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Parkes Pulsar Timing Array constraints on ultralight scalar-field dark matter
. The ultralight scalar field dark matter, consisting of extremely light bosons with m∼10-22 eV and often called

Dark energy and dark matter unification via superfluid Chaplygin gas-Einstein condensate (BEC) as dark energy (DE) and an excited state above it as dark matter (DM). The condensate

Statefinder analysis of the superfluid Chaplygin gas model) and an excited state above it as dark matter (DM). The condensate is assumed to have a negative pressure

Some remarks on axion dark matter, dark energy and energy of the quantum vacuum© 2020 World Scientific Publishing Company. In connection with the problem of dark matter, we

Generalization of Abelian Gauge Symmetry, Dark Matter and Cosmological ExpansionGeneralization of Abelian Gauge Symmetry, Dark Matter and Cosmological Expansion

Multidimensional cosmology, constants and transition to new SI units. For the solution with the fluid matter the post-Newtonian parameters β and γ corresponding to the 4-dimensional

Interacting dark sector and the coincidence problem within the scope of LRS Bianchi type I model
interaction between dark energy and dark matter in locally rotationally symmetric (LRS) Bianchi-I space

ASSESSMENT OF MASS FOR STERILE NEUTRINO FROM DATA ON DARK MATTER AND DARK ENERGY be a candidate for the role of dark matter [2]. -132 For the upper mass of the sterile neutrino

Statefinder analysis of the superfluid Chaplygin gas model) and an excited state above it as dark matter (DM). The condensate is assumed to have a negative pressure

Boson dark matter halos with a dominant noncondensed componentWe consider galaxy halos formed by dark matter bosons with mass in the range of about a few tens

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