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 e
V 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