|
| 1 | +""" |
| 2 | +Title : Calculating the Hubble Parameter |
| 3 | +
|
| 4 | +Description : The Hubble parameter H is the Universe expansion rate |
| 5 | +in any time. In cosmology is customary to use the redshift redshift |
| 6 | +in place of time, becausethe redshift is directily mensure |
| 7 | +in the light of galaxies moving away from us. |
| 8 | +
|
| 9 | +So, the general relation that we obtain is |
| 10 | +
|
| 11 | +H = hubble_constant*(radiation_density*(redshift+1)**4 |
| 12 | + + matter_density*(redshift+1)**3 |
| 13 | + + curvature*(redshift+1)**2 + dark_energy)**(1/2) |
| 14 | +
|
| 15 | +where radiation_density, matter_density, dark_energy are the relativity |
| 16 | +(the percentage) energy densities that exist |
| 17 | +in the Universe today. Here, matter_density is the |
| 18 | +sum of the barion density and the |
| 19 | +dark matter. Curvature is the curvature parameter and can be written in term |
| 20 | +of the densities by the completeness |
| 21 | +
|
| 22 | +
|
| 23 | +curvature = 1 - (matter_density + radiation_density + dark_energy) |
| 24 | +
|
| 25 | +Source : |
| 26 | +https://www.sciencedirect.com/topics/mathematics/hubble-parameter |
| 27 | +""" |
| 28 | + |
| 29 | + |
| 30 | +def hubble_parameter( |
| 31 | + hubble_constant: float, |
| 32 | + radiation_density: float, |
| 33 | + matter_density: float, |
| 34 | + dark_energy: float, |
| 35 | + redshift: float, |
| 36 | +) -> float: |
| 37 | + |
| 38 | + """ |
| 39 | + Input Parameters |
| 40 | + ---------------- |
| 41 | + hubble_constant: Hubble constante is the expansion rate today usually |
| 42 | + given in km/(s*Mpc) |
| 43 | +
|
| 44 | + radiation_density: relative radiation density today |
| 45 | +
|
| 46 | + matter_density: relative mass density today |
| 47 | +
|
| 48 | + dark_energy: relative dark energy density today |
| 49 | +
|
| 50 | + redshift: the light redshift |
| 51 | +
|
| 52 | + Returns |
| 53 | + ------- |
| 54 | + result : Hubble parameter in and the unit km/s/Mpc (the unit can be |
| 55 | + changed if you want, just need to change the unit of the Hubble constant) |
| 56 | +
|
| 57 | + >>> hubble_parameter(hubble_constant=68.3, radiation_density=1e-4, |
| 58 | + ... matter_density=-0.3, dark_energy=0.7, redshift=1) |
| 59 | + Traceback (most recent call last): |
| 60 | + ... |
| 61 | + ValueError: All input parameters must be positive |
| 62 | +
|
| 63 | + >>> hubble_parameter(hubble_constant=68.3, radiation_density=1e-4, |
| 64 | + ... matter_density= 1.2, dark_energy=0.7, redshift=1) |
| 65 | + Traceback (most recent call last): |
| 66 | + ... |
| 67 | + ValueError: Relative densities cannot be greater than one |
| 68 | +
|
| 69 | + >>> hubble_parameter(hubble_constant=68.3, radiation_density=1e-4, |
| 70 | + ... matter_density= 0.3, dark_energy=0.7, redshift=0) |
| 71 | + 68.3 |
| 72 | + """ |
| 73 | + parameters = [redshift, radiation_density, matter_density, dark_energy] |
| 74 | + if any(0 > p for p in parameters): |
| 75 | + raise ValueError("All input parameters must be positive") |
| 76 | + |
| 77 | + if any(1 < p for p in parameters[1:4]): |
| 78 | + raise ValueError("Relative densities cannot be greater than one") |
| 79 | + else: |
| 80 | + curvature = 1 - (matter_density + radiation_density + dark_energy) |
| 81 | + |
| 82 | + e_2 = ( |
| 83 | + radiation_density * (redshift + 1) ** 4 |
| 84 | + + matter_density * (redshift + 1) ** 3 |
| 85 | + + curvature * (redshift + 1) ** 2 |
| 86 | + + dark_energy |
| 87 | + ) |
| 88 | + |
| 89 | + hubble = hubble_constant * e_2 ** (1 / 2) |
| 90 | + return hubble |
| 91 | + |
| 92 | + |
| 93 | +if __name__ == "__main__": |
| 94 | + import doctest |
| 95 | + |
| 96 | + # run doctest |
| 97 | + doctest.testmod() |
| 98 | + |
| 99 | + # demo LCDM approximation |
| 100 | + matter_density = 0.3 |
| 101 | + |
| 102 | + print( |
| 103 | + hubble_parameter( |
| 104 | + hubble_constant=68.3, |
| 105 | + radiation_density=1e-4, |
| 106 | + matter_density=matter_density, |
| 107 | + dark_energy=1 - matter_density, |
| 108 | + redshift=0, |
| 109 | + ) |
| 110 | + ) |
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