[PDF] Top 20 Scalar field dark matter and the Higgs field
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Scalar field dark matter and the Higgs field
... present dark matter abundance and the initial conditions set by the inflationary dynamics require very small scalar field masses, unless the tensor-to-scalar ... See full document
16
Dynamics and Phenomenology of Scalar Field Dark Matter through the Higgs Portal
... consider the case where the field’s potential has a quartic coupling accounting for the dark scalar ...self-interactions. The model assumes an underlying scale invariance such ... See full document
125
Scale-invariant scalar field dark matter through the Higgs portal
... discuss the dynamics and phenomenology of an oscillating scalar field coupled to the Higgs boson that accounts for the dark matter in the ...Universe. ... See full document
31
ν-inflaton dark matter
... both the inflaton and dark matter to be weakly interacting neutral fields, and outside the reach of the present framework of the SM, it is interesting to speculate ... See full document
30
Constraints on mediator-based dark matter and scalar dark energy models using $\sqrt s = 13$ TeV $pp$ collision data collected by the ATLAS detector
... of the inferred limits with the constraints from direct detection ex- periments on (a) the spin-dependent WIMP-neutron or (b) WIMP-proton scattering cross-section in the context of the ... See full document
87
DARK MATTER AND VARIABLE COSMOLOGICAL CONSTANT
... baryonic matter [2]. Evidences for the existence of an unseen ‘dark’ component in the energy density of the universe comes from several independent observations at different length ... See full document
4
A simple model of exotic compact objects : interaction with a scalar field
... on the increasingly sophisticated astronomical ...to the gravitational pull on the surrounding matter, and when the gas molecules in the disk swirl very fast, they heat up ... See full document
68
Unified Models of Dark Energy and Dark Matter
... in the previous chapter comes to aid due to our inability to solve the Einstein equations with all ...Gravitational field equations are highly non-linear and we can solve them only in a few ... See full document
69
Electroweak corrections to dark matter direct detection in a vector dark matter model
... that the NLO corrections can either enhance or suppress the cross ...for the correct interpretation of the viability of the VDM model based on the experimental limits on ... See full document
35
Complex scalar dark matter in a B-L model
... potential and the gauge sector, we obtain all the DM-dominant processes concerning the relic abundance and direct ...with the current experimental constraints without resorting ... See full document
11
Dark Matter Benchmark Models for Early LHC Run-2 Searches: Report of the ATLAS/CMS Dark Matter Forum
... quarks. The third component of the triplet χ b comprises the cosmological ...Within the MFV framework, the other fermions in the flavor triplet can be made sufficiently heavy ... See full document
64
Tritium calibration of the LUX dark matter experiment
... light and charge yields of ER events in LUX are obtained by dividing the mean light and charge sig- nals by the combined energy in each energy ...bin. The re- sult is shown for 180 V/cm ... See full document
15
Radiogenic and Muon-Induced Backgrounds in the LUX Dark Matter Detector
... shields, and field shaping ...estimate the 60 Co production levels in ...From the distribution of results, the expected ac- tivation rate at sea level for 60 Co in Cu is taken to be 62 ... See full document
18
Unified description of dark energy and dark matter within the generalized hybrid metric-palatini theory of gravity
... which the search for an alternative explanation to the observed late-time accelerated expansion of the Universe stands out ...[4,5]. The standard—and simplest—explanation for this ... See full document
13
Tachyon Scalar Field Cosmology
... simplest dark energy candidate is the so-called cosmological constant Λ, whose energy density is constant in time and ...space. The ΛCDM model is fully consistent with observations, explaining ... See full document
119
Complex scalar dark matter in a B-L model
... concerning the existence of dark matter, comes from the cosmic microwave background [8, ...9]. The microwave background was emitted at the time of recombination, epoch when ... See full document
85
Scalar field dark matter with spontaneous symmetry breaking and the $3.5$ keV line
... ) and ( 18 ) are satisfied, the dark scalar never thermalizes with the cosmic plasma and behaves effectively as an oscillating condensate throughout its whole cosmic ...Given ... See full document
6
Export and internationalization field lab
... control and resource commitments (Peter Buckley, The internationalization of the firm ...If the manager does not expect to obtain accurate and reliable information, then he will opt for ... See full document
25
MATERIALS AND METHODS Field samples
... of the 39 samples that were Salmonella-positive by SMT were also Salmonella-positive by the PCR-RVB method, which also detected 15 additional Salmonella-positive ...that the additional 15 ... See full document
5
On the Earth’s magnetic field and the Hall effect
... of the Earth’s magnetic field that depended on the Hall effect as an energy transfer ...mechanism. The purpose of this paper is to demonstrate that the mechanism invoked is unimportant ... See full document
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