- #36
hellfire
Science Advisor
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Again I think you are not correct Garth. To make any assertions about the recession velocitiy you shall consider the Hubble law (v = H d), where the Hubble parameter (H) is used and NOT the first time derivative of the scale factor (a -- whose second time derivative determines whether the expansion accelerates or deccelerates). Thus, the time evolution of H is relevant for the discussion and not the time evolution of a or a-dot.Garth said:hellfire - Well spotted! You are correct for a decelerating universe , however Davis and Linewaver were also considering accelerating universes as is thought to be observed from the distant type Ia S/N data. In such a universe the reverse is true and it is in those universes that objects can be observed today as they were in the distant past, when their velocities were sub-luminal, which are receeding from us today at super-luminal velocities.
In every universe with Omega Matter different from zero, the Hubble parameter decreases. Note that in an universe filled only with a cosmological constant (no mater nor radiation), the Hubble parameter would be constant (de-Sitter exponential expansion) as you can verify taking a look to any reference about inflation. Equivalently you may notice that an accelerated exponential expansion has a constant H (integrating H = Const.). Our universe contains 0.73 of cosmological constant and 0.23 of matter, which leads the Hubble parameter to decrease with time (its expansion does also accelerate, but not exponentially).
So, again, although this objetcs were closer to us (d smaller), the Hubble parameter was much greater (H greater). This leads to a greater value of the product v = H d.
I refer you again to the calculator mentioned above. It is not my calculator, although I did also implement one and I have verified the results of this one. The formulas used are in line with the Lineweaver paper. Also the results of this one agree with Ned Wrights one. You can insert a value z for any cosmological model and you will get the result for for the Hubble parameter now and in past (emission epoch), as well as the velocity now and in past.
Regards.
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