**Author**: Ian Morison

**Publisher:** John Wiley & Sons

**ISBN:** 1118681525

**Category:** Science

**Page:** 360

**View:** 2925

Introduction to Astronomy & Cosmology is a modernundergraduate textbook, combining both the theory behind astronomywith the very latest developments. Written for science students,this book takes a carefully developed scientific approach to thisdynamic subject. Every major concept is accompanied by a workedexample with end of chapter problems to improve understanding Includes coverage of the very latest developments such asdouble pulsars and the dark galaxy. Beautifully illustrated in full colour throughout Supplementary web site with many additional full colour images,content, and latest developments.

In diesem kompetent geschriebenen Lehrbuch wird, ausgehend von der Beschreibung unserer Milchstraße, die Astronomie der Galaxien und ihrer großräumigen Verteilung eingehend dargestellt und schließlich im kosmologischen Kontext diskutiert. Aufbauend auf eine Einführung in die moderne beobachtende und theoretische Kosmologie wird die Entstehung von Strukturen und astronomischen Objekten im frühen Universum besprochen.

Dank sich stets verbessernder boden- und weltraumgestützter Teleskope stehen der Kosmologie inzwischen Daten zur Verfügung, die Rückschlüsse auf immer frühere Phasen des Universums und Vergleiche mit Modellvorstellungen erlauben. Daher gewinnt die Kosmologie in den Astronomiekursen der Universitäten beständig an Wichtigkeit. Die "Einführung in die Moderne Kosmologie" ist eine anschauliche und leicht verständliche Darstellung moderner kosmologischer Konzepte, die neben zahlreichen Beispielen und Übungsaufgaben auch Hinweise und Endergebnisse enthält, sodass das Erlernte sofort ausprobiert und kontrolliert werden kann. Das Buch ist klar eingeteilt und behandelt in sechs separaten Kapiteln Themen für Fortgeschrittene, darunter relativistische Kosmologie und Neutrino-Kosmologie. Die vorliegende Übersetzung der zweiten Auflage wurde wesentlich ergänzt und erweitert und umfasst neueste Beobachtungsergebnisse sowie zusätzliches Material zur empirischen Kosmologie und Strukturbildung.

This second edition of Introduction to Cosmology is an exciting update of an award-winning textbook. It is aimed primarily at advanced undergraduate students in physics and astronomy, but is also useful as a supplementary text at higher levels. It explains modern cosmological concepts, such as dark energy, in the context of the Big Bang theory. Its clear, lucid writing style, with a wealth of useful everyday analogies, makes it exceptionally engaging. Emphasis is placed on the links between theoretical concepts of cosmology and the observable properties of the universe, building deeper physical insights in the reader. The second edition includes recent observational results, fuller descriptions of special and general relativity, expanded discussions of dark energy, and a new chapter on baryonic matter that makes up stars and galaxies. It is an ideal textbook for the era of precision cosmology in the accelerating universe.

A thorough introduction to modern ideas on cosmology and on the physical basis of the general theory of relativity, An Introduction to the Science of Cosmology explores various theories and ideas in big bang cosmology, providing insight into current problems. Assuming no previous knowledge of astronomy or cosmology, this book takes you beyond introductory texts to the point where you are able to read and appreciate the scientific literature, which is broadly referenced in the book. The authors present the standard big bang theory of the universe and provide an introduction to current inflationary cosmology, emphasizing the underlying physics without excessive technical detail. The book treats cosmological models without reliance on prior knowledge of general relativity, the necessary physics being introduced in the text as required. It also covers recent observational evidence pointing to an accelerating expansion of the universe. The first several chapters provide an introduction to the topics discussed later in the book. The next few chapters introduce relativistic cosmology and the classic observational tests. One chapter gives the main results of the hot big bang theory. Next, the book presents the inflationary model and discusses the problem of the origin of structure and the correspondingly more detailed tests of relativistic models. Finally, the book considers some general issues raised by expansion and isotropy. A reference section completes the work by listing essential formulae, symbols, and physical constants. Beyond the level of many elementary books on cosmology, An Introduction to the Science of Cosmology encompasses numerous recent developments and ideas in the area. It provides more detailed coverage than many other titles available, and the inclusion of problems at the end of each chapter aids in self study and makes the book suitable for taught courses.

This introductory textbook has been designed by a team of experts for elementary university courses in astronomy and astrophysics. It starts with a detailed discussion of the structure and history of our own Galaxy, the Milky Way, and goes on to give a general introduction to normal and active galaxies including models for their formation and evolution. The second part of the book provides an overview of the wide range of cosmological models and discusses the Big Bang and the expansion of the Universe. Written in an accessible style that avoids complex mathematics, and illustrated in colour throughout, this book is suitable for self-study and will appeal to amateur astronomers as well as undergraduate students. It contains numerous helpful learning features such as boxed summaries, student exercises with full solutions, and a glossary of terms. The book is also supported by a website hosting further teaching materials.

This is a truly astonishing book, invaluable for anyone with an interest in astronomy. Physics Bulletin Just the thing for a first year university science course. Nature This is a beautiful book in both concept and execution. Sky & Telescope

This second edition has been updated and substantially expanded. Starting with the description of our home galaxy, the Milky Way, this cogently written textbook introduces the reader to the astronomy of galaxies, their structure, active galactic nuclei, evolution and large scale distribution in the Universe. After an extensive and thorough introduction to modern observational and theoretical cosmology, the focus turns to the formation of structures and astronomical objects in the early Universe. The basics of classical astronomy and stellar astrophysics needed for extragalactic astronomy are provided in the appendix. While this book has grown out of introductory university courses on astronomy and astrophysics and includes a set of problems and solutions, it will not only benefit undergraduate students and lecturers; thanks to the comprehensive coverage of the field, even graduate students and researchers specializing in related fields will appreciate it as a valuable reference work.

This introductory textbook for undergraduate courses in galactic astrophysics and cosmology was developed as a more compact and focused alternative to its parent volume, An Introduction to Modern Astrophysics. Aimed at astronomy and physics majors, it offers thorough coverage of galactic structure and evolution, active galaxies, cosmology, and the

Fully updated edition of the successful introductory graduate textbook on modern cosmology.

Designed for students who have a basic understanding of physics and mathematics, this text provides a fundamental, three-in-one introduction to astronomy, astrophysics, and cosmology. The astronomy section explores fundamental topics such as the celestial coordinate system, stellar classification schemes, H-R diagrams, and the masses and radii of stars. The astrophysics section addresses stellar structure, stellar atmospheres, energy generation in stars, and nucleosynthesis. Also covering galactic structure and rotation, the cosmology section introduces the Robertson-Walker metric and Friedman models of the universe and discusses the present status of the Hubble constant along with problems associated with the age of the universe. Numerous problems, diagrams, and up-to-date references make this an ideal introductory text for graduate courses in physics, mathematics, space physics, or any program for which astronomy is an option.

An Introduction to Modern Cosmology Third Edition is anaccessible account of modern cosmological ideas. The Big BangCosmology is explored, looking at its observational successes inexplaining the expansion of the Universe, the existence andproperties of the cosmic microwave background, and the origin oflight elements in the universe. Properties of the very earlyUniverse are also covered, including the motivation for a rapidperiod of expansion known as cosmological inflation. The thirdedition brings this established undergraduate textbook up-to-datewith the rapidly evolving observational situation. This fully revised edition of a bestseller takes an approachwhich is grounded in physics with a logical flow of chaptersleading the reader from basic ideas of the expansion described bythe Friedman equations to some of the more advanced ideas about theearly universe. It also incorporates up-to-date results from thePlanck mission, which imaged the anisotropies of the CosmicMicrowave Background radiation over the whole sky. The AdvancedTopic sections present subjects with more detailed mathematicalapproaches to give greater depth to discussions. Student problemswith hints for solving them and numerical answers are embedded inthe chapters to facilitate the reader’s understanding andlearning. Cosmology is now part of the core in many degree programs. Thiscurrent, clear and concise introductory text is relevant to a widerange of astronomy programs worldwide and is essential reading forundergraduates and Masters students, as well as anyone startingresearch in cosmology. Supplementary material, includingfull-colour images, updates and links for students and instructors,is available on the author’s website: ahref="http://www.roe.ac.uk/~arl/"http://www.roe.ac.uk/~arl//a.

The Fourth Edition of Introduction to Cosmology provides a concise, authoritative study of cosmology at an introductory level. Starting from elementary principles and the early history of cosmology, the text carefully guides the student on to curved spacetimes, special and general relativity, gravitational lensing, the thermal history of the Universe, and cosmological models, including extended gravity models, black holes and Hawking's recent conjectures on the not-so-black holes. Introduction to Cosmology, Fourth Edition includes: New theoretical approaches and in-depth material on observational astrophysics and expanded sections on astrophysical phenomena Illustrations throughout and comprehensive references with problems at the end of each chapter and a rich index at the end of the book Latest observational results from WMAP9, ACT, and Planck, and all cosmological parameters have been brought up to date. This text is invaluable for undergraduate students in physics and astrophysics taking a first course in cosmology. Extensively revised, this latest edition extends the chapter on cosmic inflation to the recent schism on eternal inflation and multiverses. Dark matter is discussed on galaxy and cluster scales, and dark matter candidates are presented, some requiring a five-dimensional universe and several representing various types of exotica. In the context of cosmic structures the cold dark matter paradigm is described. Dark energy models include the cosmological constant, quintessence and other single field models, f(R) models and models requiring extra dimensions.

An introductory textbook on mathematical cosmology for beginning graduate students.

Finden auch Sie die Weiten des Kosmos faszinierend und fragen sich, wie Wissenschaftler so viel über Objekte in unerreichbarer Ferne wissen können? "Astronomie für Dummies" bringt Ihnen die Weiten des Universums näher: Erkunden Sie unser Sonnensystem, ferne Galaxien und die Milchstraße. Lesen Sie wie in einem Krimi von schwarzen Löchern, dem Asteroidengürtel und der Entstehung des Universums. Außerdem gibt Stephen Maran viele Tipps zur richtigen Ausrüstung eines Astronomen. So können Sie schon bald selbst nach den Sternen greifen.

General relativity is a cornerstone of modern physics, and is of major importance in its applications to cosmology. Plebanski and Krasinski are experts in the field and in this book they provide a thorough introduction to general relativity, guiding the reader through complete derivations of the most important results. Providing coverage from a unique viewpoint, geometrical, physical and astrophysical properties of inhomogeneous cosmological models are all systematically and clearly presented, allowing the reader to follow and verify all derivations. For advanced undergraduates and graduates in physics and astronomy, this textbook will enable students to develop expertise in the mathematical techniques necessary to study general relativity.

The book discusses, based on a series of lectures given by the authors at the Universidad Autonoma of Madrid discusses the relation between cosmology and particle physics at a pedagogical level. The topics covered contain much valuable introductory materials. Very useful as a text for graduate students in this field.

This well-established, graduate-level textbook is a thorough introduction to radio telescopes and techniques for students and researchers new to the subject.

Distance determination is an essential technique in astronomy, and is briefly covered in most textbooks on astrophysics and cosmology. It is rarely covered as a coherent topic in its own right. When it is discussed the approach is frequently very dry, splitting the teaching into, for example, stars, galaxies and cosmologies, and as a consequence, books lack depth and are rarely comprehensive. Adopting a unique and engaging approach to the subject An Introduction to distance Measurement in Astronomy will take the reader on a journey from the solar neighbourhood to the edge of the Universe, discussing the range of distance measurements methods on the way. The book will focus on the physical processes discussing properties that underlie each method, rather than just presenting a collection of techniques. As well as providing the most compressive account of distance measurements to date, the book will use the common theme of distance measurement to impart basic concepts relevant to a wide variety of areas in astronomy/astrophysics. The book will provide an updated account of the progress made in a large number of subfields in astrophysics, leading to improved distance estimates particularly focusing on the underlying physics. Additionally it will illustrate the pitfalls in these areas and discuss the impact of the remaining uncertainties in the complete understanding of the Universes at large. As a result the book will not only provide a comprehensive study of distance measurement, but also include many recent advances in astrophysics.

"Neutrinos in Particle Physics, Astronomy and Cosmology" provides a comprehensive and up-to-date introduction to neutrino physics, neutrino astronomy and neutrino cosmology. The intrinsic properties and fundamental interactions of neutrinos are described, as is the phenomenology of lepton flavor mixing, seesaw mechanisms and neutrino oscillations. The cosmic neutrino background, stellar neutrinos, supernova neutrinos and ultrahigh-energy cosmic neutrinos, together with the cosmological matter-antimatter asymmetry and other roles of massive neutrinos in cosmology, are discussed in detail. This book is intended for researchers and graduate students in the fields of particle physics, particle astrophysics and cosmology. Dr. Zhizhong Xing is a professor at the Institute of High Energy Physics, Chinese Academy of Sciences, China; Dr. Shun Zhou is currently a postdoctoral fellow at the Max Planck Institute for Physics, Germany.