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Books > Science & Mathematics > Physics > Relativity physics > General
Classical electromagnetism - one of the fundamental pillars of
physics - is an important topic for all types of physicists from
the theoretical to the applied. The subject is widely recognized to
be one of the most challenging areas of the physics curriculum,
both for students to learn and for lecturers to teach. Although
textbooks on electromagnetism are plentiful, hardly any are written
in the question-and-answer style format adopted in this book. It
contains nearly 300 worked questions and solutions in classical
electromagnetism, and is based on material usually encountered
during the course of a standard university physics degree. Topics
covered include some of the background mathematical techniques,
electrostatics, magnetostatics, elementary circuit theory,
electrodynamics, electromagnetic waves and electromagnetic
radiation. For the most part the book deals with the microscopic
theory, although we also introduce the important subject of
macroscopic electromagnetism as well. Nearly all questions end with
a series of comments whose purpose is to stimulate inductive
reasoning and reach various important conclusions arising from the
problem. Occasionally, points of historical interest are also
mentioned. Both analytical and numerical techniques are used in
obtaining and analyzing solutions. All computer calculations are
performed with MathematicaCO (R) and the relevant code is provided
in a notebook; either in the solution or the comments.
Recent cosmological observations have posed a challenge for
traditional theories of gravity: what is the force driving the
accelerated expansion of the universe? What if dark energy or dark
matter do not exist and what we observe is a modification of the
gravitational interaction that dominates the universe at large
scales? Various extensions to Einstein's General Theory of
Relativity have been proposed, and this book presents a detailed
theoretical and phenomenological analysis of several leading,
modified theories of gravity. Theories with generalised
curvature-matter couplings are first explored, followed by hybrid
metric-Palatini gravity. This timely book first discusses key
motivations behind the development of these modified gravitational
theories, before presenting a detailed overview of their subsequent
development, mathematical structure, and cosmological and
astrophysical implications. Covering recent developments and with
an emphasis on astrophysical and cosmological applications, this is
the perfect text for graduate students and researchers.
Galileo Unbound traces the journey that brought us from Galileo's
law of free fall to today's geneticists measuring evolutionary
drift, entangled quantum particles moving among many worlds, and
our lives as trajectories traversing a health space with thousands
of dimensions. Remarkably, common themes persist that predict the
evolution of species as readily as the orbits of planets or the
collapse of stars into black holes. This book tells the history of
spaces of expanding dimension and increasing abstraction and how
they continue today to give new insight into the physics of complex
systems. Galileo published the first modern law of motion, the Law
of Fall, that was ideal and simple, laying the foundation upon
which Newton built the first theory of dynamics. Early in the
twentieth century, geometry became the cause of motion rather than
the result when Einstein envisioned the fabric of space-time warped
by mass and energy, forcing light rays to bend past the Sun.
Possibly more radical was Feynman's dilemma of quantum particles
taking all paths at once - setting the stage for the modern fields
of quantum field theory and quantum computing. Yet as concepts of
motion have evolved, one thing has remained constant, the need to
track ever more complex changes and to capture their essence, to
find patterns in the chaos as we try to predict and control our
world.
Tobias Schuttler stellt in diesem essential beide im Detail sehr
anspruchsvollen Gebiete - Einsteins beruhmte Relativitatstheorie
und die Satellitenortung mit GPS und Galileo - in allgemein
verstandlicher Weise dar und erklart die Einflusse der
Relativitatstheorie bei der Satellitennavigation ohne hoehere
Mathematik. Es werden auch die zu dieser Betrachtung wichtigen
Formeln genannt und motiviert. Um die Einflusse der
Relativitatstheorie auf ein Satellitennavigationssystem wie das
europaische Galileo zu verstehen, muss man sich mit dem konkreten
Messvorgang bei der Ortung auseinandersetzen. Die Grundidee des
Verfahrens ist einfach - die technische Umsetzung indes hoechst
komplex.
The two-volume book Gravitational Waves provides a comprehensive
and detailed account of the physics of gravitational waves. While
Volume 1 is devoted to the theory and experiments, Volume 2
discusses what can be learned from gravitational waves in
astrophysics and in cosmology, by systematizing a large body of
theoretical developments that have taken place over the last
decades. The second volume also includes a detailed discussion of
the first direct detections of gravitational waves. In the author's
typical style, the theoretical results are generally derived
afresh, clarifying or streamlining the existing derivations
whenever possible, and providing a coherent and consistent picture
of the field. The first volume of Gravitational Waves, which
appeared in 2007, has established itself as the standard reference
in the field. The scientific community has eagerly awaited this
second volume. The recent direct detection of gravitational waves
makes the topics in this book particularly timely.
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