Pith. sign in

REVIEW

Constraints on Cosmic Neutrino Fluxes from the ANITA Experiment

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0512265 v2 pith:GS7C6GF7 submitted 2005-12-12 astro-ph

ANITA collaboration: S. W. Barwick , J. J. Beatty , D. Z. Besson , W. R. Binns , B. Cai , J. M. Clem , A. Connolly , D. F. Cowen
show 23 more authors
P. F. Dowkontt M. A. DuVernois P. A. Evenson D. Goldstein P. W. Gorham C. L. Hebert M. H. Israel J. G. Learned K. M. Liewer J. T. Link S. Matsuno P. Miocinovic J. Nam C. J. Naudet R. Nichol K. Palladino M. Rosen D. Saltzberg D. Seckel A. Silvestri B. T. Stokes G. S. Varner F. Wu
This is my paper
classification astro-ph
keywords neutrinocosmicenergyfluxesultra-highanitaexperimentflight
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We report new limits on cosmic neutrino fluxes from the test flight of the Antarctic Impulsive Transient Antenna (ANITA) experiment, which completed an 18.4 day flight of a prototype long-duration balloon payload, called ANITA-lite, in early 2004. We search for impulsive events that could be associated with ultra-high energy neutrino interactions in the ice, and derive limits that constrain several models for ultra-high energy neutrino fluxes. We rule out the long-standing Z-burst model as the source for the ultra-high energy cosmic rays.

Discussion (0). Sign in to comment.

Pith tools