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Added a Hubble Parameter calculator file (TheAlgorithms#7921)
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""" | ||
Title : Calculating the Hubble Parameter | ||
Description : The Hubble parameter H is the Universe expansion rate | ||
in any time. In cosmology is customary to use the redshift redshift | ||
in place of time, becausethe redshift is directily mensure | ||
in the light of galaxies moving away from us. | ||
So, the general relation that we obtain is | ||
H = hubble_constant*(radiation_density*(redshift+1)**4 | ||
+ matter_density*(redshift+1)**3 | ||
+ curvature*(redshift+1)**2 + dark_energy)**(1/2) | ||
where radiation_density, matter_density, dark_energy are the relativity | ||
(the percentage) energy densities that exist | ||
in the Universe today. Here, matter_density is the | ||
sum of the barion density and the | ||
dark matter. Curvature is the curvature parameter and can be written in term | ||
of the densities by the completeness | ||
curvature = 1 - (matter_density + radiation_density + dark_energy) | ||
Source : | ||
https://www.sciencedirect.com/topics/mathematics/hubble-parameter | ||
""" | ||
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def hubble_parameter( | ||
hubble_constant: float, | ||
radiation_density: float, | ||
matter_density: float, | ||
dark_energy: float, | ||
redshift: float, | ||
) -> float: | ||
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""" | ||
Input Parameters | ||
---------------- | ||
hubble_constant: Hubble constante is the expansion rate today usually | ||
given in km/(s*Mpc) | ||
radiation_density: relative radiation density today | ||
matter_density: relative mass density today | ||
dark_energy: relative dark energy density today | ||
redshift: the light redshift | ||
Returns | ||
------- | ||
result : Hubble parameter in and the unit km/s/Mpc (the unit can be | ||
changed if you want, just need to change the unit of the Hubble constant) | ||
>>> hubble_parameter(hubble_constant=68.3, radiation_density=1e-4, | ||
... matter_density=-0.3, dark_energy=0.7, redshift=1) | ||
Traceback (most recent call last): | ||
... | ||
ValueError: All input parameters must be positive | ||
>>> hubble_parameter(hubble_constant=68.3, radiation_density=1e-4, | ||
... matter_density= 1.2, dark_energy=0.7, redshift=1) | ||
Traceback (most recent call last): | ||
... | ||
ValueError: Relative densities cannot be greater than one | ||
>>> hubble_parameter(hubble_constant=68.3, radiation_density=1e-4, | ||
... matter_density= 0.3, dark_energy=0.7, redshift=0) | ||
68.3 | ||
""" | ||
parameters = [redshift, radiation_density, matter_density, dark_energy] | ||
if any(0 > p for p in parameters): | ||
raise ValueError("All input parameters must be positive") | ||
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if any(1 < p for p in parameters[1:4]): | ||
raise ValueError("Relative densities cannot be greater than one") | ||
else: | ||
curvature = 1 - (matter_density + radiation_density + dark_energy) | ||
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e_2 = ( | ||
radiation_density * (redshift + 1) ** 4 | ||
+ matter_density * (redshift + 1) ** 3 | ||
+ curvature * (redshift + 1) ** 2 | ||
+ dark_energy | ||
) | ||
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hubble = hubble_constant * e_2 ** (1 / 2) | ||
return hubble | ||
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if __name__ == "__main__": | ||
import doctest | ||
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# run doctest | ||
doctest.testmod() | ||
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# demo LCDM approximation | ||
matter_density = 0.3 | ||
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print( | ||
hubble_parameter( | ||
hubble_constant=68.3, | ||
radiation_density=1e-4, | ||
matter_density=matter_density, | ||
dark_energy=1 - matter_density, | ||
redshift=0, | ||
) | ||
) |