GeV - PeV Neutrino Production and Oscillation in hidden jets from GRBs

Abstract

Long gamma-ray bursts have been widely associated with collapsing massive stars in the framework of collapsar model. High-energy neutrinos and photons can be produced in the internal shocks of middle relativistic jets from core-collapse supernova. Although photons can hardly escape, high-energy neutrinos could be the only signature when the jets are hidden. We show that using suitable parameters, high-energy neutrinos in GeV - PeV range can be produced in the hidden jet inside the collapsar, thus demonstrating that these objects are candidates to produce neutrinos with energies between 1 - 10 PeV which were observed with IceCube. On the other hand, due to matter effects, high-energy neutrinos may oscillate resonantly from one flavor to another before leaving the star. Using two (solar, atmospheric and accelerator parameters) and three neutrino mixing, we study the possibility of resonant oscillation for these neutrinos created in internal shocks. Also we compute the probabilities of neutrino oscillations in the matter at different distances along the jet (before leaving the star) and after in vacuum, on their path to Earth. Finally, neutrino flavor ratios on Earth are estimated.

MNRAS, accepted

References in corpus (11)

• Phenomenology with Massive Neutrinos
• Measurement of Neutrino Oscillation by the K2K Experiment
• Revealing the Supernova--Gamma-Ray Burst Connection with TeV Neutrinos
• High-energy Cosmic Rays and Neutrinos from Semi-relativistic Hypernovae
• Neutrino Spectra from Low and High Luminosity Populations of Gamma Ray Bursts
• Expected neutrino signal from supernova remnant RX J1713.7-3946 and flavor oscillations
• High energy neutrinos from a slow jet model of core collapse supernovae
• Oscillation effects on high-energy neutrino fluxes from astrophysical hidden sources
• Neutrinos from active black holes, sources of ultra high energy cosmic rays
• Inverse Compton cooling in Klein-Nishina regime and GRB prompt spectrum
• Searches for high-energy neutrino emission in the Galaxy with the combined IceCube-AMANDA detector

Cited by in corpus (41)

• Spectral analysis of the high-energy IceCube neutrinos
• Inspecting the supernova gamma-ray burst connection with high-energy neutrinos
• Astrophysical neutrinos flavored with Beyond the Standard Model physics
• Analysis and modelling of the multi-wavelength observations of the luminous GRB 190114C
• Analysis of the 4-year IceCube high-energy starting events
• Synchrotron self-Compton as a likely mechanism of photons beyond the synchrotron limit in GRB 190114C
• Multiwavelength follow-up of a rare IceCube neutrino multiplet
• Modeling the observations of GRB 180720B: From radio to sub-TeV gamma-rays
• Constraints on Minute-Scale Transient Astrophysical Neutrino Sources
• Probing decaying heavy dark matter with the 4-year IceCube HESE data
• Boosted Dark Matter and its implications for the features in IceCube HESE data
• Reverse Shock Emission Revealed in Early Photometry in the Candidate Short GRB 180418A
• Neutrino, $\gamma$-ray and cosmic ray fluxes from the core of the closest radio galaxies
• Correlation of $\gamma$-ray and high-energy cosmic ray fluxes from the giant lobes of Centaurus A
• Signatures from a quasi-spherical outflow and an off-axis top-hat jet launched in a merger of compact objects: An analytical approach
• The GeV counterpart of VER J2019+407 in the northern shell of the supernova remnant G78.2+2.1 ($\gamma$ Cygni)
• Late Central Engine Activity in GRB 180205A
• Propagation and neutrino oscillations in the base of a highly magnetized gamma-ray burst fireball flow
• Signatures of Neutrino Cooling in the SN1987A Scenario
• Resonant oscillations of GeV - TeV neutrinos in internal shocks from gamma-ray burst jets inside the stars
• TeV-PeV Neutrino Oscillation of Low-luminosity Gamma-ray Bursts
• Could a plasma in quasi-thermal equilibrium be associated to the "orphan" TeV flares ?
• Afterglow light curves of the non-relativistic ejecta mass in a stratified circumstellar medium
• Multi-wavelength radiation models for low-luminosity GRBs, and the implications for UHECRs
• Spin light of neutrino in astrophysical environments
• Description of atypical bursts seen slightly off-axis
• A hypercritical accretion scenario in Central Compact Objects accompanied with an expected neutrino burst
• Cosmic rays, neutrinos and GeV-TeV gamma rays from Starburst Galaxy NGC 4945
• The spectrum and flavor composition of the astrophysical neutrinos in IceCube
• Signature of Collapsars as Sources for High-energy Neutrinos and $r$-process Nuclei
• Reconcilement of VHE $\gamma$-ray/X-ray correlation studies in Mrk 421 and break-down at high fluxes
• Analysis of Fermi-LAT observations, UHECRs and neutrinos from the radio galaxy Centaurus B
• A Central Compact Object in Kes 79: The hypercritical regime and neutrino expectation
• GRB Afterglow of the Sub-relativistic Materials with Energy Injection
• Effects of Annihilation with Low-Energy Neutrinos on High-Energy Neutrinos from Binary Neutron Star Mergers and Rare Core-Collapse Supernovae
• Neutrino propagation in winds around the central engine of sGRB
• Could an hypercritical accretion be associated with the atypical magnetic-field behavior in RX J0822-4300?
• Search for very-high-energy photons from Gamma-ray bursts with HAWC
• Differentiating short gamma-ray bursts progenitors through multi-MeV neutrinos
• Study of PeV neutrinos around dwarf galaxies near giant lobes of Centaurus A
• Search for very-high-energy emission with HAWC from GW170817 event