Impact of the QCD dynamics on the determination of the high energy astrophysical neutrino flux
V.P. Goncalves, D. Gratieri* and A.S.d.C. Quadros
*: corresponding author
Full text: pdf
Published on: March 31, 2022
Abstract
The results presented here are based on the work \cite{EPJC21}, where we determine the impact of different assumptions in the description of the high-energy QCD interactions on the determination of the astrophysical neutrino flux, the normalization $\Phi_{Astro}$ and spectral index $\gamma$ of. The energy distribution of neutrino events at the IceCube is estimated considering the DGLAP, BFKL, CGC and BBMT approaches, and the best estimates for the flux parameters are determined using a maximum likelihood fit comparing the predictions with the distribution of observed events at IceCube. We also investigate if the increase of the effective exposure time expected in IceCube - Gen2 will allow us to disentangle the QCD dynamical effects from the description of the astrophysical neutrino flux.
DOI: https://doi.org/10.22323/1.402.0091
How to cite

Metadata are provided both in article format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in proceeding format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.