Graduate What is the jerk parameter in terms of the Density parameters?

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The jerk parameter in cosmology is defined in relation to the deceleration parameter, with the general expression being j(q) = q + 2q^2 + (1+z)dq/dz. For the ΛCDM model, the specific formula for the jerk parameter is j_0 = q_0 + 2q_0^2 + 1. However, this relationship does not hold for other cosmological models where the equation of state parameter w_DE is time-dependent. Thus, the jerk parameter can vary significantly across different cosmological frameworks. Understanding these parameters is crucial for analyzing the dynamics of the universe's expansion.
Arman777
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In cosmology the deceleration parameter defined as the

$$q_0 = \frac{1}{2}\sum_i\Omega_{i,0}(1+3w_i)$$

Is there a similar expression for the jerk parameter (##j_0##) ?
 
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Here is the asnwer

In general

$$j(q) = q + 2q^2 + (1+z)\frac{dq}{dz}$$

for $\Lambda$CDM model$$j_0 = q_0 + 2q_0^2 + 1$$

Note that for different cosmological models

$$j_0 \neq q_0 + 2q_0^2 + 1$$

since in the other models ##w_{\rm DE}## is time dependent (well at least in most of them)
 
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I always thought it was odd that we know dark energy expands our universe, and that we know it has been increasing over time, yet no one ever expressed a "true" size of the universe (not "observable" universe, the ENTIRE universe) by just reversing the process of expansion based on our understanding of its rate through history, to the point where everything would've been in an extremely small region. The more I've looked into it recently, I've come to find that it is due to that "inflation"...

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