Results 31 to 40 of about 468,012 (314)
Recent large-scale peculiar velocity surveys suggest that large matter volumes could be moving with appreciable velocity with respect to the CMB rest frame. If confirmed, such results could conflict with the Cosmological Principle according to which the matter and CMB rest frames should converge on very large scales.
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Thermodynamics of dark energy [PDF]
AbstractThermodynamic properties of dark energy are discussed assuming that dark energy is described in terms of a selfinteracting complex scalar. We first show that, under certain assumptions, selfinteracting complex scalar field theories are equivalent to purely kinetic k‐essence models.
Bilić, Nevenko, Bilić, Neven
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Barrow entropic dark energy: A member of generalized holographic dark energy family
The holographic cut-off, in the formalism of generalized holographic dark energy (HDE), is generalized to depend on LIR=LIR(Lp,L˙p,L¨p,⋯,Lf,L˙f,⋯,a), where Lp and Lf are the particle horizon and future horizon respectively, and a is the scale factor of ...
Shin'ichi Nojiri +2 more
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Dark Energy from Cosmological Energy Conservation
The value of the gravitational wave energy density is unknown. Current progress in gravitational wave detection suggests that the energy density of the stochastic gravitational wave background (SGWB) will be estimated in the next decades. A derivation of
Manuel Uruena Palomo
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Accelerated Universe from Modified Chaplygin Gas and Tachyonic Fluid
A cosmological model with an exotic fluid is investigated. We show that the equation of state of this “modified Chaplygin” gas can describe the current accelerated expansion of the universe.
Hachemi Benaoum
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63 pages, 8 figures. Invited Review for the special issue "The next decade in Dark Matter and Dark Energy" of the new Open Access journal "Physics of the Dark Universe".
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The Dark Energy Survey: more than dark energy – an overview [PDF]
32 pages, 15 figures; a revised Figure 1 and minor changes, to match the published MNRAS ...
Vinu Vikram +156 more
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Dark energy: Staring into darkness [PDF]
The path to understanding dark energy begins with a single question: has it always been the same throughout the history of the Universe?
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Inhomogeneous dark energy [PDF]
11 ...
Ali H. Chamseddine +2 more
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We investigate the possibility of a dark energy component that is scaling with epochs. A phenomenological model is introduced whose energy density depends on the redshift in such a way that a smooth transition among the three dominant phases of the universe evolution (radiation era, matter domination, asymptotic de Sitter state) is achieved. We use the
CAPOZZIELLO, SALVATORE +2 more
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