Metadata-Version: 2.1
Name: prince-cr
Version: 0.6.0
Summary: Cosmic ray PRopagation Including Nuclear Cascade equations
Home-page: https://github.com/joheinze/PriNCe
Author: Jonas Heinze and Anatoli Fedynitch
Author-email: afedynitch@gmail.com
License: BSD 3-Clause License
Description: # PriNCe - **Pr**opagation **i**ncluding **N**uclear **C**ascade **e**quations
        
        This code solves the transport equation for ultra-high energy cosmic rays on cosmological scales.
        
        ## About this version
        
        The package is numerically accurate for its current purpose (UHECR propagation). Since this the first public version, one should be cautious when deviating from the examples and check if the result makes sense, simply because so far only us (the devs) have been using it and the interfaces aren't sufficiently polished to be used *error-free* for tasks that we didn't foresee. Please file issues for anything strange, unclear, wrong, etc.. It will help us to debug the code and simplify the user interface.
        
        ## Installation
        
        is as simple as 
        
        ```bash
        pip install prince-cr
        ```
        
        Check [the docs](https://prince.readthedocs.io/en/latest/) for more details on the requirements. 
        
        ## [Documentation](https://prince.readthedocs.io/en/latest/)
        
        The docs are hosted at [readthedocs](https://prince.readthedocs.io/en/latest/). They are still *incomplete* and we are working on improvements. Feedback/comments are welcome.
        
        ## [Examples](https://github.com/joheinze/PriNCe-examples)
        
        To get started check out the [examples repository](https://github.com/joheinze/PriNCe-examples) and/or follow [the tutorial](https://prince.readthedocs.io/en/latest/tutorial.html). 
        
        ## Citation
        
        If you are using this code in your work, please cite:
        
        *A new view on Auger data and cosmogenic neutrinos in light of different nuclear disintegration and air-shower models*  
        J. Heinze, A. Fedynitch, D. Boncioli and W. Winter  
        Astrophys.J. 873 (2019) no.1, 88  
        doi: [10.3847/1538-4357/ab05ce](https://doi.org/10.3847/1538-4357/ab05ce)
        
        ## Authors
        
        - *Anatoli Fedynitch*
        - *Jonas Heinze*
        
        ## Copyright and license
        
        Code released under [the BSD 3-clause license (see LICENSE)](LICENSE).
        
        ## Acknowledgements
        
        This code has been initially developed as part of the [NEUCOS project](https://astro.desy.de/theory/neucos/index_eng.html) and has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme ([Grant No. 646623](https://cordis.europa.eu/project/id/646623)).
        
Platform: UNKNOWN
Classifier: Programming Language :: Python
Classifier: Programming Language :: Python :: 3
Classifier: Programming Language :: Python :: 3.6
Classifier: Programming Language :: Python :: 3.7
Classifier: Programming Language :: Python :: 3.8
Classifier: Topic :: Scientific/Engineering :: Physics
Classifier: Intended Audience :: Science/Research
Classifier: Development Status :: 4 - Beta
Classifier: License :: OSI Approved :: BSD License
Description-Content-Type: text/markdown
