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相关论文: Causality and the Power Spectrum

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The quantum mechanical generation of hypermagnetic and hyperlectric fields in four-dimensional conformally flat background geometries rests on the simultaneous continuity of the effective horizon and of the extrinsic curvature across the…

高能物理 - 理论 · 物理学 2017-09-13 Massimo Giovannini

Energy injected into the Cosmic Microwave Background at redshifts z<10^6 will distort its spectrum permanently. In this paper we discuss the distortion caused by annihilations of relic particles. We use the observational bounds on…

天体物理学 · 物理学 2009-12-31 Patrick McDonald , Robert J. Scherrer , Terry P. Walker

We calculate the mean power spectrum of galaxies using published power spectra of galaxies and clusters of galaxies. On small scales we use the power spectrum derived from the 2-dimensional distribution of APM galaxies, on large scales we…

The lowest multipole moments of the cosmic microwave background (CMB) are smaller than expected for a scale-invariant power spectrum. One possible explanation is a cutoff in the primordial power spectrum below a comoving scale of $k_c…

天体物理学 · 物理学 2009-11-10 Michael Kesden , Marc Kamionkowski , Asantha Cooray

Future microwave sky surveys will have the sensitivity to detect the kinematic Sunyaev-Zeldovich signal from moving galaxy clusters, thus providing a direct measurement of their line-of-sight peculiar velocity. We show that cluster peculiar…

天体物理学 · 物理学 2009-11-11 Suman Bhattacharya , Arthur Kosowsky

We try to constrain the noncommutativity length scale of the theoretical model given in Ref. [1] using the observational data from ACBAR, CBI and five year WMAP. The noncommutativity parameter is not constrained by WMAP data, however ACBAR…

天体物理学 · 物理学 2009-03-24 Earnest Akofor , A. P. Balachandran , Anosh Joseph , Larne Pekowsky , Babar A. Qureshi

Several satellite missions have uncovered a series of potential anomalies in the fluctuation spectrum of the cosmic microwave background temperature, including: (1) an unexpectedly low level of correlation at large angles, manifested via…

宇宙学与河外天体物理 · 物理学 2022-01-04 Fulvio Melia , Qingbo Ma , Jun-Jie Wei , Bo Yu

Standard cosmology connects the scale generated at late times by the cosmological constant with that generated in early times by the energy dynamics. Assuming dark energy de-coherence occurs during early times when the scale parameter…

天体物理学 · 物理学 2007-05-23 James V. Lindesay , H. Pierre Noyes

The present standard model of cosmology, $\Lambda$CDM, contains some intriguing coincidences. Not only are the dominant contributions to the energy density approximately of the same order at the present epoch, but we note that contrary to…

宇宙学与河外天体物理 · 物理学 2015-05-18 Pim van Oirschot , Juliana Kwan , Geraint F. Lewis

It is shown, that the both angular CMB Doppler spectrum: $C_l$ (Planck space telescope - cosmic microwave background [1]) and the 3D galaxy-galaxy power spectrum: $P(k)$ (Sloan Digital Sky Survey SDSS-II [2]), exhibit a considerable range…

混沌动力学 · 物理学 2015-12-14 A. Bershadskii

Cosmic microwave background measurements have pushed to higher resolution, lower noise, and more sky coverage. These data enable a unique test of the early universe's expansion rate and constituents such as effective number of relativistic…

宇宙学与河外天体物理 · 物理学 2013-08-05 Alireza Hojjati , Eric V. Linder , Johan Samsing

The article addresses a possibility of obtaining cosmologically relevant effects from the quantum nature of the Hubble horizon. Following the observation made by E.~Bianchi and C.~Rovelli in Phys.\ Rev.\ D {\bf 84} (2011) 027502 we explore…

广义相对论与量子宇宙学 · 物理学 2019-09-04 Michal Artymowski , Jakub Mielczarek

Standard cosmology has long been plagued by a number of persistent problems. The origin of the apparent acceleration of the cosmic expansion remains enigmatic. The cosmological constant has been reintroduced as a free parameter with a value…

综合物理 · 物理学 2023-02-28 Jan O. Stenflo

We analyze the limits on resonant particle production during inflation based upon the power spectrum of fluctuations in matter and the cosmic microwave background. We show that such a model is consistent with features observed in the matter…

天体物理学 · 物理学 2009-11-10 G. J. Mathews , D. J. H. Chung , K. Ichiki , T. Kajino , M. Orito

Using the recently obtained holographic cosmic duality, we reached a reasonable quantitative agreement between predictions of the Cosmic Microwave Background Radiation at small l and the WMAP observations, showing the power of the…

高能物理 - 理论 · 物理学 2009-11-10 Jianyong Shen , Bin Wang , Elcio Abdalla , Ru-Keng Su

Cosmological perturbations of sufficiently long wavelength admit a fluid dynamic description. We consider modes with wavevectors below a scale $k_m$ for which the dynamics is only mildly non-linear. The leading effect of modes above that…

宇宙学与河外天体物理 · 物理学 2015-12-09 Diego Blas , Stefan Floerchinger , Mathias Garny , Nikolaos Tetradis , Urs Achim Wiedemann

The global topology of the Universe could, in principle, affect quantum systems through boundary condition constraints. We investigate this connection by analyzing how compact, flat, cosmologically inspired topologies, specifically the…

量子物理 · 物理学 2025-05-14 Evangelos Achilleas Paraskevas , Leandros Perivolaropoulos

We consider a proposal to define the wave function of the Universe as a sum over spacetimes that eventually inflate. In the minisuperspace model, we explicitly show that a simple family of initial conditions, parametrized by a positive real…

广义相对论与量子宇宙学 · 物理学 2022-07-18 Karthik Rajeev

A constraint on the tidal charge generated within a brane world is shown. Using the shadow of a rotating black hole in a brane context in order to describe the M87* parameters recently announced by the Event Horizon Telescope Collaboration,…

广义相对论与量子宇宙学 · 物理学 2020-08-11 Juliano C. S. Neves

We analyze a general mechanism for producing a nearly scale-invariant spectrum of cosmological curvature perturbations during a contracting phase preceding a big bang, that can be entirely described using 4d effective field theory. The…

高能物理 - 理论 · 物理学 2008-11-26 Jean-Luc Lehners , Paul McFadden , Neil Turok , Paul J. Steinhardt
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