| Literature DB >> 35179913 |
R Abbasi1, M Ackermann2, J Adams3, J A Aguilar4, M Ahlers5, M Ahrens6, C Alispach7, A A Alves8, N M Amin9, R An10, K Andeen11, T Anderson12, G Anton13, C Argüelles10, Y Ashida14, S Axani15, X Bai16, A Balagopal V14, A Barbano7, S W Barwick17, B Bastian2, V Basu14, S Baur4, R Bay18, J J Beatty19,20, K-H Becker21, J Becker Tjus22, C Bellenghi23, S BenZvi24, D Berley25, E Bernardini2, D Z Besson26, G Binder18,27, D Bindig21, E Blaufuss25, S Blot2, M Boddenberg28, F Bontempo8, J Borowka28, S Böser29, O Botner30, J Böttcher28, E Bourbeau5, F Bradascio2, J Braun14, S Bron7, J Brostean-Kaiser2, S Browne31, A Burgman30, R T Burley32, R S Busse33, M A Campana34, E G Carnie-Bronca32, C Chen35, Z Chen36, D Chirkin14, K Choi37, B A Clark38, K Clark39, L Classen33, A Coleman9, G H Collin15, J M Conrad15, P Coppin40, P Correa40, D F Cowen41,12, R Cross24, C Dappen28, P Dave35, C De Clercq40, J J DeLaunay42, H Dembinski9, K Deoskar6, A Desai14, P Desiati14, K D de Vries40, G de Wasseige40, M de With43, T DeYoung38, S Dharani28, A Diaz15, J C Díaz-Vélez14, M Dittmer33, H Dujmovic8, M Dunkman12, M A DuVernois14, E Dvorak16, T Ehrhardt29, P Eller23, R Engel8,31, H Erpenbeck28, J Evans25, P A Evenson9, K L Fan25, A R Fazely44, N Feigl43, S Fiedlschuster13, A T Fienberg12, K Filimonov18, C Finley6, L Fischer2, D Fox41, A Franckowiak22,2, E Friedman25, A Fritz29, P Fürst28, T K Gaisser9, J Gallagher45, E Ganster28, A Garcia10, S Garrappa2, L Gerhardt27, A Ghadimi42, C Glaser30, T Glauch23, T Glüsenkamp13, J G Gonzalez9, S Goswami42, D Grant38, T Grégoire12, S Griswold24, M Gündüz22, C Günther28, C Haack23, A Hallgren30, R Halliday38, L Halve28, F Halzen14, M Ha Minh23, K Hanson14, J Hardin14, A A Harnisch38, A Haungs8, S Hauser28, D Hebecker43, K Helbing21, F Henningsen23, E C Hettinger38, S Hickford21, J Hignight46, C Hill47, G C Hill32, K D Hoffman25, R Hoffmann21, T Hoinka48, B Hokanson-Fasig14, K Hoshina14, F Huang12, M Huber23, T Huber8, K Hultqvist6, M Hünnefeld48, R Hussain14, S In37, N Iovine4, A Ishihara47, M Jansson6, G S Japaridze49, M Jeong37, B J P Jones50, D Kang8, W Kang37, X Kang34, A Kappes33, D Kappesser29, T Karg2, M Karl23, A Karle14, U Katz13, M Kauer14, M Kellermann28, J L Kelley14, A Kheirandish12, K Kin47, T Kintscher2, J Kiryluk36, S R Klein18,27, R Koirala9, H Kolanoski43, T Kontrimas23, L Köpke29, C Kopper38, S Kopper42, D J Koskinen5, P Koundal8, M Kovacevich34, M Kowalski43,2, T Kozynets5, E Kun22, N Kurahashi34, N Lad2, C Lagunas Gualda2, J L Lanfranchi12, M J Larson25, F Lauber21, J P Lazar10,14, J W Lee37, K Leonard14, A Leszczyńska31, Y Li12, M Lincetto22, Q R Liu14, M Liubarska46, E Lohfink29, C J Lozano Mariscal33, L Lu14, F Lucarelli7, A Ludwig38,51, W Luszczak14, Y Lyu18,27, W Y Ma2, J Madsen14, K B M Mahn38, Y Makino14, S Mancina14, I C Mariş4, R Maruyama52, K Mase47, T McElroy46, F McNally53, J V Mead5, K Meagher14, S Mechbal2, A Medina20, M Meier47, S Meighen-Berger23, J Micallef38, D Mockler4, T Montaruli7, R W Moore46, R Morse14, M Moulai15, R Naab2, R Nagai47, U Naumann21, J Necker2, L V Nguyễn38, H Niederhausen23, M U Nisa38, S C Nowicki38, A Obertacke Pollmann21, M Oehler8, B Oeyen54, A Olivas25, E O'Sullivan30, H Pandya9, D V Pankova12, N Park39, G K Parker50, E N Paudel9, L Paul11, C Pérez de Los Heros30, L Peters28, J Peterson14, S Philippen28, D Pieloth48, S Pieper21, M Pittermann31, A Pizzuto14, M Plum11, Y Popovych29, A Porcelli54, M Prado Rodriguez14, P B Price18, B Pries38, G T Przybylski27, C Raab4, A Raissi3, M Rameez5, K Rawlins55, I C Rea23, A Rehman9, P Reichherzer22, R Reimann28, G Renzi4, E Resconi23, S Reusch2, W Rhode48, M Richman34, B Riedel14, E J Roberts32, S Robertson18,27, G Roellinghoff37, M Rongen29, C Rott56,37, T Ruhe48, D Ryckbosch54, D Rysewyk Cantu38, I Safa10,14, J Saffer31, S E Sanchez Herrera38, A Sandrock48, J Sandroos29, M Santander42, S Sarkar46, S Sarkar46, K Satalecka2, M Scharf28, M Schaufel28, H Schieler8, S Schindler13, P Schlunder48, T Schmidt25, A Schneider14, J Schneider13, F G Schröder8,9, L Schumacher23, G Schwefer28, S Sclafani34, D Seckel9, S Seunarine58, A Sharma30, S Shefali31, M Silva14, B Skrzypek10, B Smithers50, R Snihur14, J Soedingrekso48, D Soldin9, C Spannfellner23, G M Spiczak58, C Spiering2, J Stachurska2, M Stamatikos20, T Stanev9, R Stein2, J Stettner28, A Steuer29, T Stezelberger27, T Stürwald21, T Stuttard5, G W Sullivan25, I Taboada35, F Tenholt22, S Ter-Antonyan44, S Tilav9, F Tischbein28, K Tollefson38, L Tomankova22, C Tönnis59, S Toscano4, D Tosi14, A Trettin2, M Tselengidou13, C F Tung35, A Turcati23, R Turcotte8, C F Turley12, J P Twagirayezu38, B Ty14, M A Unland Elorrieta33, N Valtonen-Mattila30, J Vandenbroucke14, N van Eijndhoven40, D Vannerom15, J van Santen2, S Verpoest54, C Walck6, T B Watson50, C Weaver38, P Weigel15, A Weindl8, M J Weiss12, J Weldert29, C Wendt14, J Werthebach48, M Weyrauch31, N Whitehorn38,51, C H Wiebusch28, D R Williams42, M Wolf23, K Woschnagg18, G Wrede13, J Wulff22, X W Xu44, J P Yanez46, S Yoshida47, S Yu38, T Yuan14, Z Zhang36.
Abstract
We present an all-sky 90% confidence level upper limit on the cosmic flux of relativistic magnetic monopoles using 2886 days of IceCube data. The analysis was optimized for monopole speeds between 0.750c and 0.995c, without any explicit restriction on the monopole mass. We constrain the flux of relativistic cosmic magnetic monopoles to a level below 2.0×10^{-19} cm^{-2} s^{-1} sr^{-1} over the majority of the targeted speed range. This result constitutes the most strict upper limit to date for magnetic monopoles with β≳0.8 and up to β∼0.995 and fills the gap between existing limits on the cosmic flux of nonrelativistic and ultrarelativistic magnetic monopoles.Entities:
Year: 2022 PMID： 35179913 DOI： 10.1103/PhysRevLett.128.051101
Source DB: PubMed Journal: Phys Rev Lett ISSN： 0031-9007 Impact factor: 9.161