Ultrahigh-energy neutrino scattering

Kuroda M, Schildknecht D (2013)
Physical Review D 88(5).

Journal Article | Published | English

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We predict the neutrino-nucleon cross section at ultrahigh energies relevant in connection with the search for high-energy cosmic neutrinos. Our investigation, employing the color-dipole picture, among other things, allows us to quantitatively determine which fraction of the ultrahigh-energy neutrino-nucleon cross section stems from the saturation vs the color-transparency region. We disagree with various results in the literature that predict a strong suppression of the neutrino-nucleon cross section at neutrino energies above E congruent to 10(9) GeV. Suppression in the sense of a diminished increase of the neutrino-nucleon cross section with energy only starts to occur at neutrino energies beyond E congruent to 10(14) GeV.
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Kuroda M, Schildknecht D. Ultrahigh-energy neutrino scattering. Physical Review D. 2013;88(5).
Kuroda, M., & Schildknecht, D. (2013). Ultrahigh-energy neutrino scattering. Physical Review D, 88(5).
Kuroda, M., and Schildknecht, D. (2013). Ultrahigh-energy neutrino scattering. Physical Review D 88.
Kuroda, M., & Schildknecht, D., 2013. Ultrahigh-energy neutrino scattering. Physical Review D, 88(5).
M. Kuroda and D. Schildknecht, “Ultrahigh-energy neutrino scattering”, Physical Review D, vol. 88, 2013.
Kuroda, M., Schildknecht, D.: Ultrahigh-energy neutrino scattering. Physical Review D. 88, (2013).
Kuroda, Masaaki, and Schildknecht, Dieter. “Ultrahigh-energy neutrino scattering”. Physical Review D 88.5 (2013).
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