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The apparent anisotropies of the galaxy clustering in observable redshift space provide a unique opportunity to simultaneously probe cosmic expansion and gravity on cosmological scales via the Alcock--Paczynski effect and redshift-space…

宇宙学与河外天体物理 · 物理学 2015-09-25 Yong-Seon Song , Atsushi Taruya , Akira Oka

The modification of the quantum properties of coherence of photons through their interaction with matter lies at the heart of the quantum theory of light. Indeed, the absorption and emission of photons by atoms can lead to different kinds…

The matter bounce scenario allows for a sizable parameter space where cosmological fluctuations originally exited the Hubble radius when the background energy density was small. In this scenario and its extended versions, the low energy…

宇宙学与河外天体物理 · 物理学 2016-03-02 Yi-Fu Cai , Francis Duplessis , Damien A. Easson , Dong-Gang Wang

The light-scattering spectrum for a Maxwell fluid in a steady state due to the presence of an external temperature gradient is computed. In such a fluid heat conduction is assumed to be governed by the classical Fourier law. The calculation…

统计力学 · 物理学 2007-05-23 M. Lopez de Haro , J. A. del Rio , F. Vazquez

Variability in active galactic nuclei is observed in ultraviolet to X-ray emission based light curves. This could be attributed to orbital signatures of the plasma that constitutes the accretion flow on the putative disk or in the…

高能天体物理现象 · 物理学 2015-06-19 A. Mangalam , P. Mohan

Gamma-ray burst sources are distributed with a high level of isotropy, which is compatible with either a cosmological origin or an extended Galactic halo origin. The brightness distribution is another indicator used to characterize the…

高能天体物理现象 · 物理学 2015-05-26 I. Horvath

We explore how the behavior of galaxy cluster scaling relations are affected by flux-limited selection biases and intrinsic covariance among observable properties. Our models presume log-normal covariance between luminosity (L) and…

天体物理学 · 物理学 2009-11-13 B. Nord , R. Stanek , E. Rasia , A. E. Evrard

Gravitational lensing directly measures mass density fluctuations along the lines of sight to very distant objects. No assumptions need to be made concerning bias, the ratio of fluctuations in galaxy density to mass density. Hence, lensing…

天体物理学 · 物理学 2007-05-23 Joachim Wambsganss , Renyue Cen , Jeremiah P. Ostriker

That light propagating in a gravitational field gets frequency-shifted is one of the basic consequences of any metric theory of gravity rooted in the equivalence principle. At the same time, also a time dependent material's refractive index…

广义相对论与量子宇宙学 · 物理学 2025-03-18 Alessio Belenchia , Felix Spengler , Dennis Rätzel , Daniel Braun

The interaction between refraction from a distribution of inhomogeneous plasma and gravitational lensing introduces novel effects to the paths of light rays passing by a massive object. The plasma contributes additional terms to the…

广义相对论与量子宇宙学 · 物理学 2015-05-27 Adam Rogers

We discuss from the condensed-matter point of view the recent idea that the Poisson fluctuations of cosmological constant about zero could be a source of the observed dark energy. We argue that the thermodynamic fluctuations of Lambda are…

广义相对论与量子宇宙学 · 物理学 2009-11-10 G. E. Volovik

The relativistic effects in cosmological observables contain critical information about the initial conditions and gravity on large scales. Compared to the matter density fluctuation, some of these relativistic contributions scale with…

广义相对论与量子宇宙学 · 物理学 2023-06-14 Ermis Mitsou , Jaiyul Yoo , Matteo Magi

We analyze the frequency shift of photons propagating on an asymptotically flat spacetime describing a collapsing, spherical dust cloud. We focus on the case where the interaction of the photons with the matter can be neglected. Under…

广义相对论与量子宇宙学 · 物理学 2014-12-31 Néstor Ortiz , Olivier Sarbach

The evaluation of the physical parameters or effects such as the luminosity function (LF) or the photometric maximum (PM) for galaxies is routinely modeled by their spectroscopic redshift. Here, we model LF and PM for galaxies by the…

星系天体物理 · 物理学 2018-11-06 Lorenzo Zaninetti

A simple model to explain the phase-dependence of the cyclotron absorption line observed in many X-Ray pulsars is presented. It includes several relativistic effects, namely gravitational redshift, gravitational light deflection, and - most…

天体物理学 · 物理学 2007-05-23 C. Weth

We establish a relationship between the multipoles of the expansion rate fluctuation field $\eta,$ which capture in an accurate way deviations from isotropy in the redshift-distance relation, and the multipoles of the covariant cosmographic…

宇宙学与河外天体物理 · 物理学 2025-01-06 Basheer Kalbouneh , Christian Marinoni , Roy Maartens

We show that, due to the high optical depth of the intergalactic medium to Lyman-alpha photons before the Epoch of Reionization, the Lyman-alpha scattering rate responsible for the Wouthuysen-Field effect from an isolated source will be…

天体物理学 · 物理学 2009-11-13 Jonathan Higgins , Avery Meiksin

We show that the scattering interaction between a high energy electron and a photon can be strongly enhanced by different types of localized plasmons in a non-trivial way. The scattering interaction is predicted by an eigen-response theory,…

光学 · 物理学 2014-01-21 Kin Hung Fung , Anil Kumar , Nicholas X. Fang

For known gravitational lens systems the redshift distribution of the lenses is compared with theoretical expectations for $10^{4}$~Friedmann-Lema\^\i tre~cosmological models, which more than cover the range of possible cases. The…

天体物理学 · 物理学 2011-05-23 Phillip Helbig , Rainer Kayser

Small scale clumps of ionized gas have been suggested by observations in interstellar medium and circumgalactic medium. The propagation of radio signals can be deflected by these plasma clumps, i.e. plasma lensing. One observable…

宇宙学与河外天体物理 · 物理学 2026-03-16 Xinzhong Er , Weishan Zhu , Shude Mao , Dongzi Li
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