Is the evidence for dark energy secure?
Subir Sarkar (Oxford U.)

TL;DR
This paper critically examines the evidence for dark energy, highlighting alternative explanations and emphasizing the lack of direct, definitive proof for its existence within current cosmological models.
Contribution
It challenges the prevailing view of dark energy by exploring alternative models and emphasizing the uncertainties and assumptions in interpreting observational data.
Findings
CMB data can fit models without dark energy under certain conditions
Large-scale structure data can be explained with hot dark matter like neutrinos
Inhomogeneous cosmological models may account for observations without dark energy
Abstract
Several kinds of astronomical observations, interpreted in the framework of the standard Friedmann-Robertson-Walker cosmology, have indicated that our universe is dominated by a Cosmological Constant. The dimming of distant Type Ia supernovae suggests that the expansion rate is accelerating, as if driven by vacuum energy, and this has been indirectly substantiated through studies of angular anisotropies in the cosmic microwave background (CMB) and of spatial correlations in the large-scale structure (LSS) of galaxies. However there is no compelling direct evidence yet for (the dynamical effects of) dark energy. The precision CMB data can be equally well fitted without dark energy if the spectrum of primordial density fluctuations is not quite scale-free and if the Hubble constant is lower globally than its locally measured value. The LSS data can also be satisfactorily fitted if there…
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