Power Spectrum of Velocity Fluctuations in the Universe
نویسنده
چکیده
We investigate the power spectrum of velocity fluctuations in the universe starting from four different measures of velocity: the power spectrum of velocity fluctuations from peculiar velocities of galaxies; the rms peculiar velocity of galaxy clusters; the power spectrum of velocity fluctuations from the power spectrum of density fluctuations in the galaxy distribution; and the bulk velocity from peculiar velocities of galaxies. There are various way of interpreting the observational data: (1) The power spectrum of velocity fluctuations follows a power law, V (k) ∼ k, on large scales, achieves a maximum V (k) ∼ 500 km s at a wavelength λ ∼ 120h Mpc, and declines as V (k) ∝ k on small scales. This type of power spectrum is predicted by a mixed dark matter model with density parameter Ω0 = 1. This model is consistent with all data observed, except the rms peculiar velocity of galaxy clusters. (2) The shape of the power spectrum of velocity fluctuations is similar to that in model (1), but the amplitude is lower (∼ 300 km s at λ ∼ 120h Mpc). This power spectrum is predicted by a low-density cold dark matter model with density parameter Ω0 ≃ 0.3. (3) There is a peak in the power spectrum of velocity fluctuations at a wavelength λ ≃ 120h Mpc and on larger scales the power spectrum decreases with an index n ≃ 1.0. The maximum value of the function V (k) is ∼ 420 km s. This power spectrum is consistent with the power spectrum of the galaxy distribution in the Stromlo-APM redshift survey provided the parameter β is in the range 0.5− 0.6. (4) There is a peak in the power spectrum as in model (3), but on larger scales the amplitude of fluctuations is higher than that estimated starting from the observed power spectrum of galaxies. For the parameter β in the range 0.4− 0.5, the observed rms cluster peculiar velocity is consistent with the rms amplitude of the bulk flow ∼ 340 km s at the scale 60h Mpc. In this case the value of the function V (k) at wavelength λ = 120h Mpc is ∼ 350 km s.
منابع مشابه
تصحیحات طیف با پسزمینه دوسیته در فضای کرین
Gravitational waves are the last unconfirmed prediction of the general relativity. These waves are tiny fluctuations in world frame that dessipate energy throghout space. The gravitatinal waves spectra of fluctuations can be originated from the non-linear effects during different cosmic evolution periods, especially from initially non-linear and excited vacuum state in the very early universe. ...
متن کاملA Slight Excess of Large Scale Power from Moments of the Peculiar Velocity Field
The peculiar motions of galaxies can be used to infer the distribution of matter in the Universe. It has recently been shown that measurements of the peculiar velocity field indicates an anomalously high bulk flow of galaxies in our local volume. In this paper we find the implications of the high bulk flow for the power spectrum of density fluctuations. We find that analyzing only the dipole mo...
متن کاملMass Power Spectrum in a Universe Dominated by the Chaplygin Gas
The mass power spectrum for a Universe dominated by the Chaplygin gas is evaluated numerically from scales of the order of the Hubble horizon to 100 Mpc. The results are compared with a pure baryonic Universe and a cosmological constant model. In all three cases, the spectrum increases with k, the wavenumber of the perturbations. The slope of the spectrum is higher for the baryonic model and sm...
متن کاملA Measurement of the Primordial Power Spectrum from Maxima and Boomerang Data
Model-independent measurements of the primordial power spectrum of matter density fluctuations provide a unique probe of physics in the very early universe, and can provide powerful constraints on inflationary models. We parametrize the primordial power spectrum A2s(k) as an arbitrary function, and measure its binned amplitude from the cosmic microwave background radiation anisotropy (CMB) data...
متن کاملMeasurability of vacuum fluctuations and dark energy
Vacuum fluctuations of the electromagnetic field induce current fluctuations in resistively shunted Josephson junctions that are measurable in terms of a physically relevant power spectrum. In this paper we investigate under which conditions vacuum fluctuations can be gravitationally active, thus contributing to the dark energy density of the universe. Our central hypothesis is that vacuum fluc...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 1997