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Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics
Es darf als gesichert gelten, dass Einstein bereits 1895-1896,
wAhrend er sich an der Aargauischen Kantonsschule auf die
MaturitAtsprA1/4fung vorbereitete, erste Ideen zur
RelativitAtstheorie entwickelte. Die Publikation befasst sich
eingehend mit der Aarauer Zeit des spAter zu Weltruhm gelangten
Physikers und bespricht die grundlegenden Ideen seiner Arbeiten von
1905, die diesen Weltruhm begrA1/4ndeten.
Professor Stephen Hawking is generally considered to have been one of the world's greatest thinkers. Here, his phenomenal bestseller A Brief History of Time is illustrated to bring his theories to life in a clear, captivating and visually engaging way. 'This book marries a child's wonder to a genius's intellect. We journey into Hawking's universe, while marvelling at his mind' - The Sunday Times 'Stephen Hawking can explain the complexities of cosmological physics with an engaging combination of clarity and wit...' - Observer 'Exceptional writing explaining the mysteries and beauty of our universe. The book is very fascinating and highly enjoyable. Highly recommended' - ***** Reader review 'This book is mind blowing' - ***** Reader review 'A masterpiece' - ***** Reader review ******************************************************************************************** Was there a beginning of time? Could time run backwards? Is the universe infinite or does it have boundaries? These are just some of the questions considered in the internationally acclaimed masterpiece by the world-renowned physicist Professor Stephen Hawking. It begins by reviewing the great theories of the cosmos from Newton to Einstein, before delving into the secrets which still lie at the heart of space and time, from the Big Bang to black holes, via spiral galaxies and strong theory. To this day A Brief History of Time remains a staple of the scientific canon, and its succinct and clear language continues to introduce millions to the universe and its wonders. In this edition, Professor Hawking explains his complex theories through a fresh visual dimension. Over 150 stunning colour illustrations have been specially commissioned for this purpose to help the reader understand what have become popular mythic images of our century, but which nonetheless remain difficult, abstract ideas to grasp. This stunning gift edition also includes a new appendix with updates to the text and tributes to Stephen Hawking.
Nuclear astrophysics is, in essence, a science that attempts to
understand and explain the physical universe beyond the Earth by
studying its smallest particles. "Cauldrons in the Cosmos," by
Claus E. Rolfs and William S. Rodney, serves as a basic
introduction to these endeavors. From the major discoveries in the
field to a discussion of the makeup of stars to an explanation of
standard lab techniques, this text provides students and scientists
alike a thorough and fascinating survey of the accomplishments,
goals, and methods of nuclear astrophysics. A classic in its field,
"Cauldrons in the Cosmos" will surely remain an important reference
in nuclear astrophysics for years to come.
Recent discoveries in astronomy and relativistic astrophysics as well as experiments on particle and nuclear physics have blurred the traditional boundaries of physics. It is believed that at the birth of the Universe, a whirlwind of matter and antimatter, of quarks and exotic leptons, briefly appeared and merged into a sea of energy. The new phenomena and new states of matter in the Universe revealed the deep connection between quarks and the Cosmos. Motivated by these themes, this book discusses different topics: gravitational waves, dark matter, dark energy, exotic contents of compact stars, high-energy and gamma-ray astrophysics, heavy ion collisions and the formation of the quark-gluon plasma in the early Universe. The book presents some of the latest researches on these fascinating themes and is useful for experts and students in the field.
The existence of neutron stars was not only a brilliant theoretical prediction, but also one of the most unexpected and astonishing discoveries of all heavenly bodies. Twenty-five years after the remarkable event of their discovery, neutron stars, which are the densest, the most strongly magnetized, and the most rapid ly rotating bodies in the Galaxy, remain objects of intense interest. This book is a revised and enlarged version of the original Russian edition. The last five years were marked by the discovery of a supernova in the closest galaxy and dozens of X-ray sources and millisecond pulsars, which apparently confirm the validity of the basic ideas underlying these discoveries. The author has concentrated on the astrophysical manifestations of neutron stars, which are believed mainly to be associated with the nature of their interaction with their surroundings. Naturally, this approach does not leave much room for a detailed description of the internal structure of these stars. Fortunately, there exists an excellent monograph by S. L. Shapiro and S. A. Teukolsky (Black Holes, White Dwarfs, and Neutron Stars, Wiley, New York 1985) which deals mainly with the purely physical problems. Moreover, the publication of such a book in the West partly makes amends for the lack of information about the work being done by Soviet scientists in this field."
Our Universe is amazing. This is its story, told in simple language. The story tells how the Universe came to be what it is today. It starts with the Big Bang and describes how stars, black holes, and our solar system developed. It explores the evolution of life on Earth and investigates the possibility of extra-terrestrial life. It peers into the future and wonders about the Universe's likely old age and death, or whatever else may be its end. The challenge the book takes up is to explain all of this, including some of the astonishing concepts we have in science, such as Einstein's theories of Relativity and Quantum Mechanics, using virtually no mathematics and without dumbing-down. All are described narratively and explained using examples and anecdotes. The book is written for young people with a thirst for learning about the science of space, as well as for 'grown-ups' who want a better understanding of this fascinating subject.
Combining the latest scientific advances with storytelling skills unmatched in the cosmos, an award-winning astrophysicist and popular writer leads us on a tour of some of the greatest mysteries of our universe. In the constellation of Eridanus, there lurks a cosmic mystery: It's as if something has taken a huge bite out of the universe. But what is the culprit? The hole in the universe is just one of many puzzles keeping cosmologists busy. Supermassive black holes, bubbles of nothingness gobbling up space, monster universes swallowing others-these and many other bizarre ideas are being pursued by scientists. Due to breathtaking progress in astronomy, the history of our universe is now better understood than the history of our own planet. But these advances have uncovered some startling riddles. In this electrifying new book, renowned cosmologist and author Paul Davies lucidly explains what we know about the cosmos and its enigmas, exploring the tantalizing-and sometimes terrifying-possibilities that lie before us. As Davies guides us through the audacious research offering mind-bending solutions to these and other mysteries, he leads us up to the greatest outstanding conundrum of all: Why does the universe even exist in the first place? And how did a system of mindless, purposeless particles manage to bring forth conscious, thinking beings? Filled with wit and wonder, What's Eating the Universe? is a dazzling tour of cosmic questions, sure to entertain, enchant, and inspire us all.
The eleventh COSPAR colloquium The Outer Heliosphere: The Next
Frontiers was held in Potsdam, Germany, from 24-28 July, 2000, and
is the second dedicated to this subject after the first one held in
Warsaw, Poland in 1989.
Numerous times throughout Earth's history there have been major cataclysmic events. These events have resulted in large-scale climactic changes, mythological stories of floods and visitations from the skies, and sometimes the complete extinction of life. The major planetary body that has caused much of this carnage has been referred to by many names. Jason Breshears has termed it Phoenix, based on his research into the distant past and what it was usually called by witnesses. By piecing together ancient documents from the most reputable sources available, we have, in this book, the most extensive and accurate rendering of the cycle of the Phoenix, including when it will come again. Some of us, according to the author, will live to see its return. Beyond the foundational scientific evidence, the author ties in various Bible prophecies that relate directly to it. Many books exist on this subject, but few have broken new ground like this one, due to the extensive research involved.
Paperback. This publication contains 36 papers presented at four symposia during the Thirty-first COSPAR Scientific Assembly held in Birmingham, UK during 1996. Papers reflect the following symposia themes: life science support system studies; production, processing and waste recycling in a CELSS (Controlled Ecological Life Support System); biological effects of closure and recycling in a CELSS; nutrition and productivity for bioregenerative life support; integration of bioregenerative and physical/chemical processes for space life support systems. Findings presented in this volume will be a valuable resource for CELSS researchers for many years to come.
This book introduces quantum field theory, together with its most important applications to cosmology and astroparticle physics, in a coherent framework. The path integral approach is employed right from the start, and the use of Green functions and generating functionals is illustrated first in quantum mechanics and then in scalar field theory. Massless spin one and two fields are discussed on an equal footing, and gravity is presented as a gauge theory in close analogy with the Yang-Mills case. Concepts relevant to modern research such as helicity methods, effective theories, decoupling, or the stability of the electroweak vacuum are introduced. Various applications such as topological defects, dark matter, baryogenesis, processes in external gravitational fields, inflation and black holes help students to bridge the gap between undergraduate courses and the research literature.
Compact objects are an important class of astronomical objects in current research. Supermassive black holes play an important role in the understanding of the formation of galaxies in the early Universe. Old white dwarfs are nowadays used to calibrate the age of the Universe. Mergers of neutron stars and black holes are the sources of intense gravitational waves which will be measured in the next ten years by gravitational wave detectors. Camenzind's Compact Objects in Astrophysics gives a comprehensive introduction and up-to-date overview about the physical processes behind these objects, covering the field from the beginning to most recent results, including all relevant observations. After a presentation of the taxonomy of compact objects, the
basic principles of general relativity are given. The author then
discusses in detail the physics and observations of white dwarfs
and neutron stars (including the most recent equations of state for
neutron star matter), the gravitational field of rapidly rotating
compact objects, rotating black holes (including ray tracing and
black hole magnetospheres), gravitational waves, and the new
understanding of accretion processes by means of the
magnetorotational instability of accretion disks.
This book is based on the lectures given at the "Euroschool on Exotic Beams" and collects contributions which address topics from the traditional core of the field of exotic nuclei like nuclear structure far from stability, discussing recent theoretical developments and state-of-the-art experimental methods. It provides also new perspectives in nuclear astrophysics and in applied areas such as gamma-ray emission imaging. The contributions are written with a pedagogical approach and carefully edited in order to provide the readership with a clear and fluent reading. The book is intended for PhD students and young researchers who are approaching the new research lines in nuclear physics with exotic nuclei. Only basics concepts on quantum mechanics and nuclear physics are requested to follow and master the covered arguments.
There are reasons to believe the 21st century will be the best ever for astrophysics: the James Webb Space Telescope will extend nearly twenty times the present observational limit of visible light; neutrino massiveness opens a new window for exploration on dark energy and dark matter physics and is expected to provide insights into the fate of the Universe; the Higgs boson may allow for an understanding of the weakness of gravity; gravitational waves produced at the birth of the Universe and by compact stellar objects (supermassive black holes, black hole/neutron star mergers, gamma-ray bursts, white dwarf inspirals) have unveiled a new area of astronomy. Against this background, compact stars, the theme of this volume, present unique astrophysical laboratories for probing the fabric of space-time and the building blocks of matter and their interactions at physical regimes not attainable in terrestrial laboratories.
This thesis by Cole Johnston brings novel insights into the inner workings of young massive stars. By bridging the observational fields of binary stars and asteroseismology this thesis uses state of the art statistical techniques to scrutinise theories of modern stellar astrophysics. Developing upon the commonly used isochrone fitting methodology, the author introduces the idea of isochrone cloud fitting in order to account for the full breadth of physics observed in stars. The author combines this methodology with gravity mode asteroseismic analysis to asses the level of chemical mixing deep within the stellar core in order to determine the star's age and core mass. Wrapped into a robust statistical framework to account for correlations, this methodology is employed to analyse individual stars, multiple systems, and clusters alike to demonstrate that chemical mixing has dramatic impact on stellar structure and evolution.
This book focuses on the non-traditional branches of physics and mechanics of shock waves that have arisen recently in connection with the intensive study of these waves in a wide variety of phenomena - from nuclear matter to clusters of galaxies. The book is devoted to the various physical phenomena and properties of intense shock waves. The author addresses methods of generation, diagnostics, as well as theoretical methods for describing shock waves at extremely high pressures and temperatures in laboratory and quasi-laboratory conditions. The state of materials with high energy density generated by shock wave compression is discussed. In addition, the book aims to systematize, generalize, and describe from a universal viewpoint the extensive theoretical and experimental material on the physics of high energy densities - the physics and mechanics of intense shock waves. The book is based on lectures delivered by the author at the Moscow Institute of Physics and Technology, the Higher School of Physics of Rosatom State Nuclear Energy Corporation, as well as overviews presented at many scientific conferences and symposia. It is useful to a wide range of researchers in natural sciences, giving them access to original works and allowing them to navigate the fascinating problems of the modern science of intense shock waves. |
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