Authors: Tadeo D. Gómez & Luis E. Padilla
Source: Source code at GitHub
Licence: GNU General Public License v2.0. The documentation is licensed under the GFDL.
The PBHBeta
library is a computational tool designed to calculate constraints on the abundance of Primordial Black Holes (PBHs) and the power spectrum (PS) in cosmological scenarios featuring a non-standard evolution phase between the end of inflation and Big Bang Nucleosynthesis (BBN).
This project is under development.
This code has been tested exclusively with Python version 3.9, and we strongly recommend using it with versions higher than this (Python 3.x and above).
The GitHub repository and PyPI package for PBHBeta
include the essential libraries necessary to run PBHBeta
. However, these dependencies must be imported into the notebook or console for the functions to become accesible. Refer to the Requeriments and installation sections.
If you use PBH-{math}\beta
, please cite arXiv: 2308.04642v1.
- 1.0.1 (14/08/2023) Changes were implemented in the names of modules, functions, and classes.
- 1.0 (05/08/2023) Initial version.
- Complete the description into documentation to modules and components.
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