Charles D. Dermer et al 2007 ApJ 664 L67 doi:10.1086/520638
Charles D. Dermer1, Enrico Ramirez-Ruiz2 and Truong Le1
Show affiliationsRelativistic black hole jet sources are leading candidates for high-energy (
TeV) neutrino production. The relations defining (1) efficient photopion losses of cosmic-ray protons on target photons and (2) γγ opacity of γ-rays through that same target photon field imply clear multiwavelength predictions for when and at what energies blazars and gamma-ray bursts should be most neutrino-bright and γ-ray-dim. The use of multiwavelength observations to test the standard relativistic jet model for these source is illustrated.
black hole physics; galaxies: jets; gamma rays: bursts; neutrinos; radiation mechanisms: non-thermal
Issue 2 (2007 August 1)
Received 2007 May 11, accepted for publication 2007 June 5
Published 2007 July 11
Charles D. Dermer et al 2007 ApJ 664 L67
Rémi Carles et al 2008 Nonlinearity 21 2569
Christian Röver et al 2006 Class. Quantum Grav. 23 4895
Federico Finkel et al 1999 J. Phys. A: Math. Gen. 32 6821
Erik Olsson and Kourosh Tatar 2006 Meas. Sci. Technol. 17 2843
B J Powell et al 2003 J. Phys.: Condens. Matter 15 L235
Antônio J R da Silva et al 2004 J. Phys.: Condens. Matter 16 8243
Neil P Oxtoby et al 2003 J. Phys.: Condens. Matter 15 8055
J H NamKoong and S H Lim 2009 J. Phys. D: Appl. Phys. 42 225003
Cao Feng et al 2009 Chinese Phys. Lett. 26 114203