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7. Filaments of galaxies as a clue to the origin of ultrahigh-energy cosmic rays. Kim J; Ryu D; Kang H; Kim S; Rey SC Sci Adv; 2019 Jan; 5(1):eaau8227. PubMed ID: 30613777 [TBL] [Abstract][Full Text] [Related]
8. An extremely energetic cosmic ray observed by a surface detector array. ; Abbasi RU; Allen MG; Arimura R; Belz JW; Bergman DR; Blake SA; Shin BK; Buckland IJ; Cheon BG; Fujii T; Fujisue K; Fujita K; Fukushima M; Furlich GD; Gerber ZR; Globus N; Hibino K; Higuchi R; Honda K; Ikeda D; Ito H; Iwasaki A; Jeong S; Jeong HM; Jui CH; Kadota K; Kakimoto F; Kalashev OE; Kasahara K; Kawata K; Kharuk I; Kido E; Kim SW; Kim HB; Kim JH; Kim JH; Komae I; Kubota Y; Kuznetsov MY; Lee KH; Lubsandorzhiev BK; Lundquist JP; Matthews JN; Nagataki S; Nakamura T; Nakazawa A; Nonaka T; Ogio S; Ono M; Oshima H; Park IH; Potts M; Pshirkov S; Remington JR; Rodriguez DC; Rott C; Rubtsov GI; Ryu D; Sagawa H; Sakaki N; Sako T; Sakurai N; Shin H; Smith JD; Sokolsky P; Stokes BT; Stroman TS; Takahashi K; Takeda M; Taketa A; Tameda Y; Thomas S; Thomson GB; Tinyakov PG; Tkachev I; Tomida T; Troitsky SV; Tsunesada Y; Udo S; Urban FR; Wong T; Yamazaki K; Yuma Y; Zhezher YV; Zundel Z Science; 2023 Nov; 382(6673):903-907. PubMed ID: 37995237 [TBL] [Abstract][Full Text] [Related]
9. Violation of the Greisen-Zatsepin-Kuzmin cutoff: a tempest in a (magnetic) Teapot? Why cosmic ray energies above 10(20) eV may not require new physics. Farrar GR; Piran T Phys Rev Lett; 2000 Apr; 84(16):3527-30. PubMed ID: 11019137 [TBL] [Abstract][Full Text] [Related]
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