Could a multi-PeV neutrino event have as origin the internal shocks inside the GRB progenitor star?

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• 作者：N. Fraija¹ ; ^{nifraija@astro.unam.mx" class="auth_mail" title="E-mail the corresponding author}
• 关键词：Gamma-ray burst ; General - stars ; Interiors - stars ; Jets - neutrinos
• 刊名：Journal of High Energy Astrophysics
• 出版年：2016
• 出版时间：March-June 2016
• 年：2016
• 卷：9-10
• 期：Complete
• 页码：25-34
• 全文大小：1515 K

文摘

The IceCube Collaboration initially reported the detection of 37 extraterrestrial neutrinos in the TeV–PeV energy range. The reconstructed neutrino events were obtained during three consecutive years of data taking, from 2010 to 2013. Although these events have been discussed to have an extragalactic origin, they have not been correlated to any known source. Recently, the IceCube Collaboration reported a neutrino-induced muon event with energy of 07aec0c0be38ee2288" title="Click to view the MathML source">2.6±0.3$2.6\pm 0.3$ PeV which corresponds to the highest event ever detected. Neither the reconstructed direction of this event (J2000.0), detected on June 11 2014 at R.A.=110°.34$\text{R.A.}=110\mathrm{°}.34$, Dec.=11°.48$\text{Dec.}=11\mathrm{°}.48$ matches with any familiar source. Long gamma-ray bursts (lGRBs) are usually associated with the core collapse of massive stars leading relativistic-collimated jets inside stars with high-energy neutrino production. These neutrinos have been linked to the 37 events previously detected by IceCube experiment. In this work, we explore the conditions and values of parameters so that the highest neutrino recently detected could be generated by proton–photon and proton–hadron interactions at internal shocks inside lGRB progenitor star and then detected in IceCube experiment. Considering that internal shocks take place in a relativistic collimated jet, whose (half) opening angle is θ₀∼0.1${\theta }_0\sim 0.1$, we found that lGRBs with total luminosity 0593a2" title="Click to view the MathML source">L≲10⁴⁸$L\lesssim {10}^{48}$ erg/s and internal shocks on the surface of progenitors such as Wolf–Rayet (WR) and blue super giant (BSG) stars favor this multi-PeV neutrino production, although this neutrino could be associated with L∼10^50.5$L\sim {10}^{50.5}$ (∼10⁵⁰$\sim {10}^{50}$) erg/s provided that the internal shocks occur at ∼10⁹$\sim {10}^9$(∼10^10.2) cm$(\sim {10}^{10.2})\text{cm}$ for a WR (BSG).