Results 11 to 20 of about 110,473 (324)
Scalar field dark matter and the Higgs field
We discuss the possibility that dark matter corresponds to an oscillating scalar field coupled to the Higgs boson. We argue that the initial field amplitude should generically be of the order of the Hubble parameter during inflation, as a result of its ...
O. Bertolami +2 more
doaj +4 more sources
Scalar Field (Wave) Dark Matter [PDF]
Recent high-quality observations of dwarf and low surface brightness (LSB) galaxies have shown that their dark matter (DM) halos prefer flat central density profiles.
Matos, T., Robles, Victor H.
core +2 more sources
Halos of unified dark matter scalar field [PDF]
We investigate the static and spherically symmetric solutions of Einstein's equations for a scalar field with non-canonical kinetic term, assumed to provide both the dark matter and dark energy components of the Universe. In particular, we give a prescription to obtain solutions (dark halos) whose rotation curve v_c(r) is in good agreement with ...
Daniele Bertacca +2 more
openalex +4 more sources
Effective field theory and scalar triplet dark matter
We discuss an extension of the standard model with a real scalar triplet, T, including non-renormalizable operators (NROs) up to d = 6. If T is odd under a Z 2 symmetry, the neutral component of T is a good candidate for the dark matter (DM) of the ...
Carolina Arbeláez +4 more
doaj +4 more sources
Scalar field dark matter in hybrid approach [PDF]
We develop a hybrid formalism suitable for modeling scalar field dark matter, in which the phase-space distribution associated to the real scalar field is modeled by statistical equal-time two-point functions and gravity is treated by two stochastic ...
Friedrich, Pavel, Prokopec, Tomislav
core +4 more sources
Symmetron scalar fields: Modified gravity, dark matter, or both? [PDF]
27 pages, 4 figures.
Clare Burrage +3 more
openalex +4 more sources
Cosmological constraints on scalar field dark matter [PDF]
This paper aims to put constraints on the parameters of the Scalar Field Dark Matter (SFDM) model, when dark matter is described by a free real scalar field filling the whole universe, plus a cosmological constant term. By using a compilation of 51 [Formula: see text] data and 1048 Supernovae data from Panteon, a mass range for the scalar field was ...
A. A. Escobal +2 more
openaire +3 more sources
The quantum character of the Scalar Field Dark Matter [PDF]
ABSTRACT The scalar field dark matter (SFDM) model, also called Fuzzy, Wave, Bose–Einstein, and Ultra-light Dark Matter, has received a lot of attention because it has been able to provide simpler and more natural explanations for various features of galaxies, such as the number of satellite galaxies and the cusp-core problem.
Tonatiuh Matos
openalex +3 more sources
Search for Chameleon Scalar Fields with the Axion Dark Matter Experiment [PDF]
Scalar fields with a "chameleon" property, in which the effective particle mass is a function of its local environment, are common to many theories beyond the standard model and could be responsible for dark energy. If these fields couple weakly to the photon, they could be detectable through the afterglow effect of photon-chameleon-photon transitions.
G. Rybka +13 more
openalex +4 more sources
Can dark matter be a scalar field? [PDF]
In this paper we study a real scalar field as a possible candidate to explain the dark matter in the universe. In the context of a free scalar field with quadratic potential, we have used Union 2.1 SN Ia observational data jointly with a Planck prior over the dark matter density parameter to set a lower limit on the dark matter mass as $m\geq0.12H_0 ...
Jesus, J. F. +3 more
openaire +4 more sources

