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Barrow's history of 20th-century cosmologies takes us from steady-state to big bang theories, universes that create themselves in closed time loops, bouncing or eternally inflating universes, and "kinky", "deviant" or "Mixmaster" universes – the zoo of possible solutions to Einstein's equations is populated by strange fauna indeed.
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The paper is organized as follows: In "Closed-time path integral formalism and the generating functional in non-equilibrium QCD" section a brief discussion on the generating functional in non-equilibrium QCD is presented.
We found that variations of ±5% of either mRNA or protein half-life resulted in variations in mean closed time and mean burst size that were always smaller than 5%.
However, mean closed time was lower in induced tgind β2a suggesting that a portion of overexpressed β2a exerts functional action similar to the recombinant channel data presented.
The lack of significant difference in either open or closed times within bursts indicates that the opening/closing kinetics of α1β2γ2 and α3β2γ2 receptors do not differ.
These rate constants were used to calculate the PDFs, mean open and mean closed times in Figure 2. We next investigated whether constitutive activity of these channels influenced the cellular membrane potential (V m).
In typical space-times without closed time-like curves this means that one has, in essence, complete freedom of matter distribution on a space-like hypersurface.
Suppose that one is in a space-time with closed time-like lines, such that certain counterfactual distributions of matter on some neighborhood of a point p are ruled out if one holds that space-time structure fixed.
In the closed-time path integral formulation in non-equilibrium the generating functional in the background field method of QCD is given by Eq. (3).
So we have evidence that there are no closed time-like lines in our world or one remotely like it.
In the closed-time path integral formulation the generating functional in non-equilibrium QCD is given by Eq. (1).
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