[PDF] Top 20 Un modelo de enseñanza participativa del Derecho Constitucional
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Energy-Momentum Tensor and Parameters in Cosmological Model
... dark energy are attracting the attention of scientists around the world, becoming the hottest topic, challenging traditional standard models of particle and ...dark energy is using the equation of state P = ... See full document
17
Bulk Viscous Anisotropic Cosmological Models with Dynamical Cosmological Parameters G and ∧
... negative energy field in an expanding ...of cosmological models with causal ...V cosmological models with varying gravitational and cosmologi- cal ...viscous cosmological models with variable ... See full document
116
Bianchi Type-VIo Wet Dark Fluid Cosmological Model with Linearly Varying Deceleration Parameter in f(R,T) Gravity
... VIo cosmological model with Wet Dark Fluid (WDF) in f(R,T) gravity , where R is the Ricci scalar and T the trace of stress energy-momentum tensor, in the context of late time ... See full document
7
Constraints on Dynamical Dark Energy with Precision Cosmological Data
... IPL model also leaves important imprints on the CMB power spectrum and the evolution of matter ...same parameters, a change in cosmological distances is reflected in a shift of the position of the ... See full document
292
The gauge-invariant canonical energy-momentum tensor
... Typical examples of measurable non-local quantities in Quantum ChromoDynamics (QCD) are parton distribution functions (PDFs) whose gauge invariance is ensured by a Wilson line along a path determined by the factorization ... See full document
9
Higgs-radion phenomenology in stabilized RS models
... In all the main radion production processes, there are contributing Feynman diagrams involving off- shell fermions. The radion can be emitted from various fermion currents containing off-shell fermion propagators in ... See full document
8
The Cosmological Constant: 2nd Order Quantum Mechanical Correction to the Newton Gravity
... pressure tensor density (CPTD) that in the classical limit leads to the cosmo- logical constant ...classical cosmological constant is set to ze- ro, the model shows, that exists a residual ... See full document
8
Energy Momentum Tensor for Photonic System
... Now, it is well known that the energy momentum tensor is of fundamental importance in the study of gravitational physics. This parameter is related to the characteristics of gravity, as seen from ... See full document
6
Constraining Cosmological Parameters using Sunyaev-Zel'dovich cluster surveys
... * . However, since we will only restrict ourselves to a qualitative discussion we will not incorporate this effect. The parameter could model nongravitational heat input. Since smaller clusters 共 that is, groups ... See full document
56
On the effective Stefan-Boltzmann law and the thermodynamic origin of the initial radiation density in warm inflation
... radiation energy density should be assumed to be finite at the starting point of the warm ...radiation energy den- sity, we derive an effective Stefan-Boltzmann law by considering the non-vanishing trace of ... See full document
6
Towards Energy Discretization in Quantum Cosmology
... In this article we analyzed the consequences of an alternative equation for quantum cosmology which was established in the context of TEGR. The standard way to introduce QC is by means the Wheeler-DeWitt equation. ... See full document
13
Functions of State for Spinor Gas in General Relativity
... The energy momentum tensor of perfect fluid is a simplified but successful model in astrophysics. In this paper, assuming the particles driven by gravity and moving along geodesics, we derived ... See full document
36
Mana, Annalisa (2013): Optically selected galaxy clusters as a cosmological probe. Dissertation, LMU München: Fakultät für Physik
... The correlation function is one of the best statistical tools to measure quantitatively the clustering of objects in a sample. Correlation statistic methods are an impor- tant tool for relating galaxies and clusters to ... See full document
12
Anisotropic Dark Energy Cosmological Model in Lyra Geometry
... dark energy in Lyra Geometry. Shchigolev et al. [42] investigated Cosmological models with a varying term in Lyra’s ...dark energy model in Lyra manifold and Vacuum expansion in arbitrary ... See full document
42
Tomography and gravitational radii for hadrons by three-dimensional structure functions
... Abstract. Three-dimensional tomography of hadrons can be investigated by general- ized parton distributions (GPDs), transverse-momentum-dependent parton distributions (TMDs), and generalized distribution ... See full document
37
On the energy-momentum tensor of light in strong fields : an all optical view of the Abraham-Minkowski controversy
... Theories of non-linear vacuum electrodynamics give us the opportunity to approach the Abraham-Minkowski debate from an entirely new perspective, using an all-optical set up. In such theories the vacuum acts as a ... See full document
10
Kinetic equilibrium and relativistic thermodynamics
... total energy-momentum four ...ergy momentum vector and not only on its absolute ...the energy-momentum vector, but for interacting bod- ies we should consider the ... See full document
21
Some Discussion of Gravitational constant and cosmological constant Using Bianchi Type-I cosmological Model
... .The term Λ arises naturally in general relativistic quantum field theory, where it is interpreted as the energy density of the vacuum[1-4].Some authors [5-9] argued for the dependence of Λ . Bianchi Type-I models ... See full document
7
Energy-momentum tensor correlation function in Nf = 2 + 1 full QCD at finite temperature
... This work was in part supported by JSPS KAKENHI Grant Numbers JP25800148, JP26287040, JP26400244, JP26400251, JP15K05041, JP16H03982, and JP17K05442. This research used compu- tational resources of HA-PACS and COMA ... See full document
17
The solution to the cosmological constant problem
... Dark Energy and the Cosmological Constant, a new approach to the ground state of empty space is ...resulting model for the vacuum state associated with empty space proposes a crystalline-like texture ... See full document
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