[PDF] Top 20 On Gaugino Dominated Dark Matter
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On Gaugino Dominated Dark Matter
... baryonic dark matter and DE for dark ...exotic matter strongly exists in the form of non-baryonic matter, the MSSM is therefore expected to provide a good candidate for the DM component ... See full document
6
1609.05927.pdf
... Dark matter drops out of kinetic equilibrium with standard model particles when the momentum- transfer rate equals the expansion ...as dark matter kinetically decouples from the plasma. ... See full document
8
Dark Matter and Dark Energy in the Universe
... a matter dominated phase when the field oscillates at the minimum of the ...% matter is responsible for the late phase expansion and 23 % matter called Dark Matter is responsible ... See full document
9
HOW TO REVEAL THE NATURE OF DARK MATTER AND DARK ENERGY
... A lepton is an elementary, half-integer spin particle that does not undergo strong interactions but is subject to the Pauli exclusion principle; no two leptons of the same species can be in exactly the same state at the ... See full document
25
No need for dark-matter, dark-energy or inflation, once ordinary matter is properly represented?
... star dominated, age of stars ...of matter. Consider, for example, what would happen to the dark-matter content of a cluster, if each galaxy in it were to vaporize, evenly distributing its mass ... See full document
41
Gravitation, Dark Matter and Dark Energy: The Real Universe
... In contrast superfluids, superconductors and the HQS, have broken U ( ) 1 symmetry and are dominated by collective effects. These quantum fluids are strongly correlated systems, in which the BE correlation ... See full document
71
21-cm observations and warm dark matter models
... warm dark matter models were those of sufficiently massive Standard Model neutrinos (see, ...radiation dominated epoch and homogenized primordial density perturbations on scales below the ... See full document
8
Origin of the Universe, Dark Energy, and Dark Matter
... General relativity is a classical theory, based on continuum mathematics, inevit- ably involving an infinite number of degrees of freedom. General relativity al- lows for finite (closed) universes and infinite (flat and ... See full document
19
The Novel Interaction Model of Dark Energy and Dark Matter
... of Dark Energy is more than the total mass of Dark Matter in the Universe ...of Dark Energy to Dark Matter in the very early Universe? From the viewpoint of ...fluctuations ... See full document
6
Bouncing cosmologies with dark matter and dark energy
... on dark matter and dark energy with a symmetric ...when dark matter dominates for the resulting spectrum to be nearly scale-invariant; however, most of the modes observed today in the ... See full document
23
No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
... Other authors have proposed more exotic alternatives to CDM in which the dynamics of the particles lead naturally to core for- mation on the mass scales of interest. The most popular amongst these is warm dark ... See full document
14
Cosmological Models of the Universe
... for matter, radiation and dark energy dominated each for open k=-1, closed k=1 and flat k=0, to obtain the value of scale factor and time as the evolution proceeds through stages where various types ... See full document
44
Dark Matter 2014
... Using liquid xenon as WIMP target combines sev- eral advantages [30]: the high atomic number A ≈ 131 for an excellent WIMP sensitivity; the high Z = 54 for dense, compact detectors providing self-shielding against ... See full document
9
Halo concentrations and the fundamental plane of galaxy clusters
... central region corresponding to the initially collapsed overdense region. The solution was originally developed for objects totally composed of baryons, and thus, ρ, p, and m are for the gas. However, the non-dimensional ... See full document
15
Searching the Parameters of Dark Matter Halos on the Basis of Dwarf Galaxies’ Dynamics
... Article devoted to searching the parameters of dark matter halos on the base of dwarf galaxies’ dynamics (Messier 32 and Leo I). For doing this, we propose the new approach founded on con- struction the ... See full document
7
Predicted Dark Matter Quantitation in Flat Space Cosmology
... of dark matter-to-visible matter ratios within the most accessible nearby co-moving galaxies, but to determine the average dark matter-to-visible matter ...the dark ... See full document
5
Ground State Nucleon, Dark Energy and Dark Matter
... Only possibility for this transition to happen is finite lifetime of nucleon in respect of such transformations and stimulated emission, developing at some conditions. These conditions realize, when massive ... See full document
9
Dark Matter as a Metric Perturbation
... the matter power spectrum per data from the Sloan Digital Sky Survey, as well as the CMB angular power spectrum per data from WMAP and the Boomerang experiment for ` ≤ 1000, which includes the third ... See full document
23
Cosmoparticle physics of dark matter
... composite dark matter was presented by the model of mirror ...mirror matter can be present in the Universe in the form of elusive mirror objects, having symmetric properties with ordinary ... See full document
15
Ockham, Olbers and dark matter
... Once again the red shift must be considered, since much of the radiation will be from distant matter unless alpha is relatively large. But now the numerical integration code displays a much reduced distortion of ... See full document
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