[PDF] Top 20 Distribution of Mass and Energy in Five General Cosmic Models
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Distribution of Mass and Energy in Five General Cosmic Models
... The results illustrated in Figures 1(a)-(c) are supported by those displayed in Figures 2(a)-(c) which show the distributions of the universe horizon volume in the general models in the ranges up to t = 0.5 ... See full document
8
Distribution of Mass and Energy in Closed Model of the Universe
... It is worthy now to study the distributions of equivalent mass of radiation, mass of matter and equivalent mass of dark energy within the horizon volume of the universe to get deeper sig[r] ... See full document
11
Oxytree pruned biomass torrefaction - mathematical models of the influence of temperature and residence time on fuel properties improvement
... The common assumption is that the amount of biomass produced during the pruning treatment of the Oxytree plantation is too small to be economically used for energy purposes. Nevertheless, assuming that the ... See full document
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Particle spectra and mass composition in the ultra-high energy region in the framework of the Galactic origin of cosmic rays
... cut-off energy. The highly inhomogeneous (fractal-like) distribution of matter and magnetic fields in the Galaxy that leads to extremely large free paths of particles (so called “L´evy flights”), along with ... See full document
5
Ultra-high-energy cosmic rays mass composition studies with the Telescope Array Surface Detector data
... parameter distribution histograms for all the energy ...atomic mass ln A is shown in comparison with the Telescope array hybrid re- sults ...atomic mass ln A is shown in comparison with the ... See full document
6
Vertical distribution of dry mass in cereals straw and its loss during harvesting
... renewable energy but still its energetic value is strongly dependent on the moisture content (Tavakoli et ...of mass applied to the soil (Pabin et ...prognostic models used to assess the increase of ... See full document
7
Numerical Study of the Electron Lateral Distribution in Atmospheric Showers of High Energy Cosmic Rays
... the mass of cosmic rays cannot be measured ...the cosmic particles at very high energy, it is necessary to study the characteristics of the distribution of secondary particles created ... See full document
5
The Measure Concentration of Convex Geometry in a Quasi Banach Spacetime behind the Supposedly Missing Dark Energy of the Cosmos
... x R ε x fixes the width of parallel slices. That way we can conclude that the volume ‘mass’ distribution is Gaussian and for a fixed slab width almost 95.5% of the mass lies in this slice [58]. Now ... See full document
6
Measuring Cosmic Acceleration And Constraining Dark Energy Models With Transients Discovered In The Dark Energy Survey
... electron energy distribution inferred from the radio+X-ray data modeling discussed in M17 and in A17 is better de- scribed by a shallow power-law (index p ∼ ... See full document
183
Stationary mass distribution and non locality in models of coalescence and shattering
... the energy of the colliding parti- cles [11, ...size distribution of the fragmented parti- cles is typically a power law distribution [13–16], repro- ducible in simple tractable models [17, ... See full document
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Modelling the cosmic spectral energy distribution and extragalactic background light over all time
... The case for the second axiom is stronger. The recent advent of integral field spectroscopic observations has enabled more robust determination of the mass growth history of galaxies. McDermid et al. (2015) found ... See full document
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Cosmological Distances in Five General Cosmic Models
... the cosmic distances mentioned above are most com- monly used in many cosmological ...specifying cosmic distances, interesting es- timations were computed in the general models at the present ... See full document
6
General Derivation of Mass Energy Relation without Electrodynamics or Einstein’s Postulates
... the Energy-Mass relation E ≈ mc 2 was obtained by many differing electrostatic and electromagnetic considerations—and related to the mass of a stationary or moving point-like ...to mass in ... See full document
6
The distribution of cosmic ray neutrons in the atmosphere
... xLi iiCalibration of neutron density detectors 175 iiiNeutron density measurements in flight DN3 179 ivNormalisation to measurements by Miles 1964 180 v Comparison with the results of Li[r] ... See full document
289
Testing of the VENUS 4.12, DPMJET 2.55, QGSJET II-03 and SIBYLL 2.3 hadronic interaction models via help of the atmospheric vertical muon spectra
... this energy estimated with help of the fluorescence ...these models should be thoroughly tested. Usually these models are tested with the help of the accelerator data at small values ( ∼ 0) of the ... See full document
11
Exergy Analysis of Heat Energy Transfer and Distribution
... The paper presents the fundamental laws which have to be known in order to describe the exergy conditions in a heating system. An analysis of the »Šalelška dolina« district-hea ting system is made. The parameters ... See full document
8
Antarctic intermediate water mass formation in ocean general circulation models
... ocean general circulation model simulations with coarse resolution and a z-coordinate, a mid-depth salinity minimum characteristic of this intermediate water is ...water mass and which are the source ... See full document
33
Cosmic Dark Energy Density from Classical Mechanics and Seemingly Redundant Riemannian Finitely Many Tensor Components of Einstein’s General Relativity
... We determine the limit of the ratio formed by the independent components of the Riemann tensor to the non-zero component as space dimensionality tends to infinity and find it to be 12. Subse- quently we use this result ... See full document
5
Cosmic Ray Interaction Models: an Overview
... The energy of the primary particle is reconstructed from the measured lateral density of charged particles (mostly, elec- trons and positrons) while the particle type is inferred from the relative fraction of ... See full document
7
Study of muons in extensive air showers from ultra-high energy cosmic rays measured with the Telescope Array experiment
... threshold energy of air shower particles ( ∼ 10 MeV for TA SD and 300 MeV for Auger SD) and R conditions are ...lateral distribution of the data falls down slower than the MC on the high muon pu- rity ... See full document
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