pm_cosmicRate Module Reference

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

Data Types
interface	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	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	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. More...
interface	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. More...
interface	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	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	getLogRateDensityP15
	Generate and return the unnormalized Gamma-Ray Burst Formation Rate (GRBFR) density based on the estimates of Petrosian et al (2015). More...

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

Detailed Description

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

Specifically, the cosmic rate densities of formations of two celestial objects are currently implemented in this module:

1. the cosmic Star Formation Rate (SFR) density in the Universe under different modeling scenarios,
2. the cosmic Long-duration Gamma-Ray Burst (LGRB) Formation Rate (LGRBFR) density in the Universe as a function of cosmological redshift.

Cosmic rate

The rate of occurrence of a cosmic phenomenon can be readily computed by multiplying its cosmic rate density with the differential comoving volume element of the Universe at the given redshift.
The following two generic interfaces return the normalized differential comoving volume element for a variety of possible input arguments:

1. getVolComDiffNormed
   
2. setVolComDiffNormed
   

See the generic interfaces above and examples below for computing of the cosmic rates of events from their cosmic rate densities.

See also

pm_cosmology

Final Remarks ⛓

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Copyright

Computational Data Science Lab

Author:

Amir Shahmoradi, September 1, 2017, 12:00 AM, Institute for Computational Engineering and Sciences (ICES), The University of Texas Austin

Variable Documentation

MODULE_NAME

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

Definition at line 55 of file pm_cosmicRate.F90.