Connection between relic neutrinos and cosmic rays at {approx_gt}10{sup 20};eV?

Journal Article · Thu Oct 01 04:00:00 EDT 1998 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.56587· OSTI ID:365839

Weiler, T J ^[1]

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1. Department of Physics Astronomy, Vanderbilt University, Nashville, Tennessee 37235 (United States)

The observation of cosmic-ray events above the Greisen{endash}Kuzmin{endash}Zatsepin (GZK) cutoff of 5{times}10{sup 19}&hthinsp;eV challenges orthodox modeling. We discuss a possible solution which uses Standard Model (SM) physics augmented only by {approx_lt} eV neutrino masses as suggested by solar, atmospheric, and terrestrial neutrino detection and the cosmological preference for a hot dark matter component. In this scheme, cosmic ray neutrinos from distant, highest-energy sources annihilate relatively nearby on the relic-neutrino background to produce {open_quotes}Z-bursts{close_quotes}, highly-collimated, highly-boosted ({gamma}{sub Z}{approximately}10{sup 11}) hadronic jets. ¿From the SM and hot Big Bang cosmology, the probability for each neutrino flavor at its resonant energy to annihilate within the halo of our galactic supercluster is likely within an order of magnitude of 1{percent}. The kinematics of the annihilation are completely determined by the neutrino masses and the properties of the {ital Z} boson. The burst energy is E{sub R}=4&hthinsp;(eV/m{sub {nu}}){times}10{sup 21}&hthinsp;eV, and the burst content includes, on average, thirty photons and 2.7 nucleons with super-GZK energies. Several tests of the neutrino annihilation hypothesis are indicated. {copyright} {ital 1998 American Institute of Physics.}

• Sponsoring Organization: USDOE
• DOE Contract Number: FG02-85ER40226
• OSTI ID: 365839
• Report Number(s): CONF-980455--
• Journal Information: AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 444; ISSN 0094-243X; ISSN APCPCS
• Country of Publication: United States
• Language: English

Related Subjects

66 PHYSICS
COSMIC NEUTRINOS
COSMIC PROTONS
COSMIC RADIATION
NEUTRINO OSCILLATION
PEV RANGE
WEINBERG-SALAM GAUGE MODEL
Z NEUTRAL BOSONS