SourceProp

Propagation of ultra-high-energy cosmic rays in the source environent and through intergalactic space a la UFA15.

Usage

usage: bin/runFit <fit config> <doFit (default = 1)> <nThreads (default=1)>

Installation

Set ROOT environment, then type

make

License

Released under GPLv3.

Please cite the papers below if you find this code useful in your research.

@article{Unger:2015laa,
    author = "Unger, Michael and Farrar, Glennys R. and Anchordoqui, Luis A.",
    title = "{Origin of the ankle in the ultrahigh energy cosmic ray spectrum, and of the extragalactic protons below it}",
    eprint = "1505.02153",
    archivePrefix = "arXiv",
    primaryClass = "astro-ph.HE",
    doi = "10.1103/PhysRevD.92.123001",
    journal = "Phys. Rev. D",
    volume = "92",
    number = "12",
    pages = "123001",
    year = "2015"
}
@article{Muzio:2019leu,
    author = "Muzio, Marco Stein and Unger, Michael and Farrar, Glennys R.",
    title = "{Progress towards characterizing ultrahigh energy cosmic ray sources}",
    eprint = "1906.06233",
    archivePrefix = "arXiv",
    primaryClass = "astro-ph.HE",
    doi = "10.1103/PhysRevD.100.103008",
    journal = "Phys. Rev. D",
    volume = "100",
    number = "10",
    pages = "103008",
    year = "2019"
}
@article{Muzio:2021zud,
    author = "Muzio, Marco Stein and Farrar, Glennys R. and Unger, Michael",
    title = "{Probing the environments surrounding ultrahigh energy cosmic ray accelerators and their implications for astrophysical neutrinos}",
    eprint = "2108.05512",
    archivePrefix = "arXiv",
    primaryClass = "astro-ph.HE",
    doi = "10.1103/PhysRevD.105.023022",
    journal = "Phys. Rev. D",
    volume = "105",
    number = "2",
    pages = "023022",
    year = "2022"
}