ملخص
The origin of high-energy neutrinos (0.1-1 PeV range) detected by IceCube remains a mystery. In this work, we explore the possibility that efficient neutrino production can occur in structured jets of BL Lac objects, characterized by a fast inner spine surrounded by a slower layer. This scenario has been widely discussed in the framework of the high-energy emission models for BL Lac objects and radio galaxies. One of the relevant consequences of a velocity structure is the enhancement of the inverse Compton emission caused by the radiative coupling of the two zones. We show that a similar boosting could occur for the neutrino output of the spine through the photo-meson reaction of high-energy protons scattering off the amplified soft target photon field of the layer. Assuming the local density and the cosmological evolution of γ-ray BL Lac object derived from Fermi Large Area Telescope data, we calculate the expected diffuse neutrino intensity, which can match the IceCube data for a reasonable choice of parameters.
| اللغة الأصلية | الإنجليزيّة |
|---|---|
| رقم المقال | L18 |
| دورية | Astrophysical Journal Letters |
| مستوى الصوت | 793 |
| رقم الإصدار | 1 |
| المعرِّفات الرقمية للأشياء | |
| حالة النشر | نُشِر - 20 سبتمبر 2014 |
| منشور خارجيًا | نعم |
بصمة
أدرس بدقة موضوعات البحث “STRUCTURED JETS IN BL LAC OBJECTS: EFFICIENT PeV NEUTRINO FACTORIES? Efficient PeV neutrino factories?'. فهما يشكلان معًا بصمة فريدة.قم بذكر هذا
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