Abstract

We consider the possibility that the universe is made of a single dark fluid described by a logotropic equation of state P=Aln⁡(ρ/ρ∗)P=A\ln(ρ/ρ_*), where ρρ is the rest-mass density, ρ∗ρ_* is a reference density, and AA is the logotropic temperature. The energy density εε is the sum of two terms: a rest-mass energy term ρc2ρc^2 that mimics dark matter and an internal energy term u(ρ)=−P(ρ)−Au(ρ)=-P(ρ)-A that mimics dark energy. This decomposition leads to a natural, and physical, unification of dark matter and dark energy, and elucidates their mysterious nature. The logotropic model depends on a single parameter B=A/ρΛc2B=A/ρ_Λc^2 where ρΛρ_Λ is the cosmological density. For B=0B=0, we recover the ΛΛCDM model. Using cosmological constraints, we find that 0≤B≤0.094250\le B\le 0.09425. We consider the possibility that dark matter halos are described by the same logotropic equation of state. When B>0B>0, pressure gradients prevent gravitational collapse and provide halo density cores instead of cuspy density profiles, in agreement with the observations. The universal rotation curve of logotropic dark matter halos is consistent with the observational Burkert profile up to the halo radius. Interestingly, if we assume that all the dark matter halos have the same logotropic temperature BB, we find that their surface density Σ=ρ0rhΣ=ρ_0 r_h is constant. This result is in agreement with the observations where it is found that Σ0=141 M⊙/pc2Σ_0=141\, M_{\odot}/{\rm pc}^2 for dark matter halos differing by several orders of magnitude in size. Using this observational result, we obtain B=3.53×10−3B=3.53\times 10^{-3}. Assuming that ρ∗=ρPρ_*=ρ_P, where ρPρ_P is the Planck density, we predict B=3.53×10−3B=3.53\times 10^{-3}, in perfect agreement with the value obtained from the observations.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.