2853: Redshift

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Redshift

Title text: So do you have any plans for z=-0.000000000000045?

Explanation

This explanation may be incomplete or incorrect: Created by a SHIFTY RED MATTER BALL - Please change this comment when editing this page. Do NOT delete this tag too soon. If you can address this issue, please edit the page! Thanks.

In cosmology, redshift refers to the way that light from distant objects in the universe is stretched out, making it appear more red than it would otherwise. This occurs because the universe is expanding, and as a result, light waves are stretched as they travel through space. The "z" value is a dimensionless measure of the redshift. A higher "z" value, or redshift, corresponds to earlier times in the history of the universe. This is because as the universe expands, light from distant galaxies is stretched to longer, redder wavelengths as it travels towards us. The further away a galaxy is, the longer its light has been traveling, and thus the more the universe has expanded since that light began its journey. Therefore, a higher redshift indicates a galaxy that is further away and that the light we see from it left when the universe was younger. Conversely, a lower redshift means the light has traveled a shorter distance and time, indicating a more recent epoch in the history of the universe. Negative values of "z" indicate a blueshift, which indicate objects that are approaching the observer, generally used in cosmological work to calculate rotation speeds of nearby objects.

The joke here is that Cueball is asking Ponytail when they became interested in cosmology, and instead of giving a time like "in college" or "as a kid," they respond with a very precise redshift value "z=0.00000000038." This absurdly precise number is due to a highly recent event compared to the start of the universe, within the cosmologist's lifetime. The negative blueshift question in the title text is a playful way of asking about a future event, as it is approaching the speakers. Specifically it is a closer event to present day to when the cosmologist became interested in her field of study as the absolute value of z is 10^4 smaller and indicates a closer albeit future event.

Assuming a particular cosmology, and in particular values for the Hubble constant (H₀) and the curvature of the universe, it is possible to specify a particular look-back time. For z = 0.00000000038, and a flat Lambda CDM cosmology, with H₀ = 69.32 km / (Mpc s), a value of Ω₀ of 0.2865, a cosmic background temperature of 2.725 K, the look-back time is of around 1960 days, or five and a half years, which could suggest that the person started studying cosmology as part of a Ph.D. program.

Negative numbers of z would indicate a "look-forward" time, or a time in the future, and the same model indicates that z = -0.000000000000045 corresponds to about 5.5 hours in the future.

The use of non-standard units of measurement has also been seen in 2707: Astronomy Numbers, with (higher) redshift values previously visited as a part of 2764: Cosmological Nostalgia Content.

Transcript

This transcript is incomplete. Please help editing it! Thanks.

[Ponytail and Cueball are sitting at a table, eating dinner.]

Cueball: So, when did you first get interested in early universe cosmology?

Ponytail: Sometime around z=0.00000000038.

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Discussion

Does it make any sense to try and relate the two Z values to a more "normal" time? MAP (talk) 21:08, 10 November 2023 (UTC)

I have added exactly that, using `astropy.cosmology` for the calculations Juandesant (talk) 21:16, 10 November 2023 (UTC)

There is a big error in the current explanation, saying it means they were interested in this since the early universe, but that would only be true if the z value was much closer to 1. I'm not exactly sure as I haven't done the math, but with that many decimal places of zero's it is probably near enough history to be during their lifetime. So the joke isn't being interested in the early universe since the early universe, but rather so interested in it that they talk about other things with the same terminology.--172.70.126.142 21:18, 10 November 2023 (UTC)

Why aren't these values expressed in scientific notation? Separately, do they make sense logarithmically? JohnHawkinson (talk) 07:12, 11 November 2023 (UTC)

Part of the joke is that the values are unwieldy to use compared to everyday language and units. The scientific notation would have lessened this. However they are given in a universal standard time instead of some solar system or human related units, so they generally should be clearly preferred. Sebastian --172.68.110.188 15:37, 11 November 2023 (UTC)

I feel like the Earth's gravitational field would affect the answer as z goes to zero? 172.69.22.210 06:57, 12 November 2023 (UTC)

Calculation

Thanks to ChatGPT-4 and the Fortran-90 code from arxiv:1303.5961 (which please see, it's really cool) here's how to get the look-back time from redshift in Python:

from scipy.special import hyp2f1  # hypergeometric function 2F1 is in integral solution
from numpy import format_float_positional

# Cosmological parameters from the Fortran params.f90 header
#H0 = 67.15       # Hubble constant in km/s/Mpc (or, 73.5: the "crisis in cosmology")
H0 = 69.32        # from Explainxkcd for 2853: Redshift; seems a consensus compromise
#OL = 0.683       # Cosmological constant for dark energy density, Omega_Lambda or _vac
#Om = 0.317       # Density parameter for matter, Omega_mass
Om = 0.286        # From https://arxiv.org/pdf/1406.1718.pdf page 8
OL = 1.0 - Om - 0.4165/(H0**2)  # flat curvature, from https://www.astro.ucla.edu/~wright/CC.python
                  # (on https://www.astro.ucla.edu/~wright/CosmoCalc.html which see)
#print(f"{OL=:.3F}")  # 0.714

# Age of universe at redshift z as a closed-form solution to its integral definition,
def age_at_z(z):  # ...which is 27 times faster than the original numeric integration
    hypergeom = hyp2f1(0.5, 0.5, 1.5, -OL / (Om * (z + 1)**3))
    return (2/3) * hypergeom / (Om**0.5 * (z + 1)**1.5) * (977.8 / H0)  # 977.8 for Gyr

# Current age of the universe at redshift 0 in Gyr
age0 = age_at_z(0)  # 13.78

# Function to calculate the look-back time at redshift z in Gyr
def zt(z):  # from the function name in the Fortran cosmonom.f90 code
    return age0 - age_at_z(z)

# For z = 0.00000000038
z1 = 0.00000000038
look_back_time_years_z1 = zt(z1) * 1e9 # from Gyr to years
print("Look-back time for z=" + 
      f"{format_float_positional(z1)}: {look_back_time_years_z1:.1f} years")

# For z = -0.000000000000045
z2 = -0.000000000000045
look_back_time_hours_z2 = zt(z2) * 1e9 * 365.25 * 24
print("Look-back time for z=" +
      f"{format_float_positional(z2)}: {look_back_time_hours_z2:.1f} hours")

The output being:

Look-back time for z=0.00000000038: 5.4 years
Look-back time for z=-0.000000000000045: -5.5 hours

And should you wish to make this quick reference chart for interpreting observations in the JWST era:

Or this one showing the age of the universe from redshift:

P.S. Some commentary from ChatGPT-4 about the special Gaussian hypergeometric function hyp2f1 in the closed-form solution of the integral:

The appearance of the hypergeometric function 2F1 in the solution for the age of the universe as a function of redshift is a profound example of the interconnectedness of mathematical functions and physical phenomena. The hypergeometric function, which encompasses a vast family of functions, can describe a wide range of behaviors and has properties that make it particularly suited to representing solutions to differential equations that arise in physics.

In the context of cosmology, the use of 2F1 in calculating the age of the universe from redshift is not just a mathematical convenience but rather a reflection of the underlying physics. The Friedman equations, which govern the expansion of the universe, are derived from General Relativity and lead to solutions involving integrals that can express the evolution of the universe's scale factor over time. When these integrals are solved, they often involve special functions like 2F1, which encode information about the geometry of the universe and the relative contributions of matter, radiation, and dark energy.

The presence of 2F1 in this solution indicates that the relationship between the age of the universe and redshift is non-linear and depends on the integral of a function that encapsulates the dynamics of cosmic expansion. It's also worth noting that special functions like 2F1 often have interesting properties, such as symmetry and recurrence relations, which sometimes allow physicists to gain insights into the behavior of the universe under different conditions or scales.

Furthermore, solutions involving 2F1 are not merely academic exercises; they can be compared with observational data, such as measurements of the cosmic microwave background radiation, distributions of galaxies, or supernovae light curves. These comparisons can test the validity of our cosmological models and potentially offer new insights into the nature of dark energy and dark matter, the curvature of the universe, and other fundamental questions in cosmology.

In summary, the use of 2F1 in the closed-form solution for the age of the universe from redshift is a powerful reminder that mathematics provides us with the tools to decode the cosmos, offering deeper understanding and raising new questions about the fundamental structure and evolution of the universe.

Liv2splain (talk) 19:25, 14 November 2023 (UTC)

A further simplification: hyp2f1(0.5, 0.5, 1.5, z**2) = arcsin(z) / z. 172.69.150.141 (talk) 13:43, 17 November 2023 (please sign your comments with ~~~~)

-OL / (Om * (z + 1)**3) is not z**2. 172.70.210.234 10:09, 22 July 2024 (UTC)