Theoretically palatable flavor combinations of astrophysical neutrinos

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Standard

Theoretically palatable flavor combinations of astrophysical neutrinos. / Bustamante, Mauricio; Beacom, John F.; Winter, Walter.

In: Physical Review Letters, Vol. 115, 161302, 08.06.2015.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Bustamante, M, Beacom, JF & Winter, W 2015, 'Theoretically palatable flavor combinations of astrophysical neutrinos', Physical Review Letters, vol. 115, 161302. https://doi.org/10.1103/PhysRevLett.115.161302

APA

Bustamante, M., Beacom, J. F., & Winter, W. (2015). Theoretically palatable flavor combinations of astrophysical neutrinos. Physical Review Letters, 115, [161302]. https://doi.org/10.1103/PhysRevLett.115.161302

Vancouver

Bustamante M, Beacom JF, Winter W. Theoretically palatable flavor combinations of astrophysical neutrinos. Physical Review Letters. 2015 Jun 8;115. 161302. https://doi.org/10.1103/PhysRevLett.115.161302

Author

Bustamante, Mauricio ; Beacom, John F. ; Winter, Walter. / Theoretically palatable flavor combinations of astrophysical neutrinos. In: Physical Review Letters. 2015 ; Vol. 115.

Bibtex

@article{f056f2ae721c4627af88d93fa602c480,
title = "Theoretically palatable flavor combinations of astrophysical neutrinos",
abstract = "The flavor composition of high-energy astrophysical neutrinos can reveal the physics governing their production, propagation, and interaction. The IceCube Collaboration has published the first experimental determination of the ratio of the flux in each flavor to the total. We present, as a theoretical counterpart, new results for the allowed ranges of flavor ratios at Earth for arbitrary flavor ratios in the sources. Our results will allow IceCube to more quickly identify when their data imply standard physics, a general class of new physics with arbitrary (incoherent) combinations of mass eigenstates, or new physics that goes beyond that, e.g., with terms that dominate the Hamiltonian at high energy.",
keywords = "astro-ph.HE, hep-ph",
author = "Mauricio Bustamante and Beacom, {John F.} and Walter Winter",
note = "13 pages, 12 figures. Matches published version",
year = "2015",
month = jun,
day = "8",
doi = "10.1103/PhysRevLett.115.161302",
language = "English",
volume = "115",
journal = "Physical Review Letters",
issn = "0031-9007",
publisher = "American Physical Society",

}

RIS

TY - JOUR

T1 - Theoretically palatable flavor combinations of astrophysical neutrinos

AU - Bustamante, Mauricio

AU - Beacom, John F.

AU - Winter, Walter

N1 - 13 pages, 12 figures. Matches published version

PY - 2015/6/8

Y1 - 2015/6/8

N2 - The flavor composition of high-energy astrophysical neutrinos can reveal the physics governing their production, propagation, and interaction. The IceCube Collaboration has published the first experimental determination of the ratio of the flux in each flavor to the total. We present, as a theoretical counterpart, new results for the allowed ranges of flavor ratios at Earth for arbitrary flavor ratios in the sources. Our results will allow IceCube to more quickly identify when their data imply standard physics, a general class of new physics with arbitrary (incoherent) combinations of mass eigenstates, or new physics that goes beyond that, e.g., with terms that dominate the Hamiltonian at high energy.

AB - The flavor composition of high-energy astrophysical neutrinos can reveal the physics governing their production, propagation, and interaction. The IceCube Collaboration has published the first experimental determination of the ratio of the flux in each flavor to the total. We present, as a theoretical counterpart, new results for the allowed ranges of flavor ratios at Earth for arbitrary flavor ratios in the sources. Our results will allow IceCube to more quickly identify when their data imply standard physics, a general class of new physics with arbitrary (incoherent) combinations of mass eigenstates, or new physics that goes beyond that, e.g., with terms that dominate the Hamiltonian at high energy.

KW - astro-ph.HE

KW - hep-ph

U2 - 10.1103/PhysRevLett.115.161302

DO - 10.1103/PhysRevLett.115.161302

M3 - Journal article

VL - 115

JO - Physical Review Letters

JF - Physical Review Letters

SN - 0031-9007

M1 - 161302

ER -

ID: 184745452