[PDF] Top 20 Calidad en empresas del sector automotriz en Lima Metropolitana
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A dark matter component decaying after recombination: lensing constraints with Planck data
... of dark matter decaying after recombination and argued that such a model is able to reconcile the emerging tension between the cosmological probes in high redshift and low ...from ... See full document
18
Constraints on Dark Energy Models from Selected Galaxy Clusters (S-Z + X-Ray Data) and Gravitational Lensing Data
... luminous matter, 26% of Cold Dark Matter (CDM) and about 70% is a exotic component known as dark energy (DE) which it is traditionally presented as the main responsible for the late ... See full document
34
Cosmological implications of baryon acoustic oscillation measurements
... SN data, these measurements yield impressively tight constraints on the cosmic expan- sion history and correspondingly stringent tests of dark energy ...These data sets also enable precise ... See full document
631
The light photon, dark matter and the whirling of dark matter, the theory of the birth of universe
... Mass and Energy, both are eternal quantities. Any particle having energy; has respective quantity of mass. The various particles are generated from the very basic, the smallest of the smallest, ultimate mass particles, ... See full document
149
Planck intermediate results XLVII Planck constraints on reionization history
... Non-parametric reconstructions of the ionization fraction have also been proposed to probe the reionization history. Such methods are based on exploring reionization parameters in bins of redshift (Lewis et al. 2006). ... See full document
88
Search for dark matter produced in association with a Higgs boson decaying to two bottom quarks in pp collisions at root s=8 TeV with the ATLAS detector
... C. W þ jets and top quark backgrounds In the resolved channel, the W þ jets control region is very similar to the signal region, except that the lepton veto is replaced by the requirement of one isolated muon with p T ... See full document
10
Two-component Dark Matter in the vectorlike hypercolor extension of the Standard Model
... observations. Dark Matter occupies about a quarter of the Universe mass and plays a crucial role in the evolution of ...one component, (for information about such models, see) [4–14] ... See full document
170
Planck 2015 results XXIV Cosmology from Sunyaev Zeldovich cluster counts
... of matter from dark matter ...on dark matter only simulations (Cui et ...CMB constraints hinted at by the di ff erent observations ...of dark matter halos (e.g., ... See full document
35
First constraints on fuzzy dark matter from Lyman alpha forest data and hydrodynamical simulations
... present constraints on the masses of extremely light bosons dubbed fuzzy dark matter from Lyman-α forest ...as dark matter candidates that may resolve some of the current small scale ... See full document
14
Renneby, Malin Nicole (2019): Weak gravitational lensing as a probe of large-scale structure and galaxy formation. Dissertation, LMU München: Fakultät für Physik
... models in post-processing. Substructures were first resolved in N -body simulations twenty years ago (e.g. Ghigna et al., 1998; Klypin et al., 1999) and at present, there exists & 30 different approaches to identify ... See full document
65
Constraints on Dynamical Dark Energy with Precision Cosmological Data
... DOI: 10.4236/jmp.2018.92021 303 Journal of Modern Physics other cosmological probes such as the Cosmic Microwave Background Radiation (CMB) [3], Baryon Acoustic Oscillations (BAO) and Large Scale Structure (LSS) surveys ... See full document
292
On the Planck Scale and Properties of Matter
... the Planck time, taken as the fundamental ...experimental data suggests that the period doubling process takes place in three and four internal degrees of ... See full document
78
Planck intermediate results XLIX Parity violation constraints from polarization data
... The Planck Collaboration acknowledges the support of: ESA; CNES, and CNRS / INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes, ... See full document
19
Dark Matter
... of dark matter wind [44] increase greatly, and kinetic energy of dark matter [45] wind in unit volume increases several tens of times or even several hundreds of ... See full document
33
Markovic, Katarina (2013): Cosmology in the nonlinear domain: warm dark matter. Dissertation, LMU München: Fakultät für Physik
... theory matter power spectrum to the WDM linear theory power spectrum, from which we calculate the Sheth-Tormen mass ...our constraints it would be necessary to have a fitting formula to simulations giving ... See full document
8
Dark Matter without Matter
... DOI: 10.4236/jmp.2018.913147 2337 Journal of Modern Physics forces act in the system in rest of this model, the comoving system is free of forces. The subluminal cosmos expands in free fall; the Einstein elevator prin- ... See full document
83
Constraints on low-mass WIMPs from the EDELWEISS-III dark matter search
... to select interactions taking place inside a large fiducial fraction of each detector. During the third stage of the EDELWEISS experiment, a ten-month-long run in low-background conditions was carried out with an array ... See full document
5
New constraints on the free streaming of warm dark matter from intermediate and small scale Lyman alpha forest data
... However, whereas the temperature degeneracy with the free streaming length comes as no surprise, the mean flux degeneracy might not be naively expected (bottom left panel of Fig. 3). Since this degeneracy has a similar ... See full document
51
Astrophysical Constraints on Dark Matter
... We use the high resolution extended DM halo profile obtained in Gao et al. [2012] and model the WIMP spectrum with the DMFit package Jeltema & Pro- fumo [2008] as implemented in the Science Tools analysis software. ... See full document
26
Effect of the Dilaton Field on Deflection Angle of Massive Photons by Black Holes in Einstein-Maxwell-Dilaton-Axion Theory
... mysterious, dark matter is one of the greatest enigmas of astro- physics and ...of dark matter are shown by SISSA which disproves the empirical relations in support of alternative theories ... See full document
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