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相关论文: Dynamical suppression of non-adiabatic modes

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The Cosmological Principle states that the universe is statistically isotropic and homogeneous on large length scales, typically $\gtrsim 70$Mpc. A detection of significant deviation would help us falsify the simplest models of inflation.…

宇宙学与河外天体物理 · 物理学 2025-08-26 Bhuwan Joshi , Rahul Kothari

We show that the difference between the theoretically expected and measured by WMAP amplitude of the quadrupole fluctuations of CMB can be related to the impact of the anisotropic curvature of the homogeneous universe dominated by the dark…

天体物理学 · 物理学 2008-11-26 M. Demiański , A. G. Doroshkevich

We numerically investigate gauge field instabilities in anisotropic SU(2) plasmas using weak field initial conditions. The growth of unstable modes is stopped by non-abelian effects for moderate anisotropy. If we increase the anisotropy the…

高能物理 - 唯象学 · 物理学 2008-11-26 D. Bodeker , K. Rummukainen

Contaldi et al. [1] have suggested that an initial period of kinetic energy domination in single field inflation may explain the lack of CMB power at large angular scales. We note that in this situation it is natural that there also be a…

天体物理学 · 物理学 2009-08-13 John F. Donoghue , Koushik Dutta , Andreas Ross

We consider various sets of Vlasov-Fokker-Planck equations modeling the dynamics of charged particles in a plasma under the effect of a strong magnetic field. For each of them in a regime where the strength of the magnetic field is…

偏微分方程分析 · 数学 2020-06-30 Maxime Herda , Luis Miguel Rodrigues

Entropic Dynamics is a framework in which dynamical laws are derived as an application of entropic methods of inference. No underlying action principle is postulated. Instead, the dynamics is driven by entropy subject to the constraints…

量子物理 · 物理学 2015-09-11 Ariel Caticha

Nonadiabatic transitions are known to be major loss channels for atoms in magnetic traps, but have thus far not been experimentally reported upon for trapped molecules. We have observed and quantified losses due to nonadiabatic transitions…

原子物理 · 物理学 2009-09-10 Moritz Kirste , Boris Saratakov , Melanie Schnell , Gerard Meijer

The evolution of the non-adiabatic pressure perturbation during inflation driven by two scalar fields is studied numerically for three different types of models. In the first model, the fields have standard kinetic terms. The other two…

宇宙学与河外天体物理 · 物理学 2013-03-14 C. van de Bruck , S. Vu

The systematic analysis of non-adiabatic effect on convective mode has been conducted using wave energy relation. In the adiabatic analysis, the "propagation diagram" for convective mode is proposed as a useful tool to see its behavior. In…

太阳与恒星天体物理 · 物理学 2026-03-12 Hiroyasu Ando

The South Pole Telescope (SPT), Atacama Cosmology Telescope (ACT), and Wilkinson Microwave Anisotropy Probe (WMAP) have each reported measurements of the cosmic microwave background's (CMB) angular power spectrum which favor the existence…

宇宙学与河外天体物理 · 物理学 2013-05-30 Dan Hooper , Farinaldo S. Queiroz , Nickolay Y. Gnedin

Injection of high energy electromagnetic particles around the recombination epoch can modify the standard recombination history and therefore the CMB anisotropy power spectrum. Previous studies have put strong constraints on the amount of…

宇宙学与河外天体物理 · 物理学 2019-12-19 Sandeep Kumar Acharya , Rishi Khatri

The standard inflationary model presents a simple scenario within which the homogeneity, isotropy and flatness of the universe appear as natural outcomes and, in addition, fluctuations in the energy density are originated during the…

天体物理学 · 物理学 2023-03-08 E. Martinez-Gonzalez , P. Vielva

Within the context of supersymmetric hybrid inflation, we study a multiple-stage inflationary scenario that can generate a primordial spectrum of adiabatic density perturbations with a break at $k_b \simeq 0.05 h Mpc^{-1}$. The presence of…

高能物理 - 唯象学 · 物理学 2007-05-23 Mairi Sakellariadou , Nikos Tetradis

There is an apparent power deficit relative to the $\Lambda$CDM prediction of the CMB spectrum at large scales, which, though not yet statistically significant, persists from WMAP to Planck data. Proposals that invoke some form of initial…

广义相对论与量子宇宙学 · 物理学 2016-01-12 Pisin Chen , Yu-Hsiang Lin

The recent Planck data on the power spectrum of temperature anisotropies of the cosmic microwave background marginally support deviations from the $\Lambda$CDM model at several multipoles. With a view towards current and forthcoming…

宇宙学与河外天体物理 · 物理学 2017-12-27 Spyros Sypsas

Recently formulated model of highly-anisotropic and strongly dissipative hydrodynamics is used in 3+1 dimensions to study behavior of matter produced in ultra-relativistic heavy-ion collisions. We search for possible effects of the initial…

核理论 · 物理学 2012-06-22 Radoslaw Ryblewski , Wojciech Florkowski

We study the Cosmic Microwave Background (CMB) anisotropies produced by cosine-type quintessence models. In our analysis, effects of the adiabatic and isocurvature fluctuations are both taken into account. For purely adiabatic fluctuations…

天体物理学 · 物理学 2009-11-06 Masahiro Kawasaki , Takeo Moroi , Tomo Takahashi

The nonlinear collisional dynamics of coupled driven plasma waves in the presence of background dissipation is studied analytically within kinetic theory. Sufficiently near marginal stability, phase space correlations are poorly preserved…

等离子体物理 · 物理学 2023-05-18 N. M. Pham , V. N. Duarte

The implications of the WMAP (Wilkinson Microwave Anisotropy Probe) third year data for inflation are investigated using both the slow-roll approximation and an exact numerical integration of the inflationary power spectra including a…

天体物理学 · 物理学 2009-11-11 Jerome Martin , Christophe Ringeval

We study several anisotropic inflationary models and their implications for the observed violation of statistical isotropy in the CMBR data. In two of these models the anisotropy decays very quickly during the inflationary phase of…

宇宙学与河外天体物理 · 物理学 2017-09-15 Pranati K. Rath , Tanmay Mudholkar , Pankaj Jain , Pavan K. Aluri , Sukanta Panda