholberg, Kate, Semenec, Ingrida, Shiraishi, Takuya, Spitz, Joshua, Sun, Kai, Suzuki, Katsuhiko, Tanin, Erwin H., Vincent, Aaron, Vladimirov, Nikita, Walsworth, Ronald L., Watanabe, Hiroko
Publikováno v:
Phys.Dark Univ. 41 (2023) 101245
Minerals are solid state nuclear track detectors - nuclear recoils in a mineral leave latent damage to the crystal structure. Depending on the mineral and its temperature, the damage features are retained in the material from minutes (in low-melting
Externí odkaz:
http://arxiv.org/abs/2301.07118
Autor:
Butler, Joel N., Chivukula, R. Sekhar, de Gouvêa, André, Han, Tao, Kim, Young-Kee, Cushman, Priscilla, Farrar, Glennys R., Kolomensky, Yury G., Nagaitsev, Sergei, Yunes, Nicolás, Gourlay, Stephen, Raubenheimer, Tor, Shiltsev, Vladimir, Assamagan, Kétévi A., Quinn, Breese, Elvira, V. Daniel, Gottlieb, Steven, Nachman, Benjamin, Chou, Aaron S., Soares-Santos, Marcelle, Tait, Tim M. P., Narain, Meenakshi, Reina, Laura, Tricoli, Alessandro, Barbeau, Phillip S., Merkel, Petra, Zhang, Jinlong, Huber, Patrick, Scholberg, Kate, Worcester, Elizabeth, Artuso, Marina, Bernstein, Robert H., Petrov, Alexey A., Craig, Nathaniel, Csáki, Csaba, El-Khadra, Aida X., Baudis, Laura, Hall, Jeter, Lesko, Kevin T., Orrell, John L., Gonski, Julia, Psihas, Fernanda, Simon, Sara M.
The 2021-22 High-Energy Physics Community Planning Exercise (a.k.a. ``Snowmass 2021'') was organized by the Division of Particles and Fields of the American Physical Society. Snowmass 2021 was a scientific study that provided an opportunity for the e
Externí odkaz:
http://arxiv.org/abs/2301.06581
The decade since Snowmass 2013 has seen extraordinary progress of high energy physics research performed--or planned for--at underground facilities. Drs. T. Kajita and A.B. McDonald were awarded the 2015 Nobel Prize in Physics for the discovery of ne
Externí odkaz:
http://arxiv.org/abs/2211.13450
Autor:
Alfonso, Krystal, Araujo, Gabriela R., Baudis, Laura, Bowden, Nathaniel, Cogswell, Bernadette K., Erickson, Anna, Galloway, Michelle, Hecht, Adam A., Mudiyanselage, Rathsara R. H. Herath, Huber, Patrick, Jovanovic, Igor, Khodaparast, Giti A., Magill, Brenden A., O'Donnell, Thomas, Smith, Nicholas W. G., Zhang, Xianyi
The PALEOCCENE concept offers the potential for room-temperature, passive and robust detectors in the gram to kilogram range for the detection of low-energy nuclear recoil events. Nuclear recoil events can be caused by neutron scattering, coherent el
Externí odkaz:
http://arxiv.org/abs/2203.05525
Publikováno v:
Eur. Phys. J. C 81, 1060 (2021)
Detectors using liquid xenon as target are widely deployed in rare event searches. Conclusions on the interacting particle rely on a precise reconstruction of the deposited energy which requires calibrations of the energy scale of the detector by mea
Externí odkaz:
http://arxiv.org/abs/2109.07151
Autor:
GERDA collaboration, Agostini, Matteo, Bakalyarov, Alexander M., Balata, Marco, Barabanov, Igor, Baudis, Laura, Bauer, Christian, Bellotti, Enrico, Belogurov, Sergej, Bettini, Alessandro, Bezrukov, Leonid, Borowicz, Dariusz, Bossio, Elisabetta, Bothe, Vikas, Brudanin, Victor, Brugnera, Riccardo, Caldwell, Allen, Cattadori, Carla, Chernogorov, Andrey, Comellato, Tommaso, D'Andrea, Valerio, Demidova, Elena V., Di Marco, Natalia, Domula, Alexander, Doroshkevich, Evgenyi, Egorov, Viacheslav, Fischer, Felix, Fomina, Maria, Gangapshev, Albert, Garfagnini, Alberto, Gooch, Chris, Grabmayr, Peter, Gurentsov, Valery, Gusev, Konstantin, Hakenmüller, Janina, Hemmer, Sabine, Hiller, Roman, Hofmann, Werner, Hult, Mikael, Inzhechik, Lev V., Csáthy, Jozsef Janicskó, Jochum, Josef, Junker, Matthias, Kazalov, Vladimir, Kermaïdic, Yoann, Kihm, Thomas, Kirpichnikov, Igor V., Klimenko, Alexander, Kneißl, Raphael, Knöpfle, Karl T., Kochetov, Oleg, Kornoukhov, Vasily N., Krause, Patrick, Kuzminov, Valery V., Laubenstein, Matthias, Lazzaro, Andrea, Lindner, Manfred, Lippi, Ivano, Lubashevskiy, Alexey, Lubsandorzhiev, Bayarto, Lutter, Guillaume, Macolino, Carla, Majorovits, Bela, Maneschg, Werner, Miloradovic, Michael, Mingazheva, Rizalina, Misiaszek, Marcin, Moseev, Pavel, Nemchenok, Igor, Panas, Krysztof, Pandola, Luciano, Pelczar, Krysztof, Pertoldi, Luigi, Piseri, Paolo, Pullia, Alberto, Ransom, Chloe, Riboldi, Stefano, Rumyantseva, Nadezda, Sada, Cinzia, Salamida, Francesco, Schönert, Stefan, Schreiner, Jochen, Schütt, Mario, Schütz, Ann-Katrin, Schulz, Oliver, Schwarz, Mario, Schwingenheuer, Bernhard, Selivanenko, Oleg, Shevchik, Egor, Shirchenko, Mark, Simgen, Hardy, Smolnikov, Anatoly, Stukov, Danila, Vanhoefer, Laura, Vasenko, Andrey A., Veresnikova, Anna, Vignoli, Chiara, von Sturm, Katharina, Wester, Thomas, Wiesinger, Christoph, Wojcik, Marcin, Yanovich, Evgeny, Zatschler, Birgit, Zhitnikov, Igor, Zhukov, Sergey V., Zinatulina, Daniya, Zschocke, Andreas, Zsigmond, Anna J., Zuber, Kai, Zuzel, Grzegorz
The GERmanium Detector Array (GERDA) experiment at the Gran Sasso underground laboratory (LNGS) of INFN is searching for neutrinoless double-beta ($0\nu\beta\beta$) decay of $^{76}$Ge. The technological challenge of GERDA is to operate in a "backgrou
Externí odkaz:
http://arxiv.org/abs/1909.02522
Autor:
Bergé, Joel, Baudis, Laura, Brax, Philippe, Chiow, Sheng-wey, Christophe, Bruno, Doré, Olivier, Fayet, Pierre, Hees, Aurélien, Jetzer, Philippe, Lämmerzahl, Claus, List, Meike, Métris, Gilles, Pernot-Borràs, Martin, Read, Justin, Reynaud, Serge, Rhodes, Jason, Rievers, Benny, Rodrigues, Manuel, Sumner, Timothy, Uzan, Jean-Philippe, Yu, Nan
Publikováno v:
Experimental Astronomy (2021) 51:1737-1766
We speculate on the development and availability of new innovative propulsion techniques in the 2040s, that will allow us to fly a spacecraft outside the Solar System (at 150 AU and more) in a reasonable amount of time, in order to directly probe our
Externí odkaz:
http://arxiv.org/abs/1909.00834