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The Cosmological Parameters 2014

The Review of Particle Physics 2014, 2014
Lahav, Ofer, Liddle, Andrew R, Lahav, Ofer; Liddle, Andrew R   +4 more
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Kinetic Jeans instability in FOG framework. [PDF]

Sci Rep
Das M, Atteya A, Karmakar PK.
europepmc   +1 more source

Origins and lifetimes of secular and tidal bars in simulated disc galaxies. [PDF]

Mon Not R Astron Soc
Frosst M, Obreschkow D, Ludlow A, Fraser-McKelvie A.   +3 more
europepmc   +1 more source

Status of the ΛCDM theory: supporting evidence and anomalies. [PDF]

Philos Trans A Math Phys Eng Sci
Peebles PJE.
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Measurement of the Weyl potential evolution from the first three years of dark energy survey data. [PDF]

Nat Commun
Tutusaus I, Bonvin C, Grimm N.
europepmc   +1 more source

DNA as a quantum system in evolution. [PDF]

PLoS One
Garcia NA.
europepmc   +1 more source

Timelike Thin-Shell Evolution in Gravitational Collapse: Classical Dynamics and Thermodynamic Interpretation. [PDF]

Entropy (Basel)
Schubert AG.
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Status of Cosmological Parameters

COSMO-97, 1998
The cosmological parameters that I will discuss are the Hubble parameter H 0 ≡100h km s-1 Mpc-1, the age of the universe t 0, the average density Ω0, and the cosmological constant Λ. The most important recent development is the new analyses based on Hipparchos data indicating that the oldest Globular Clusters in our Galaxy have ages of ∼ 11 Gyr.
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MEASUREMENT OF COSMOLOGICAL PARAMETERS

Science with the New Generation of High Energy Gamma-Ray Experiments, 2006
The study of the cosmic microwave background (CMB) has played a crucial role in establishing a new standard of precision in the determination of cosmological parameters. The full-sky, high-resolution maps of the CMB recently produced by the WMAP space mission, have reinforced the evidence in favor of a fiat universe, dominated by dark matter and dark ...
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Cosmology III: The cosmological parameters

2014
In Chap. 4 and 7, we described the fundamental aspects of the standard model of cosmology. Together with the knowledge of galaxies, clusters of galaxies, and AGNs that we have gained in the other chapters, we are now ready to discuss the determination of the various cosmological parameters. In the course of this discussion, we will describe a number of
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