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| Author | : Andrew R. Liddle |
| Publisher | : Cambridge University Press |
| Total Pages | : 420 |
| Release | : 2000-04-13 |
| Genre | : Science |
| ISBN | : 9780521575980 |
A thorough and up-to-date graduate textbook on the most promising theory of the universe - inflationary cosmology.
| Author | : David H. Lyth |
| Publisher | : Cambridge University Press |
| Total Pages | : 516 |
| Release | : 2009-06-11 |
| Genre | : Science |
| ISBN | : 1139643746 |
The origin and evolution of the primordial perturbation is the key to understanding structure formation in the earliest stages of the Universe. It carries clues to the types of physical phenomena active in that extreme high-density environment. Through its evolution, generating first the observed cosmic microwave background anisotropies and later the distribution of galaxies and dark matter in the Universe, it probes the properties and dynamics of the present Universe. This graduate-level textbook gives a thorough account of theoretical cosmology and perturbations in the early Universe, describing their observational consequences and showing how to relate such observations to primordial physical processes, particularly cosmological inflation. With ambitious observational programmes complementing ever-increasing sophistication in theoretical modelling, cosmological studies will remain at the cutting edge of astrophysical studies for the foreseeable future.
| Author | : P. J. E. Peebles |
| Publisher | : Princeton University Press |
| Total Pages | : 439 |
| Release | : 2020-09-15 |
| Genre | : Science |
| ISBN | : 0691209839 |
The classic account of the structure and evolution of the early universe from Nobel Prize–winning physicist P. J. E. Peebles An instant landmark on its publication, The Large-Scale Structure of the Universe remains the essential introduction to this vital area of research. Written by one of the world's most esteemed theoretical cosmologists, it provides an invaluable historical introduction to the subject, and an enduring overview of key methods, statistical measures, and techniques for dealing with cosmic evolution. With characteristic clarity and insight, P. J. E. Peebles focuses on the largest known structures—galaxy clusters—weighing the empirical evidence of the nature of clustering and the theories of how it evolves in an expanding universe. A must-have reference for students and researchers alike, this edition of The Large-Scale Structure of the Universe introduces a new generation of readers to a classic text in modern cosmology.
| Author | : Steff Jaywan |
| Publisher | : Dedona Publishing |
| Total Pages | : 74 |
| Release | : |
| Genre | : Science |
| ISBN | : |
The concept of cosmic inflation stands as one of the most revolutionary and compelling ideas in modern astrophysics. First proposed in the early 1980s, inflation theory has transformed our understanding of the universe's earliest moments, providing profound insights into its large-scale structure and the intricate patterns of galaxies we observe today. This book goes on a journey to unravel the complexities of this remarkable theory, exploring its origins, implications, and the compelling evidence that supports it. Cosmic inflation posits that the universe underwent an exponential expansion within a fraction of a second after the Big Bang. This rapid inflation smoothed out any initial irregularities, setting the stage for the universe's current uniformity and flatness. It also stretched quantum fluctuations to astronomical scales, seeding the formation of galaxies and cosmic structures. Through this lens, we gain a clearer picture of how the universe evolved from a hot, dense state to the vast, structured cosmos we inhabit. This book is designed to cater to both curious laypersons and dedicated students of cosmology. We will delve into the fundamental principles of inflation theory, explore its mathematical underpinnings, and examine the observational evidence that lends it credence. From the cosmic microwave background radiation to the distribution of galaxies, we will see how inflation theory elegantly explains many of the universe's most perplexing features. This book is designed to cater to both curious laypersons and dedicated students of cosmology. We will delve into the fundamental principles of inflation theory, explore its mathematical underpinnings, and examine the observational evidence that lends it credence. From the cosmic microwave background radiation to the distribution of galaxies, we will see how inflation theory elegantly explains many of the universe's most perplexing features.
| Author | : T. Shanks |
| Publisher | : Springer Science & Business Media |
| Total Pages | : 472 |
| Release | : 2012-12-06 |
| Genre | : Science |
| ISBN | : 940113510X |
This book represents the proceedings from the NATO sponsored Advanced Research Workshop entitled "Observational Tests of Inflation" held at the University of Durham, England on the 10th-14th December, 1990. In recent years, the cosmological inflation model has drawn together the worlds of particle physics, theoretical cosmology and observational astronomy. The aim of the workshop was to bring together experts in all of these fields to discuss the current status of the inflation theory and its observational predictions. The simplest inflation model makes clear predictions which are testable by astronomical observation. Foremost is the prediction that the cosmological density parameter, no, should have a value negligibly different from the critical, Einstein-de Sitter value of 00=1. The other main prediction is that the spectrum of primordial density fluctuations should be Gaussian and take the Harrison-Zeldovich form. The prediction that n =l, in patticular, leads to several important consequences o for cosmology. Firstly, there is the apparent contradiction with the limits on baryon density from Big Bang nucleosynthesis which has led to the common conjecture that weakly interacting particles rather than baryons may form the dominant mass constituent of the Universe. Secondly, with n =l, the age of the Universe is uncomfortably short if o the Hubble constant and the ages of the oldest star clusters lie within their currently believed limits.
| Author | : Andrei Linde |
| Publisher | : CRC Press |
| Total Pages | : 384 |
| Release | : 1990-05-17 |
| Genre | : Science |
| ISBN | : 9783718604906 |
A monograph on inflationary cosmology and cosmological phase transitions, investigating modern cosmology's relationship to elementary particle physics. This work also includes a non-technical discussion of inflationary cosmology for those unfamiliar with the theory.
| Author | : J. A. Peacock |
| Publisher | : Cambridge University Press |
| Total Pages | : 700 |
| Release | : 1999 |
| Genre | : Science |
| ISBN | : 9780521422703 |
A comprehensive and authoritative introduction to contemporary cosmology for advanced undergraduate and graduate students.
| Author | : T. Padmanabhan |
| Publisher | : Cambridge University Press |
| Total Pages | : 504 |
| Release | : 1993 |
| Genre | : Science |
| ISBN | : 9780521424868 |
This text provides an up-to-date and pedagogical introduction to this exciting area of research.
| Author | : Reza Mansouri |
| Publisher | : Springer Science & Business Media |
| Total Pages | : 385 |
| Release | : 2012-12-06 |
| Genre | : Science |
| ISBN | : 9401141754 |
The modern Persian word for cosmology is "Keyhan-shenakht", which is also the title of a Persian book written more than 800 years ago. The same term can also be found in Old Persian. In spite of this old tradition, modern cosmology is a new~omer within the scientific disciplines in Iran. The cosmology community' is small and not yet well established. Given the spectacular recent advances in observational and theoretical cosmology, the large amount of new observational data which will become available in the near future, and the rapid expansion of the international cosmology community, it was realized that Iran should play a more active role in the exciting human endeavour which cosmology constitutes. This was the main motivation to establish a School on Cosmology in Iran. The plan is to hold a cosmology school every three years somewhere in Iran. The focus of this First School on Cosmology was chosen to be structure formation, a rapidly evolving cornerstone of modern cosmology. The topics of the school were selected in order to give both a broad overview of the current status of cosmological structure formation, and an in-depth dis cussion of the key issues theory of cosmological perturbations and analysis of cosmic microwave anisotropies. The lectures by Blanchard and Sarkar give an overview of homogeneous cosmological models and standard big bang cosmology. In his contribution, Padmanabhan presents a comprehen sive discussion of the growth of cosmological perturbations.
| Author | : Georg Wolschin |
| Publisher | : Springer |
| Total Pages | : 188 |
| Release | : 2010-03-10 |
| Genre | : Science |
| ISBN | : 364210598X |
The lectures that four authors present in this volume investigate core topics related to the accelerated expansion of the Universe. Accelerated expansion occured in the ?36 very early Universe – an exponential expansion in the in ationary period 10 s after the Big Bang. This well-established theoretical concept had rst been p- posed in 1980 by Alan Guth to account for the homogeneity and isotropy of the observable universe, and simultaneously by Alexei Starobinski, and has since then been developed by many authors in great theoretical detail. An accelerated expansion of the late Universe at redshifts z
