dComovVol

omega.m

omega.lambda

Function computes differential comoving volume in a flat cosmology.

misc

Package encapsulates standard expressions for distances, times, luminosities, and other quantities useful in observational cosmology, including molecular line observations.  Currently coded for a flat universe only.

Andrew Harris

cosmoFns

Functions for Cosmological Distances, Times, Luminosities, Etc

dComovVol function

<dl> <dt>z</dt>
<dd>Redshift</dd> <dt>omega.m</dt>
<dd>Omega matter parameter</dd> <dt>omega.lambda</dt>
<dd>Omega lambda parameter</dd> <dt>H.0</dt>
<dd>Hubble constant in km/s/Mpc</dd></dl>

Arguments

Author

Differential comoving volume — dComovVol

<dl>

 <dt>z</dt>
<dd>Redshift</dd>

 <dt>omega.m</dt>
<dd>Omega matter parameter</dd>

 <dt>omega.lambda</dt>
<dd>Omega lambda parameter</dd>

 <dt>H.0</dt>
<dd>Hubble constant in km/s/Mpc</dd>

</dl>

dComovVol: Differential comoving volume

Description

Usage

Value

Arguments

Author

References

Examples