Skip to main content
Download PDF
- Main
Search for GeV neutrino emission during intense gamma-ray solar flares with the IceCube Neutrino Observatory
- Abbasi, R;
- Ackermann, M;
- Adams, J;
- Aguilar, JA;
- Ahlers, M;
- Ahrens, M;
- Alispach, C;
- Alves, AA;
- Amin, NM;
- An, R;
- Andeen, K;
- Anderson, T;
- Ansseau, I;
- Anton, G;
- Argüelles, C;
- Axani, S;
- Bai, X;
- V., A Balagopal;
- Barbano, A;
- Barwick, SW;
- Bastian, B;
- Basu, V;
- Baum, V;
- Baur, S;
- Bay, R;
- Beatty, JJ;
- Becker, K-H;
- Tjus, J Becker;
- Bellenghi, C;
- BenZvi, S;
- Berley, D;
- Bernardini, E;
- Besson, DZ;
- Binder, G;
- Bindig, D;
- Blaufuss, E;
- Blot, S;
- Böser, S;
- Botner, O;
- Böttcher, J;
- Bourbeau, E;
- Bourbeau, J;
- Bradascio, F;
- Braun, J;
- Bron, S;
- Brostean-Kaiser, J;
- Burgman, A;
- Busse, RS;
- Campana, MA;
- Chen, C;
- Chirkin, D;
- Choi, S;
- Clark, BA;
- Clark, K;
- Classen, L;
- Coleman, A;
- Collin, GH;
- Conrad, JM;
- Coppin, P;
- Correa, P;
- Cowen, DF;
- Cross, R;
- Dave, P;
- De Clercq, C;
- DeLaunay, JJ;
- Dembinski, H;
- Deoskar, K;
- De Ridder, S;
- Desai, A;
- Desiati, P;
- de Vries, KD;
- de Wasseige, G;
- de With, M;
- DeYoung, T;
- Dharani, S;
- Diaz, A;
- Vélez, JC Díaz;
- Dujmovic, H;
- Dunkman, M;
- DuVernois, MA;
- Dvorak, E;
- Ehrhardt, T;
- Eller, P;
- Engel, R;
- Evans, J;
- Evenson, PA;
- Fahey, S;
- Fazely, AR;
- Fiedlschuster, S;
- Fienberg, AT;
- Filimonov, K;
- Finley, C;
- Fischer, L;
- Fox, D;
- Franckowiak, A;
- Friedman, E;
- Fritz, A;
- Fürst, P;
- Gaisser, TK;
- Gallagher, J;
- Ganster, E;
- Garrappa, S;
- Gerhardt, L;
- Ghadimi, A;
- Glaser, C;
- Glauch, T;
- Glüsenkamp, T;
- Goldschmidt, A;
- Gonzalez, JG;
- Goswami, S;
- Grant, D;
- Grégoire, T;
- Griffith, Z;
- Griswold, S;
- Gündüz, M;
- Haack, C;
- Hallgren, A;
- Halliday, R;
- Halve, L;
- Halzen, F;
- Minh, M Ha;
- Hanson, K;
- Hardin, J;
- Harnisch, AA;
- Haungs, A;
- Hauser, S;
- Hebecker, D;
- Helbing, K;
- Henningsen, F;
- Hettinger, EC;
- Hickford, S;
- Hignight, J;
- Hill, C;
- Hill, GC;
- Hoffman, KD;
- Hoffmann, R;
- Hoinka, T;
- Hokanson-Fasig, B;
- Hoshina, K;
- Huang, F;
- Huber, M;
- Huber, T;
- Hultqvist, K;
- Hünnefeld, M;
- Hussain, R;
- In, S;
- Iovine, N;
- Ishihara, A;
- Jansson, M;
- Japaridze, GS;
- Jeong, M;
- Jones, BJP;
- Joppe, R;
- Kang, D;
- Kang, W;
- Kang, X;
- Kappes, A;
- Kappesser, D;
- Karg, T;
- Karl, M;
- Karle, A;
- Katz, U;
- Kauer, M;
- Kellermann, M;
- Kelley, JL;
- Kheirandish, A;
- Kim, J;
- Kin, K;
- Kintscher, T;
- Kiryluk, J;
- Klein, SR;
- Koirala, R;
- Kolanoski, H;
- Köpke, L;
- Kopper, C;
- Kopper, S;
- Koskinen, DJ;
- Koundal, P;
- Kovacevich, M;
- Kowalski, M;
- Krings, K;
- Krückl, G;
- Kurahashi, N;
- Kyriacou, A;
- Gualda, C Lagunas;
- Lanfranchi, JL;
- Larson, MJ;
- Lauber, F;
- Lazar, JP;
- Leonard, K;
- Leszczyńska, A;
- Li, Y;
- Liu, QR;
- Lohfink, E;
- Mariscal, CJ Lozano;
- Lu, L;
- Lucarelli, F;
- Ludwig, A;
- Luszczak, W;
- Lyu, Y;
- Y., W;
- Madsen, J;
- Mahn, KBM;
- Makino, Y;
- Mallik, P;
- Mancina, S;
- Mariş, IC;
- Maruyama, R;
- Mase, K;
- McNally, F;
- Meagher, K;
- Medina, A;
- Meier, M;
- Meighen-Berger, S;
- Merz, J;
- Micallef, J;
- Mockler, D;
- Momenté, G;
- Montaruli, T;
- Moore, RW;
- Morse, R;
- Moulai, M;
- Naab, R;
- Nagai, R;
- Naumann, U;
- Necker, J;
- Nguyễn, LV;
- Niederhausen, H;
- Nisa, MU;
- Nowicki, SC;
- Nygren, DR;
- Pollmann, A Obertacke;
- Oehler, M;
- Olivas, A;
- O’Sullivan, E;
- Pandya, H;
- Pankova, DV;
- Park, N;
- Parker, GK;
- Paudel, EN;
- Peiffer, P;
- de los Heros, C Pérez;
- Philippen, S;
- Pieloth, D;
- Pieper, S;
- Pizzuto, A;
- Plum, M;
- Popovych, Y;
- Porcelli, A;
- Rodriguez, M Prado;
- Price, PB;
- Pries, B;
- Przybylski, GT;
- Raab, C;
- Raissi, A;
- Rameez, M;
- Rawlins, K;
- Rea, IC;
- Rehman, A;
- Reimann, R;
- Renschler, M;
- Renzi, G;
- Resconi, E;
- Reusch, S;
- Rhode, W;
- Richman, M;
- Riedel, B;
- Robertson, S;
- Roellinghoff, G;
- Rongen, M;
- Rott, C;
- Ruhe, T;
- Ryckbosch, D;
- Cantu, D Rysewyk;
- Safa, I;
- Herrera, SE Sanchez;
- Sandrock, A;
- Sandroos, J;
- Santander, M;
- Sarkar, S;
- Sarkar, S;
- Satalecka, K;
- Scharf, M;
- Schaufel, M;
- Schieler, H;
- Schlunder, P;
- Schmidt, T;
- Schneider, A;
- Schneider, J;
- Schröder, FG;
- Schumacher, L;
- Sclafani, S;
- Seckel, D;
- Seunarine, S;
- Sharma, A;
- Shefali, S;
- Silva, M;
- Skrzypek, B;
- Smithers, B;
- Snihur, R;
- Soedingrekso, J;
- Soldin, D;
- Spiczak, GM;
- Spiering, C;
- Stachurska, J;
- Stamatikos, M;
- Stanev, T;
- Stein, R;
- Stettner, J;
- Steuer, A;
- Stezelberger, T;
- Stokstad, RG;
- Stuttard, T;
- Sullivan, GW;
- Taboada, I;
- Tenholt, F;
- Ter-Antonyan, S;
- Tilav, S;
- Tischbein, F;
- Tollefson, K;
- Tomankova, L;
- Tönnis, C;
- Toscano, S;
- Tosi, D;
- Trettin, A;
- Tselengidou, M;
- Tung, CF;
- Turcati, A;
- Turcotte, R;
- Turley, CF;
- Twagirayezu, JP;
- Ty, B;
- Elorrieta, MA Unland;
- Valtonen-Mattila, N;
- Vandenbroucke, J;
- van Eijk, D;
- van Eijndhoven, N;
- Vannerom, D;
- van Santen, J;
- Verpoest, S;
- Vraeghe, M;
- Walck, C;
- Wallace, A;
- Watson, TB;
- Weaver, C;
- Weindl, A;
- Weiss, MJ;
- Weldert, J;
- Wendt, C;
- Werthebach, J;
- Weyrauch, M;
- Whelan, BJ;
- Whitehorn, N;
- Wiebe, K;
- Wiebusch, CH;
- Williams, DR;
- Wolf, M;
- Woschnagg, K;
- Wrede, G;
- Wulff, J;
- Xu, XW;
- Xu, Y;
- Yanez, JP;
- Yoshida, S;
- Yuan, T;
- Zhang, Z
- et al.
Published Web Location
https://doi.org/10.1103/physrevd.103.102001Abstract
Solar flares convert magnetic energy into thermal and nonthermal plasma energy, the latter implying particle acceleration of charged particles such as protons. Protons are injected out of the coronal acceleration region and can interact with dense plasma in the lower solar atmosphere, producing mesons that subsequently decay into gamma rays and neutrinos at O(MeV-GeV) energies. We present the results of the first search for GeV neutrinos emitted during solar flares carried out with the IceCube Neutrino Observatory. While the experiment was originally designed to detect neutrinos with energies between 10 GeV and a few PeV, a new approach allowing for a O(GeV) energy threshold will be presented. The resulting limits allow us to constrain some of the theoretical estimates of the expected neutrino flux.
Many UC-authored scholarly publications are freely available on this site because of the UC's open access policies. Let us know how this access is important for you.
Main Content
For improved accessibility of PDF content, download the file to your device.
Enter the password to open this PDF file:
File name:
-
File size:
-
Title:
-
Author:
-
Subject:
-
Keywords:
-
Creation Date:
-
Modification Date:
-
Creator:
-
PDF Producer:
-
PDF Version:
-
Page Count:
-
Page Size:
-
Fast Web View:
-
Preparing document for printing…
0%