Results 41 to 50 of about 41,122 (294)

Unified Description of Dark Energy and Dark Matter within the Generalized Hybrid Metric-Palatini Theory of Gravity

open access: yesUniverse, 2020
The generalized hybrid metric-Palatini theory of gravity admits a scalar-tensor representation in terms of two interacting scalar fields. We show that, upon an appropriate choice of the interaction potential, one of the scalar fields behaves like dark ...
Paulo M. Sá
doaj   +1 more source

Stability of Cauchy horizon in a charged de-Sitter spacetime with dark matter

open access: yesEuropean Physical Journal C: Particles and Fields, 2023
The violation of strong cosmic censorship (SCC) in RNdS black holes by a minimally coupled neutral massless scalar field has recently been discovered. This paper investigates the stability of the Cauchy horizon of a spherically charged de-Sitter black ...
Xue-Ying Nan, Jia Tan, Jie Jiang
doaj   +1 more source

Testing the mean field theory of scalar field dark matter

open access: yesSciPost Physics Proceedings, 2023
Scalar field dark matter offers an interesting alternative to the traditional WIMP dark matter picture. Astrophysical and cosmological simulations are useful to constraining the mass of the dark matter particle in this model. This is particularly true at
Andrew Eberhardt, Alvaro Zamora, Michael Kopp, Tom Abel
doaj   +1 more source

Scalar field dark matter with a cosh potential, revisited [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2019
Dark matter models in which the constituent particle is an ultra-light boson have become part of the mainstream discussion in cosmology and astrophysics.
L. Ureña‐López
semanticscholar   +1 more source

Rotation curves of high-resolution LSB and SPARC galaxies with fuzzy and multistate (ultralight boson) scalar field dark matter [PDF]

open access: yes, 2017
Cold dark matter (CDM) has shown to be an excellent candidate for the dark matter (DM) of the Universe at large scales, however it presents some challenges at the galactic level. The scalar field dark matter (SFDM), also called fuzzy, wave, Bose-Einstein
T. Bernal   +3 more
semanticscholar   +1 more source

A stable finite-volume method for scalar field dark matter [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
We describe and test a family of new numerical methods to solve the Schrödinger equation in self-gravitating systems, e.g. Bose–Einstein condensates or ‘fuzzy’/ultra-light scalar field dark matter.
P. Hopkins
semanticscholar   +1 more source

Scalar-field dark energy nonminimally and kinetically coupled to dark matter [PDF]

open access: yesPhysical Review D, 2019
We provide a general framework for studying the dark energy cosmology in which a scalar field ϕ is nonminimally and kinetically coupled to cold dark matter (CDM).
R. Kase, S. Tsujikawa
semanticscholar   +1 more source

COMPLEX SCALAR FIELD DARK MATTER ON GALACTIC SCALES [PDF]

open access: yesModern Physics Letters A, 2014
The nature of the cosmological dark matter (DM) remains elusive. Recent studies have advocated the possibility that DM could be composed of ultra-light, self-interacting bosons, forming a Bose–Einstein condensate (BEC) in the very early Universe. We consider models which are charged under a global U(1)-symmetry such that the DM number is conserved. It
Rindler-Daller, Tanja, Shapiro, Paul R.
openaire   +2 more sources

Triple unification of inflation, dark energy, and dark matter in two-scalar-field cosmology [PDF]

open access: yesPhysical Review D, 2020
A unified description of inflation, dark energy, and dark matter is presented within a two-scalar-field cosmological model. Inflation, assumed to be of the warm type, is driven by one of the scalar fields, which, shortly after the end of the inflationary
P. M. S'a
semanticscholar   +1 more source

Brief History of Ultra-light Scalar Dark Matter Models

open access: yesEPJ Web of Conferences, 2018
This is a review on the brief history of the scalar field dark matter model also known as fuzzy dark matter, BEC dark matter, wave dark matter, or ultra-light axion. In this model ultra-light scalar dark matter particles with mass m = O(10-22)eV condense
Lee Jae-Weon
doaj   +1 more source

Home - About - Disclaimer - Privacy