Accès ouvert déclaré
2022
conference-paper
Searching for neutrino transients below 1 TeV with IceCube
Michael J Larson, M. Ackermann, Jenni Adams, Juanan Aguilar, M. Ahlers, Maryon Ahrens, Cyril Martin Alispach, A. A. Alves, Najia Moureen Binte Amin, Rui An, K. Andeen, Tyler Anderson, G. Anton, C. Argüelles, Yosuke Ashida, Spencer Axani, X. Bai, Anastasia Maria Barbano, S. W. Barwick, Benjamin Bastian, Vedant Basu, S. Baur, R. C. Bay, J. J. Beatty, Karl H. Becker, Chiara Bellenghi, S. BenZvi, D. Berley, E. Bernardini, D. Z. Besson, G. Binder, D. Bindig, E. Blaufuss, Summer Blot, Matthias Boddenberg, Federico Bontempo, Jürgen Borowka, S. Böser, O. Botner, Etienne Bourbeau, Federica Bradascio, J. Braun, S. Bron, Jannes Brostean-Kaiser, Sally-Ann Browne, A. Burgman, Ryan T. Burley, Raffaela Busse, Michael Campana, Erin Carnie-Bronca, Chujie Chen, D. Chirkin, K. Choi, Bryanlee Clark, Kenneth L. Clark, Lew Classen, Alan Coleman, Gabriel Collin, J. M. Conrad, Paul Coppin, Pablo Correa, D. F. Cowen, R. Cross, Christian Dappen, Pranav Dave, C. De Clercq, James DeLaunay, H.-P. Dembinski, Kunal Deoskar, Sam De Ridder, Abhishek Desai, P. Desiati, Meike De With, T. DeYoung, Sukeerthi Dharani, A. Diaz, J. C. Díaz–Vélez, Markus Dittmer, Hrvoje Dujmović, M. Dunkman, M. A. DuVernois, Emily Dvorak, Thomas Ehrhardt, P. Eller, Ralph Engel, Hannah Erpenbeck, John Evans, P.A. Evenson, Kwok Lung Fan, A. R. Fazely, Sebastian Fiedlschuster, Aaron Fienberg, Kirill Filimonov, C. Finley, Leander Fischer, D. B. Fox, A. Franckowiak, Elizabeth Friedman, Alexander Fritz, Philipp Fürst, T. K. Gaisser, J. S. Gallagher, Erik Ganster, Alfonso García, S. Garrappa, L. Gerhardt, Christian Gläser, Theo Glauch, Thorsten Glusenkamp, A. Goldschmidt, J. E. Gonzalez, Sreetama Goswami, Darren Grant, T. Grégoire, Spencer Griswold, Mehmet Gündüz, Christoph Günther, Christian Haack, Allan Hallgren, R. Halliday, L. Halve, F. Halzen, Kael Hanson, John Hardin, Alexander Harnisch, A. Haungs, Simon Hauser, D. Hebecker, K. Helbing, Felix Henningsen, Emma C. Hettinger, Stephanie Hickford, Joshua Hignight, Colton Hill, G. C. Hill, Kara Hoffman, R. Hoffmann, Tobias Hoinka, Benjamin Hokanson-Fasig, K. Hoshina, Feifei Huang, Matthias Huber, Thomas S. Huber, K. Hultqvist, Mirco Hünnefeld, Raamis Hussain, Seongjin In, N. Iovine, A. Ishihara, Matti Jansson, George Japaridze, Minjin Jeong, B. J. P. Jones, Donghwa Kang, Woosik Kang, Xinyue Kang, A. Kappes, David Kappesser, T. Karg, Martina Karl, A. Karle, U. Katz, M. Kauer, Moritz Kellermann, J. L. Kelley, Ali Kheirandish, Ken'ichi Kin, T. Kintscher, J. Kiryluk, Ramesh Koirala, H. Kolanoski, Tomas Kontrimas, L. Köpke, Claudio Kopper, Sandro Kopper, D. J. Koskinen, Paras Koundal, Michael Kovacevich, M. Kowalski, Tetiana Kozynets, Emma Kun, Neha Navnitkumar Lad, J. L. Lanfranchi, Frederik Hermann Lauber, Jeffrey Lazar, Jiwoong Lee, Agnieszka Leszczyńska, Yijia Li, Massimiliano Lincetto, Qinrui Liu, Maria Liubarska, Elisa Lohfink, L. Lu, Francesco Lucarelli, Andrew Ludwig, William Luszczak, Yang Lyu, W. Y., J. Madsen, K. B. M. Mahn, Yuya Makino, Sarah Mancina, Ioana Codrina Mariş, R. Maruyama, K. Mase, Thomas McElroy, Frank McNally, J. V. Mead, Kieron Meagher, Andrés Medina, Maximilian Meier, S. Meighen-Berger, Jessie Micallef, D. Mockler, T. Montaruli, R. W. Moore, R. Morse, Marjon Moulai, Richard Naab, R. Nagai, Uwe Naumann, Jannis Necker, Le Viet Nguyen, Hans Niederhausen, M. U. Nisa, Sarah Nowicki, Dave Nygren, Marie Oehler, A. Olivas, Erin O’Sullivan, Hershal Pandya, D. V. Pankova, Nahee Park, Grant Parker, Ek Narayan Paudel, Larissa Paul, Lilly Peters, Josh Peterson, Saskia Philippen, D. Pieloth, Sarah Pieper, Martin Pittermann, A. Pizzuto, M. Plum, Yuiry Popovych, Alessio Porcelli, P. B. Price, B. Pries, G. T. Przybylski, Christoph Raab, Amirreza Raissi, M. Rameez, K. Rawlins, I. C. Rea, Abdul Rehman, Patrick Reichherzer, R. Reimann, Giovanni Renzi, E. Resconi, Simeon Reusch, W. Rhode, Mike Richman, Benedikt Riedel, Ella Roberts, Sally Robertson, Gerrit Roellinghoff, Martin Rongen, C. Rott, T. Ruhe, D. Ryckbosch, I. Safa, Julian Saffer, Alexander Sandrock, J. Sandroos, M. Santander, S. Sarkar, Sourav Sarkar, K. Satalecka, Maximilian Karl Scharf, Merlin Schaufel, H. Schieler, Sebastian Schindler, P. Schlunder, Torsten Schmidt, A. Schneider, Judith Schneider, Frank Schröder, L. Schumacher, Georg Schwefer, D. Seckel, S. Seunarine, Ankur Sharma, Manuel Silva, Barbara Skrzypek, Ben Smithers, Robert Snihur, Jan Soedingrekso, Dennis Soldin, Christian Spannfellner, G. M. Spiczak, Christian Spiering, Juliana Stachurska, M. Stamatikos, Robert Stein, J. Stettner, A. Steuer, T. Stezelberger, Timo Stürwald, Thomas Stuttard, G. W. Sullivan, I. Taboada, F. Tenholt, S. Ter–Antonyan, S. Tilav, Franziska Tischbein, Kirsten Tollefson, Lenka Tomankova, Christoph Tönnis, S. Toscano, Delia Tosi, Alexander Trettin, Maria Tselengidou, C. F. Tung, A. Turcati, Roxanne Turcotte, Colin Turley, Jean Pierre Twagirayezu, Bunheng Ty, Nora Valtonen-Mattila, J. Vandenbroucke, D. Vannerom, Stef Verpoest, M. Vraeghe, C. Walck, Timothyblake Watson, Chris Weaver, Philip Weigel, Andreas Weindl, Matthew J. Weiss, Jan Weldert, Chris Wendt, Johannes Werthebach, Mark Weyrauch, N. Whitehorn, C. H. Wiebusch, Dawn Williams, Martin Wolf, K. Woschnagg, Gerrit Wrede, Johan Wilfried Wulff, Xianwu Xu, Yiqian Xu, Juan Pablo Yáñez, S. Yoshida, Shiqi Yu, Tianlu Yuan, Zelong Zhang
2Citations signalées — pas une note de qualité
19Institutions déclarées
7Pays d’affiliation déclarés
Résumé fourni par la source
Recent observations of GeV gamma-rays from novae have led to a paradigm shift in the understanding of these objects. While it is now believed that shocks contribute significantly to the energy budget of novae, it is still unknown if the emission is hadronic or leptonic in origin. Neutrinos could hold the key to definitively differentiating between these two scenarios, though the energies of such particles would be much lower than are typically targeted with neutrino telescopes. IceCube's densely instrumented DeepCore sub-array provides the ability to reduce the threshold for observation from 1 TeV down to approximately 10 GeV. We will discuss recent measurements in this low energy regime, details of a new sub-TeV selection, and prospects for future searches for transient neutrino emission.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
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Institutions déclarées
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Sujets associés
Astrophysics and Cosmic PhenomenaRadio Astronomy Observations and TechnologyNeutrino Physics Research