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[PDF] Top 20 K-mouflage Cosmology: the Background Evolution

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K-mouflage Cosmology: the Background Evolution

K-mouflage Cosmology: the Background Evolution

... on the cosmology of K-mouflage models and leave their gravitational properties for fur- ther ...At the background level and for K-mouflage models leading to ... Voir le document complet

19

K-mouflage Cosmology: Formation of Large-Scale Structures

K-mouflage Cosmology: Formation of Large-Scale Structures

... In the nonlinear regime, we use the spherical collapse to deduce the halo mass function and the deviation of the power spectrum from ...expected the halo mass function is ... Voir le document complet

25

The Quantum Field Theory of K-mouflage

The Quantum Field Theory of K-mouflage

... that the quantum corrections are negligible. We then focus on “healthy” K- mouflage theories which pass the Solar System tests [16], ...satisfy the stringent quantitative constraints of ... Voir le document complet

40

The effective field theory of K-mouflage

The effective field theory of K-mouflage

... that the dark-energy effective-field-theory language which will be used throughout this paper is only a book-keeping device to analyse cosmological pertur- bations around a given background ...In the ... Voir le document complet

38

K-mouflage Cosmology: Formation of Large-Scale Structures

K-mouflage Cosmology: Formation of Large-Scale Structures

... about the dif- ferences between the three types of screening mechanisms at the cosmological ...with the Vainshtein and K-mouflage properties have a modified background ... Voir le document complet

25

Squeezing formalism and canonical transformations in cosmology

Squeezing formalism and canonical transformations in cosmology

... ] the mode functions f ~k (⌘, ~x) = e ik⌘+i~k~ x (1 i/k⌘)/ p 2k, corresponding to the Bunch-Davies vacuum in de Sitter space), the class of ↵-vacua associated to b a f is ... Voir le document complet

85

Dark nuclei. I. Cosmology and indirect detection

Dark nuclei. I. Cosmology and indirect detection

... in the dark sector, has been considered for some ...far, the DM candidate has been assumed to be a hadron of the dark sector, such as a dark meson or a dark ...if the analogy with the ... Voir le document complet

20

On the $k$-regularity of the $k$-adic valuation of Lucas sequences

On the $k$-regularity of the $k$-adic valuation of Lucas sequences

... ν k (u n+1 ) n≥0 is k-regular for every integer k ≥ 2, so that Theorem ...dropping the assumption that k and b are relatively ...if k and b have a common prime factor p such that ... Voir le document complet

12

Cosmology using advanced gravitational-wave detectors alone

Cosmology using advanced gravitational-wave detectors alone

... To calculate the number of detected systems given a set of cosmological and NS mass-distribution parameters, ~ we integrate over this distribution, which is equivalent to integrating ov[r] ... Voir le document complet

23

Projections of the
EU populations by foreign/national background

Projections of the EU populations by foreign/national background

... underestimated. The renewal of the labour force is undoubtedly expected to come from ...migration. The European Union would see its group of persons aged 15-39 years with a national background ... Voir le document complet

38

Background on Fracture Mechanics

Background on Fracture Mechanics

... established the equivalence of Irwin's propagation criterion involving the stress-intensity factor(s) and Grifftith's one involving the energy release ...established the existence of a line ... Voir le document complet

10

Cosmology of hidden sector with Higgs portal

Cosmology of hidden sector with Higgs portal

... from the discovery of electron to quantum mechanics, relativity, their fusion into quantum field theory and finally the Standard Model, a quantum field theory that apparently describes every directly ... Voir le document complet

75

Semantic Background Subtraction

Semantic Background Subtraction

... Over the last two decades, a large number of methods have been proposed for this task (see [1, 2] for ...model the background using low-level features such as color components [3, 4], edges [5], ... Voir le document complet

6

Constructing observables in cosmology : towards new probes of the dark sector

Constructing observables in cosmology : towards new probes of the dark sector

... is the linear power spectrum and P ( 1 ) (k, z) the one-loop correction in the diagrammatic representation (Scoccimarro and Frieman, 1996 ) which depends on coupling between higher-order ... Voir le document complet

181

The Beyond Within: Grotto-Heavens (dongtian) in Taoist Ritual and Cosmology

The Beyond Within: Grotto-Heavens (dongtian) in Taoist Ritual and Cosmology

... for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or ...not. The documents may come from teaching and research institutions in France or abroad, or from ... Voir le document complet

28

Radio background measurements at the Pierre Auger Observatory

Radio background measurements at the Pierre Auger Observatory

... shows the experimental setup. The short dipole powered by a battery was linked to the acquisition system by 300 m of optical ...fiber. The optical receiver converted the optical signal ... Voir le document complet

13

Probing Cosmology with the homogeneity scale of the Universe through large scale structure surveys.

Probing Cosmology with the homogeneity scale of the Universe through large scale structure surveys.

... In cosmology, as discussed in the previous chapter, one of the basic pillars of our understanding of the universe is the Cosmological ...that the universe should be smooth, i.e. ... Voir le document complet

214

Dalitz plot analysis of the decay B[superscript ±]→K[superscript ±]K[superscript ±]K[superscript ∓]

Dalitz plot analysis of the decay B[superscript ±]→K[superscript ±]K[superscript ±]K[superscript ∓]

... on the total number of B  B  pairs, a 0.7% uncertainty due to the modeling of B  B backgrounds, and a ...from the uncertainty on the R q  q sideband extrapolation ...coefficient. ... Voir le document complet

11

Branching Fraction Measurements of Charged B Decays to $K^{*+}K^+K^-, K^{*+}\pi^+K^-, K^{*+}K^+\pi^-$ and $K^{*+}\pi^+\pi^-$ Final States

Branching Fraction Measurements of Charged B Decays to $K^{*+}K^+K^-, K^{*+}\pi^+K^-, K^{*+}K^+\pi^-$ and $K^{*+}\pi^+\pi^-$ Final States

... corresponding background asymme- try A Bkg Dπ of ...only). The systematic error on A K ∗ h 1 h 2 was calculated by considering contributions due to track finding, fit bi- ases, B-background ... Voir le document complet

8

Non-LTE abundances of Mg and K in extremely metal-poor stars and the evolution of [O/Mg], [Na/Mg], [Al/Mg] and [K/Mg] in the Milky Way.

Non-LTE abundances of Mg and K in extremely metal-poor stars and the evolution of [O/Mg], [Na/Mg], [Al/Mg] and [K/Mg] in the Milky Way.

... from the ground level of potassium were reported by Rahman-Attia et ...levels the cross-sections calculated with the help of quantum defect method (Hofsaess, 1979) were ...For the other ... Voir le document complet

10

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