Measuring flavor ratios of high-energy astrophysical neutrinos
- Fermilab
- Fermilab; Santa Barbara, KITP
- Wisconsin U., Madison
- Hawaii U.; Santa Barbara, KITP
- Vanderbilt U.; Santa Barbara, KITP
We discuss the prospects for next generation neutrino telescopes, such as IceCube, to measure the flavor ratios of high-energy astrophysical neutrinos. The expected flavor ratios at the sources are $$\phi_{\nu_e}:\phi_{\nu_{\mu}}:\phi_{\nu_{\tau}} = 1:2:0$$, and neutrino oscillations quickly transform these to $1:1:1$. The flavor ratios can be deduced from the relative rates of showers ($$\nu_e$$ charged-current, most $$\nu_\tau$$ charged-current, and all flavors neutral-current), muon tracks ($$\nu_\mu$$ charged-current only), and tau lepton lollipops and double-bangs ($$\nu_\tau$$ charged-current only). The peak sensitivities for these interactions are at different neutrino energies, but the flavor ratios can be reliably connected by a reasonable measurement of the spectrum shape. Measurement of the astrophysical neutrino flavor ratios tests the assumed production mechanism and also provides a very long baseline test of a number of exotic scenarios, including neutrino decay, CPT violation, and small-$$\delta m^2$$ oscillations to sterile neutrinos.
- Research Organization:
- Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
- DOE Contract Number:
- AC02-07CH11359
- OSTI ID:
- 1875890
- Report Number(s):
- FERMILAB-PUB-03-180-A; MADPH-03-1336; arXiv:hep-ph/0307025; oai:inspirehep.net:622515
- Journal Information:
- Phys.Rev.D, Journal Name: Phys.Rev.D Vol. 68
- Country of Publication:
- United States
- Language:
- English
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