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Mostrando ítems 111-120 de 13064
Generalized AKNS System, Non-vanishing Boundary Conditions and N-Dark-Dark Solitons
(Universidad Nacional de Ingeniería, 2019)
The dark matter profile of the Milky Way: a non-parametric reconstruction
(Iop Publishing Ltd, 2015-04-10)
We present the results of a new, non-parametric method to reconstruct the Galactic dark matter profile directly from observations. Using the latest kinematic data to track the total gravitational potential and the observed ...
Secluded WIMPs, dark QED with massive photons, and the galactic center gamma-ray excess
(Elsevier B.V., 2016-02-01)
We discuss a particular secluded WIMP dark matter model consisting of neutral fermions as the dark matter candidate and a Proca-Wentzel (PW) field as a mediator. In the model that we consider here, dark matter WIMPs interact ...
CCDM model from quantum particle creation: constraints on dark matter mass
(Iop Publishing Ltd, 2014-07-01)
In this work the results from the quantum process of matter creation have been used in order to constrain the mass of the dark matter particles in an accelerated Cold Dark Matter model (Creation Cold Dark Matter, CCDM). ...
Can the dark matter annihilation signal be significantly boosted by substructures?
(IOP Publishing, 2016)
A very general cosmological consideration suggests that, along with galactic dark
matter halos, much smaller dark matter structures may exist. These structures are usually
called ‘clumps’, and their mass extends to 10−6M⊙ ...
Systematic uncertainties from halo asphericity in dark matter searches
(Iop Publishing Ltd, 2015)
A Data Driven Solution to the Dark Matter ProblemA Data Driven Solution to the Dark Matter Problem
(USFQ PRESS, departamento editorial de la Universidad San Francisco de Quito USFQ, 2023)
Stability of the curvature perturbation in dark sectors` mutual interacting models
(ELSEVIER SCIENCE BV, 2009)
We consider perturbations in a cosmological model with a small coupling between dark energy and dark matter. We prove that the stability of the curvature perturbation depends on the type of coupling between dark sectors. ...
GRB Hubble diagram and constraints on a ??(t) CDM model
(Oxford journals, 2013)