TeV neutrinos and gamma rays from pulsars

Abstract

Recent studies suggest that pulsars could be strong sources of TeV muon neutrinos provided positive ions are accelerated by pulsar polar caps to PeV energies. In such a situation muon neutrinos are produced through the delta resonance in interactions of pulsar accelerated ions with its thermal radiation field. High energy gamma rays also should be produced simultaneously in pulsar environment as both charged and neutral pions are generated in the interactions of energetic hadrons with the ambient photon fields. Here we estimate TeV gamma ray flux at Earth from few nearby young pulsars. When compared with the observations we find that proper consideration of the effect of polar cap geometry in flux calculation is important. Incorporating such an effect we obtain the (revised) event rates at Earth due to few potential nearby pulsars. The results suggest that pulsars are unlikely to be detected by the upcoming neutrino telescopes. We also estimate TeV gamma ray and neutrino fluxes from pulsar nebulae for the adopted model of particle acceleration.

Six pages, accepted in MNRAS

References in corpus (5)

• Observations of the Crab Nebula with H.E.S.S
• Astroparticle Physics with High Energy Neutrinos: from AMANDA to IceCube
• Search for Pulsed VHE Gamma-Ray Emission from Young Pulsars with H.E.S.S
• Flux predictions of high-energy neutrinos from pulsars
• Contribution of a nearby Pulsar to Cosmic Rays observed at Earth

Cited by in corpus (8)

• Cascade Events at IceCube+DeepCore as a Definitive Constraint on the Dark Matter Interpretation of the PAMELA and Fermi Anomalies
• Search for spatial coincidence between IceCube neutrinos and radio pulsars
• Searching for PeV neutrinos from photomeson interactions in magnetars
• Probing the cosmic ray mass composition in the knee region through TeV secondary particle fluxes from solar surroundings
• A stacked search for spatial coincidences between IceCube neutrinos and radio pulsars
• Newly born extragalactic millisecond pulsars as efficient emitters of PeV neutrinos
• Diffuse flux of PeV neutrinos from centrifugally accelerated protons in active galactic nuclei
• Diffuse emission of TeV Neutrinos and Gamma-rays from young pulsars by Photo-meson interaction in the galaxy