ParaMonte Fortran 2.0.0
Parallel Monte Carlo and Machine Learning Library
See the latest version documentation.
pm_cosmicRate.F90 File Reference

Go to the source code of this file.

Data Types

interface  pm_cosmicRate::getLogRateDensityH06
 Generate and return the unnormalized Comoving Star Formation Rate (SFR) density for a given redshift \(z\) based on the estimates of Hopkins and Beacom et al. (2006), assuming a piecewise power-law fit.
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interface  pm_cosmicRate::getLogRateDensityL08
 Generate and return the unnormalized Comoving Star Formation Rate (SFR) density for a given redshift \(z\) based on the estimates of Li (2008), assuming a piecewise power-law fit.
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interface  pm_cosmicRate::getLogRateDensityM14
 Generate and return the unnormalized Comoving Star Formation Rate (SFR) density for a given redshift \(z\) based on the estimates of Eqn. 15 of Madau 2014: Cosmic Star-Formation History. More...
 
interface  pm_cosmicRate::getLogRateDensityM17
 Generate and return the unnormalized Comoving Star Formation Rate (SFR) density for a given redshift \(z\) based on the estimates of Eqn. 15 of Madau 2014: Cosmic Star-Formation History. More...
 
interface  pm_cosmicRate::getLogRateDensityF18
 Generate and return the unnormalized Comoving Star Formation Rate (SFR) density for a given redshift \(z\) based on the estimates of Fermi LAT Collaboration 2018: A gamma-ray determination of the Universe’s star formation history. More...
 
interface  pm_cosmicRate::getLogRateDensityB10
 Generate and return the unnormalized Comoving LGRB Formation Rate (LGFR) density for a given redshift \(z\) based on the Metallicity-corrected estimates of Butler et al. (2010): B10, assuming a piecewise power-law LGFR model. More...
 
interface  pm_cosmicRate::getLogRateDensityP15
 Generate and return the unnormalized Gamma-Ray Burst Formation Rate (GRBFR) density based on the estimates of Petrosian et al (2015). More...
 

Modules

module  pm_cosmicRate
 This module contains procedures and generic interfaces for computing the cosmic rates of celestial phenomena.
 

Variables

character(*, SK), parameter pm_cosmicRate::MODULE_NAME = "@pm_cosmicRate"