Scaling Cosmology
نویسنده
چکیده
We show that with the help of a suitable coupling between dark energy and cold dark matter it is possible to reproduce any scaling solution ρX ∝ ρMa , where ρX and ρM are the densities of dark energy and dark matter, respectively. We demonstrate how the case ξ = 1 alleviates the coincidence problem. Future observations of supernovae at high redshift as well as quasar pairs which are planned to discriminate between different cosmological models will also provide direct constraints on the coupling between dark matter and dark energy.
منابع مشابه
Scaling Relations of Spiral Galaxies and Their Application to Cosmology
The theoretical background for the main scaling relations of spiral galaxies is discussed, and compared with the observational datum. The luminosity–linewidth relation (TFR) is the best determined among those; the sources of scatter of each are discussed. The results of applications of the TFR to Cosmology, using several all–sky samples of galaxies, are summarized. They yield estimates of H◦, o...
متن کاملRelational Motivation for Conformal Operator Ordering in Quantum Cosmology
Operator-ordering in quantum cosmology is a major as-yet unsettled ambiguity with not only formal but also physical consequences. We determine the Lagrangian origin of the conformal invariance that underlies the conformal operator-ordering choice in quantum cosmology. It is particularly naturally and simply manifest in relationalist producttype actions (such as the Jacobi action for mechanics o...
متن کاملA simulated TCDM cosmology cluster catalogue: the NFW profile and the temperature-mass scaling relations
متن کامل
Accelerated expansion in a stochastic self-similar fractal Universe
In a recent paper, a cosmological model based on El Naschie E infinity cantorian spacetime was presented [1]. In that work it was claimed that the present accelerated expansion of the Universe can be obtained as the effect of a scaling law on newtonian cosmology with a certain time dependent gravitational constant (G). In the present work we show that it may be problematic to explain the presen...
متن کاملProbing Cosmology and Galaxy Cluster Structure with the Sunyaev–Zel’dovich Decrement vs. X–ray Temperature Scaling Relation
Scaling relations among galaxy cluster observables, which will become available in large future samples of galaxy clusters, could be used to constrain not only cluster structure, but also cosmology. We study the utility of this approach, employing a physically motivated parametric model to describe cluster structure, and applying it to the expected relation between the Sunyaev-Zel’dovich decrem...
متن کاملGeneralized Statistical Models of Voids and Hierarchical Structure in Cosmology
Generalized statistical models of voids and hierarchical structure in cosmology are developed. The often quoted negative binomial model and the frequently used thermodynamic model are shown to be special cases of a more general distribution that contains a parameter a. This parameter is related to the Lévy index and the Fisher critical exponent , the latter of which describes the power-law fall...
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 2008