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Cosmological measure with volume averaging and the vacuum energy problem
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abstract
In this paper, we give a possible solution to the cosmological constant problem. It is shown hat the traditional approach, based on volume weighting of probabilities, leads to an incoherent onclusion: the probability that a randomly chosen observer measures $\Lambda=0$ is exactly equal to 1. Using an alternative, volume averaging measure, instead of volume weighting can explain why the osmological constant is non-zero.
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Cited by 1 Pith paper
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Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling
Bulk flow speeds and directions are fitted to supernova data, and the neutrino-coupled f(R) model gives the largest fitted velocities, but the claim is a comparison of fit parameters rather than a prediction.
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