87 research outputs found
A Critique of Supernova Data Analysis in Cosmology
Observational astronomy has shown significant growth over the last decade and
has made important contributions to cosmology. A major paradigm shift in
cosmology was brought about by observations of Type Ia supernovae. The notion
that the universe is accelerating has led to several theoretical challenges.
Unfortunately, although high quality supernovae data-sets are being produced,
their statistical analysis leaves much to be desired. Instead of using the data
to directly test the model, several studies seem to concentrate on assuming the
model to be correct and limiting themselves to estimating model parameters and
internal errors. As shown here, the important purpose of testing a cosmological
theory is thereby vitiated.Comment: v2: Revised, comments and references added; Published version
[vailable at http://www.raa-journal.org/raa/index.php/raa/article/view/539
The lighter side of gravity: How Swami Gurutwananda received enlightenment?
This article does not have an abstract
Cosmology: past, present and future
This is a broad-brush review of the development of cosmology during the twentieth century. The 'past' deals with the first nine decades of the century while the 'present' deals with the last decade. Although technological achievements have helped the astronomer in better viewing the universe, a 'final' understanding still eludes the search for the correct cosmological model. The article ends with a list of unsolved questions which the 'future' may eventually answer
The quasi-steady state cosmology: theory and observations
This is a review of an alternative cosmology, recently proposed by Fred Hoyle, Geoffrey Burbidge and this author. It begins with a brief discussion of why one needs an alternative cosmology, when the standard hot big bang cosmology is claimed to be doing well. It is argued that the observational and theoretical constraints on the standard big bang cosmology, from various directions, leave a very narrow window, if any, in the parameter space of plausible models. There is thus a strong case for alternative cosmologies. The rest of the review concentrates on one alternative, the quasi steady state cosmology (QSSC) and summarises the recent work on this model. This includes, the theoretical formulation and simple exact solutions of the basic equations, their relationship to various observations, the stability of solutions and the toy model for understanding the growth of structures in the Universe
Einstein's legacy: relativistic cosmology
This review gives a historical account of how cosmology has developed since the 1917 paper of Albert Einstein. Today it is a frontier level science drawing on contemporary astronomy as well as contemporary physics, stretching both as far as extrapolations will permit. Thanks to numerous observations at different wavelengths, cosmologists today have their plates full. Extrapolations of laboratory tested physics are called for to understand all information within the framework of a standard model. The success and shortcomings of this approach are briefly discussed against the historical backdrop
Comparison of cosmological models using Bayesian theory
Using the Bayesian theory of model comparison, a new cosmological model due to John and Joseph [M. V. John and K. Babu Joseph, Phys. Rev. D 61, 87304 (2000)] is compared with the standard \Omega_{\Lambda} \neq 0 cosmological model. Their analysis based on the recent apparent magnitude-redshift data of Type Ia supernovas found evidence against the new model; our more careful analysis finds instead that this evidence is not strong. On the other hand, we find that the angular size-redshift data from compact (milliarcsecond) radio sources do not discriminate between the two models. Our analysis serves as an example of how to compare the relative merits of cosmological models in general, using the Bayesian approach
Cosmology and Cosmogony in a Cyclic Universe
In this paper we discuss the properties of the quasi-steady state
cosmological model (QSSC) developed in 1993 in its role as a cyclic model of
the universe driven by a negative energy scalar field. We discuss the origin of
such a scalar field in the primary creation process first described by F. Hoyle
and J. V. Narlikar forty years ago. It is shown that the creation processes
which takes place in the nuclei of galaxies are closely linked to the high
energy and explosive phenomena, which are commonly observed in galaxies at all
redshifts.
The cyclic nature of the universe provides a natural link between the places
of origin of the microwave background radiation (arising in hydrogen burning in
stars), and the origin of the lightest nuclei (H, D, He and He). It
also allows us to relate the large scale cyclic properties of the universe to
events taking place in the nuclei of galaxies. Observational evidence shows
that ejection of matter and energy from these centers in the form of compact
objects, gas and relativistic particles is responsible for the population of
quasi-stellar objects (QSOs) and gamma-ray burst sources in the universe.
In the later parts of the paper we briefly discuss the major unsolved
problems of this integrated cosmological and cosmogonical scheme. These are the
understanding of the origin of the intrinsic redshifts, and the periodicities
in the redshift distribution of the QSOs.Comment: 51 pages including 1 figur
The unexpected resurgence of Weyl geometry in late 20-th century physics
Weyl's original scale geometry of 1918 ("purely infinitesimal geometry") was
withdrawn by its author from physical theorizing in the early 1920s. It had a
comeback in the last third of the 20th century in different contexts: scalar
tensor theories of gravity, foundations of gravity, foundations of quantum
mechanics, elementary particle physics, and cosmology. It seems that Weyl
geometry continues to offer an open research potential for the foundations of
physics even after the turn to the new millennium.Comment: Completely rewritten conference paper 'Beyond Einstein', Mainz Sep
2008. Preprint ELHC (Epistemology of the LHC) 2017-02, 92 pages, 1 figur
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