'Waxman 03' presentation slideshows

UHECRs & GRBs

UHECRs & GRBs. Eli Waxman Weizmann Institute, ISRAEL. The acceleration challenge. v. R. /G. B. v. 2R. G 2. G 2. l =R/ G. (d t RF =R/ G c). [Hillas, ARA&A (1984); Waxman 04]. The suspects. Active Galactic Nuclei (steady): G ~ few requires L>10 47 erg/s Few, brightest AGN

269 views • 18 slides