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We present a model to predict the luminosity function for radio galaxies and their linear size distribution at any redshift. The model takes a black hole mass function and Eddington ratio distribution as input and tracks the evolution of…

星系天体物理 · 物理学 2017-06-28 A. Saxena , H. J. A. Röttgering , E. E. Rigby

It is generally argued that the present cosmological observations support the accelerating models of the universe, as driven by the cosmological constant or `dark energy'. We argue here that an alternative model of the universe is possible…

天体物理学 · 物理学 2009-11-07 J. V. Narlikar , R. G. Vishwakarma , G. Burbidge

The cosmological peculiar velocity field (deviations from the pure Hubble flow) of matter carries significant information on dark energy, dark matter and the underlying theory of gravity on large scales. Peculiar motions of galaxies…

宇宙学与河外天体物理 · 物理学 2013-01-17 Adi Nusser , Enzo Branchini , Martin Feix

We consider light propagation in an inhomogeneous irrotational dust universe with vanishing cosmological constant, with initial conditions as in standard linear perturbation theory. A non-perturbative approach to the dynamics of such a…

广义相对论与量子宇宙学 · 物理学 2016-09-30 Harald Skarke

A systematic survey measuring the submillimetre continuum luminosity in radio galaxies between redshifts z ~ 0.1 - 5 is currently in progress. The first results from observations with the bolometer array SCUBA on the JCMT suggest a trend of…

天体物理学 · 物理学 2007-05-23 D. H. Hughes , J. S. Dunlop , E. N. Archibald , S. Rawlings , S. A. Eales

We calculate the expected number of strongly lensed radio sources in a sample of 6500 sources observed with the Very Large Array as part of the Cosmic Lens All Sky Survey (CLASS) during the first two sessions of its observations. A…

天体物理学 · 物理学 2011-05-23 Asantha R. Cooray

Observations of distant supernovae indicate that the Universe is now in a phase of accelerated expansion the physical cause of which is a mystery. Formally, this requires the inclusion of a term acting as a negative pressure in the…

By assuming the inverse square law of solar wind plasma density as representative of other stars, it is shown that just outside a star the {\it outward} deflection of a passing radio signal at $\nu\approx 1$~GHz (which is capable of…

高能天体物理现象 · 物理学 2025-08-11 Richard Lieu

The standard interpretation of observations such as the peak apparent magnitude of Type Ia supernova made from one location in a lumpy Universe is based on the idealised Friedmann-Lema\^itre Robertson-Walker spacetime. All possible…

宇宙学与河外天体物理 · 物理学 2022-11-24 Obinna Umeh

An alternative model describing the dynamics of a flat Universe without cosmological constant and allowing a gradual change of c with time is proposed. New relationships of redshift vs. distance and cosmic background radiation temperature…

天体物理学 · 物理学 2007-05-23 Juan Casado Gimenez

We have derived the radiative-transfer equation for a point source with a specified intensity and spectrum, originating in the early Universe between the epochs of annihilation and recombination, at redshifts $z_\s =10^8\div 10^4$. The…

天体物理学 · 物理学 2009-11-11 D. I. Nagirner S. L. Kirusheva

Fast radio bursts (FRBs) are very short and bright transients visible over extragalactic distances. The radio pulse undergoes dispersion caused by free electrons along the line of sight, most of which are associated with the large-scale…

宇宙学与河外天体物理 · 物理学 2022-01-19 Steffen Hagstotz , Robert Reischke , Robert Lilow

The first principles analysis of the radiation by an arbitrary source in a flat Friedmann-Robertson-Walker space-time is presented. The obtained analytical solution explicitly shows that the cosmological redshift is not of kinematic origin…

经典物理 · 物理学 2009-07-03 Neil V. Budko

The recent Cosmic Microwave Background (CMB) experiments have shown that the average density of the universe is close to the critical one and the universe is asymptotically flat (Euclidean). Taking into account that the universe remains…

综合物理 · 物理学 2012-07-02 Dimitar Valev

Using a new radio sample, 6C* designed to find radio galaxies at z > 4 along with the complete 3CRR and 6CE sample we extend the radio galaxy K-z relation to z~4.5. The 6C* K-z data significantly improve delineation of the K-z relation for…

天体物理学 · 物理学 2022-03-02 Matt J. Jarvis , Steve Rawlings , Steve Eales , Katherine M. Blundell , Chris J. Willott

An observer stationary with respect to comoving coordinates of the expanding universe should find the redshift distribution to be isotropic. However, a peculiar motion of the observer would introduce a dipole anisotropy in the observed…

宇宙学与河外天体物理 · 物理学 2019-07-15 Ashok K. Singal

Gravitational waves can provide an accurate measurement of the luminosity distance to the source, but cannot provide the source redshift unless the degeneracy between mass and redshift can be broken. This makes it essential to infer the…

宇宙学与河外天体物理 · 物理学 2021-02-24 Suvodip Mukherjee , Benjamin D. Wandelt , Samaya M. Nissanke , Alessandra Silvestri

In an isotropic and homogeneous Hubble expansion, all transverse motion is peculiar. Like the radial peculiar velocities of galaxies, transverse peculiar velocities are a means to trace the density of matter that does not rely on light…

宇宙学与河外天体物理 · 物理学 2018-09-05 Jeremy Darling , Alexandra E. Truebenbach

The Hubble relation between distance and redshift is a purely cosmographic relation that depends only on the symmetries of a FLRW spacetime, but does not intrinsically make any dynamical assumptions. This suggests that it should be possible…

广义相对论与量子宇宙学 · 物理学 2016-11-15 Matt Visser , Celine Cattoen

It is shown that the Hubble constant can be derived from the standard luminosity function of galaxies as well as from a new luminosity function as deduced from the mass-luminosity relationship for galaxies. An analytical expression for the…

宇宙学与河外天体物理 · 物理学 2011-09-20 Lorenzo Zaninetti