Astronomy

Does the Hubble constant depend on redshift?

Does the Hubble constant depend on redshift?


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I know there are lot of questions on the Hubble constant already, but I am curious to know if it changes with redshift? If at current redshift, $z=0$, we know its value to be 0.7, will it be different at higher redshift ($z=0.1$)? If so, is there any relationship with redshift?


Yes, definitely.

The Hubble constant describes the expansion rate of the Universe, and the expansion may, in turn, may be decelerated by "regular" matter/energy, and accelerated by dark energy.

It's more or less the norm to use the term Hubble constant $H_0$ for the value today, and Hubble parameter $H(t)$ or $H(a)$ for the value at a time $t$ or, equivalently, a scale factor $a = 1/(1+z)$, where $z$ is the redshift.

The value is given by the Friedmann equation: $$ frac{H^2(a)}{H_0^2} = frac{Omega_mathrm{r}}{a^4} + frac{Omega_mathrm{M}}{a^3} + frac{Omega_k}{a^2} + Omega_Lambda, $$ where ${ Omega_mathrm{r}, Omega_mathrm{M}, Omega_k, Omega_Lambda } simeq { 10^{-3},0.3,0,0.7 } $ are the fractional energy densities in radiation, matter, curvature, and dark energy, respectively.

For instance, you can solve the above equation at $z=0.1$ and find that the expansion rate was 5% higher than today.

Since everything but dark energy dilutes with increasing $a$, $H(a)$ will asymptotically converge to a value $H_0sqrt{Omega_Lambda} simeq 56,mathrm{km},mathrm{s}^{-1},mathrm{Mpc}^{-1}$.

The figure below shows the evolution of the Hubble parameter with time:

As noted by KenG, the fact that $H$ decreases with time may seem at odds with the accelerated expansion of the Universe. But $H$ describes how fast a point in space at a given distance recedes. Later, that point will be farther away, and so will recede faster. From the definition of the Hubble parameter, $Hequivdot{a}/a$, multiplying by the scale factor shows the acceleration $da/dt$:


What the Hubble constant really depends on is how old was the universe at the time, but if you have a dynamical model of the universe, you can map that into z and come up with a function H(z). So in that sense, the answer is "yes," but be careful-- we also think of z as a measure of how far away the objects are, and H does not depend on location it depends on age. What's more, the z we get from a given measurement reflects all the expansion, so all the H's, since that light was emitted, not just the value of that H at that z. It would be a bit like if you were using your height to talk about your age, and you look at a picture of yourself at 4 feet tall, and say you were growing two inches a year when you were that tall. That would be like the H that applies in that picture, but the ratio of the height you are now to the height in that picture depends on more than just the rate you were growing in that picture.

(Also-- what do you mean the value of the Hubble constant is 0.7 now? That sounds like the fraction of total energy that is "dark energy," so is more about the rate of acceleration of the expansion rather than the rate of expansion itself. If you are asking about that, then this number has been rising with age of the universe, so can be mapped into a function of z if we are using z to talk about the age of the universe at the time.)


Watch the video: Ο Hubble, η διαστολή του σύμπαντος και οι συνέπειές της. (June 2022).