Results 21 to 30 of about 203,417 (295)

Cosmological Special Theory of Relativity, Cosmological Quantum Physics, Cosmological Uncertainty Principles, Cosmological General Theory of Relativity

open access: yesSSRN Electronic Journal, 2023
In cosmological special relativity theory, we study Maxwell equations, electromagnetic wave equations and functions. In the cosmological special theory of relativity, we study energy?momentum relations, the Klein-Gordon equation and wave functions. If we solve the Klein?Gordon equation, we obtain the Yukawa potential in the cosmological inertial frame.
openaire   +1 more source

Coarse-grained cosmological perturbation theory [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2012
Semi-analytical methods, based on Eulerian perturbation theory, are a promising tool to follow the time evolution of cosmological perturbations at small redshifts and at mildly nonlinear scales. All these schemes are based on two approximations: the existence of a smoothing scale and the single-stream approximation, where velocity dispersion of the ...
Pietroni, Massimo   +3 more
openaire   +4 more sources

Non-minimal coupled warm inflation with quantum-corrected self-interacting inflaton potential

open access: yesEuropean Physical Journal C: Particles and Fields, 2022
In this work, we investigate the non-minimally coupled scenario in the context of warm inflation with quantum-corrected self-interacting potential. We transform the potential in the Jordan frame to the Einstein frame and consider a dissipation parameter ...
Daris Samart   +3 more
doaj   +1 more source

Cosmology: theory [PDF]

open access: yesProceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP 2013), 2014
Plenary talk delivered at the European Physical Society Conference on High Energy Physics, 18-24 July, 2013, Stockholm ...
openaire   +3 more sources

Cosmological Perturbation Theory [PDF]

open access: yesProgress of Theoretical Physics Supplement, 1984
The linear perturbation theory of spatially homogeneous and isotropic universes is reviewed and reformulated extensively. In the first half of the article, a gauge-invariant formulation of the theory is carried out with special attention paid to the geometrical meaning of the perturbation.
Hideo Kodama, Misao Sasaki
openaire   +1 more source

Unimodular Approaches to the Cosmological Constant Problem

open access: yesUniverse, 2023
We review selected aspects of unimodular gravity and we discuss its viability as a solution of the old cosmological constant problem. In unimodular gravity, the cosmological constant is promoted to a global degree of freedom.
Pavel Jiroušek
doaj   +1 more source

Anisotropic Fractional Cosmology: K-Essence Theory

open access: yesFractal and Fractional, 2023
In the particular configuration of the scalar field k-essence in the Wheeler–DeWitt quantum equation, for some age in the Bianchi type I anisotropic cosmological model, a fractional differential equation for the scalar field arises naturally.
José Socorro   +2 more
doaj   +1 more source

Cosmological Spectrum of Two-Point Correlation Function from Vacuum Fluctuation of Stringy Axion Field in De Sitter Space: A Study of the Role of Quantum Entanglement

open access: yesUniverse, 2020
In this work, we study the impact of quantum entanglement on the two-point correlation function and the associated primordial power spectrum of mean square vacuum fluctuation in a bipartite quantum field theoretic system.
Sayantan Choudhury, Sudhakar Panda
doaj   +1 more source

Quantum Fractionary Cosmology: K-Essence Theory

open access: yesUniverse, 2023
Using a particular form of the quantum K-essence scalar field, we show that in the quantum formalism, a fractional differential equation in the scalar field variable, for some epochs in the Friedmann–Lemaı^tre–Robertson–Walker (FLRW) model (radiation and
J. Socorro, J. Juan Rosales
doaj   +1 more source

Perturbation theory in nonstandard cosmology [PDF]

open access: yes, 2019
We study inhomogeneous perturbations away from the strongly homogeneous background cosmology previously studied. The problem is greatly simplified by using the mapping on the inner Schwarzschild solution.
Scharf, Günter
core   +1 more source

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