“Their observations measured the evolution of the Hubble parameter over time by constructing a Hubble diagram: a plot of distance modulus versus redshift (Figure 11.33). For small $z$, the Hubble diagram tells the value of Ho. At large $z$, the diagram shows evidence for changes in the expansion rate. At a given distance, for example, if the universe is deceler ating, the expansion rate will have been higher in the past than predicted by $H(t) = Ho$. Therefore, if gravity slows the expansion (as was expected) at large $μ$ (i.e. the universe in the past), the observed redshift should be higher than predicted. This deviation will increase with increasing $µ$.”
I quoted a book that I found on Google. The book says that supernova studies have shown that the value of Hubble parameters has been smaller in the past. However, it is known that H(t) always decreases with time. I think what this book says is a(t)/dt. What does H(t) from the book mean?
And I don't think the meaning of H(t) is the same in many references. What exactly is H(t) used in supernova cosmology?
