Results 1 to 10 of about 2,527 (263)
I discuss the classical cosmological tests-- angular size-redshift, flux-redshift, and galaxy number counts-- in the light of the cosmology prescribed by the intepretation of CMB anisotropies. The discussion is somewhat of a primer for physicists, with emphasis upon the possible systematic uncertainties in the observations and their interpretation ...
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Despite the title, I am afraid that I will not be able to really do justice to the broad topic I was given to review. But I will show the current striking level of precise consistency between the CMB and LSS data \textit{within the \LCDM\ theoretical framework} (with the acronyms CMB and LSS standing for Cosmic Microwave Background and Large Scale ...
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Observations in quantum cosmology
Abstract In this review, we focus on whether a canonical quantization of general relativity can produce testable predictions for cosmology. In particular, we examine how this approach can be used to model the evolution of primordial perturbations. This program of quantum geometrodynamics, first advocated by John Wheeler and Bryce DeWitt,
Leonardo Chataignier +2 more
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Machine learning for observational cosmology
Abstract An array of large observational programs using ground-based and space-borne telescopes is planned in the next decade. The forthcoming wide-field sky surveys are expected to deliver a sheer volume of data exceeding an exabyte.
Kana Moriwaki +2 more
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Cosmological observations in non-local F(R) cosmology [PDF]
12 pages, 7 figures, will be published in Astrophysics and space ...
Farajollahi, H. +3 more
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Predicting cosmological observables with PyCosmo
Astronomy and Computing ...
F. Tarsitano +9 more
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“Observables” in causal set cosmology [PDF]
LaTeX, 1+19 pages, 2 ...
Brightwell, Graham +4 more
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Observational cosmology in macroscopic gravity [PDF]
22 ...
Clifton, T, Coley, A, Hoogen, RVD
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Reconciling a decelerating Universe with cosmological observations [PDF]
Asta Heinesen
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Modified Friedmann cosmologies—Theory and observations
We investigate a class of Cardassian scenarios of the universe evolution in notions of the qualitative theory of dynamical systems. This theory allows us to analyze all solutions for all possible initial conditions on the phase plane. In the Cardassian models we find that big-rip singularities are present as a typical behavior in the future if $n<0$.
Szydłowski, Marek, Czaja, Wojciech
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