Welcome to NNSFν#

Zenodo arXiv PyPI Status License

NNSFν povides predictions for neutrino inelastic structure functions valid for the complete range of energies relevant for phenomenology involving \(\nu / \bar{\nu}\)-experiments, from oscillation measurements carried out with reactors, accelerators, and atmospheric neutrinos to astroparticle physics at ultra-high-energy (UHE) neutrino telescopes such as IceCube and KM3NET.


⚡ Getting Started

Description of the package and instructions for the installation.

To quick start

🔥 Tutorials

Various tutorials on using the codes and generate predictions.

To tutorials

Citing NNSFν#

To reference NNSFν in a scientific publication please use the following:

@article{Candido:2023utz,
    author = "Candido, Alessandro and Garcia, Alfonso and Magni, Giacomo and Rabemananjara, Tanjona and Rojo, Juan and Stegeman, Roy",
    title = "{Neutrino Structure Functions from GeV to EeV Energies}",
    eprint = "2302.08527",
    archivePrefix = "arXiv",
    primaryClass = "hep-ph",
    reportNumber = "Nikhef 2022-014, Edinburgh 2022/27, TIF-UNIMI-2023-5",
    month = "2",
    year = "2023"
}

If NNSFν proves to be useful in your work, please also reference the codes:

@misc{https://doi.org/10.5281/zenodo.7657132,
  doi = {10.5281/ZENODO.7657132},
  url = {https://zenodo.org/record/7657132},
  author = "Candido, Alessandro and Garcia, Alfonso and Magni, Giacomo and Rabemananjara, Tanjona and Rojo, Juan and Stegeman, Roy",
  title = "{Neutrino Structure Functions from GeV to EeV Energies}",
  publisher = {Zenodo},
  year = {2023},
  copyright = {Open Access}
}

Indices and tables#