By Robert Resnick
This e-book provides an outstanding advent to the idea of specific relativity. Professor Resnick provides a basic and unified improvement of the topic with surprisingly transparent discussions of the facets that sometimes hassle newbies. He comprises, for instance, a piece at the logic of relativity. His presentation is energetic and interspersed with historic, philosophical and specified subject matters (such because the dual paradox) that would arouse and carry the reader's curiosity. you can find many distinct positive factors that assist you clutch the fabric, equivalent to worked-out examples,summary tables,thought questions and a wealth of fine difficulties. The emphasis through the ebook is actual. The experimental heritage, experimental affirmation of predictions, and the actual interpretation of rules are under pressure. The publication treats relativistic kinematics, relativistic dynamics, and relativity and electromagnetism and includes detailed appendices at the geometric illustration of space-time and on basic relativity. Its association allows an teacher to alter the size and intensity of his remedy and to take advantage of the publication both with or following classical physics. those positive factors make it a great significant other for introductory classes.
Read Online or Download An introduction to the special theory of relativity PDF
Best relativity books
In those inspiring lectures David Bohm explores Albert Einstein’s celebrated thought of Relativity that remodeled eternally the best way we expect approximately time and area. but for Bohm the results of the speculation have been way more innovative either in scope and influence even than this. Stepping again from dense theoretical and medical element during this eye-opening paintings, Bohm describes how the thought of relativity moves on the center of our very notion of the universe, whether we're physicists or philosophers.
"A vintage of physics . .. the 1st systematic presentation of Einstein's concept of relativity. " — British magazine for Philosophy and technology. lengthy one of many commonplace texts within the box, this wonderful advent probes deeply into Euclidean house, Riemann's house, Einstein's basic relativity, gravitational waves and effort, and legislation of conservation.
The up to date and multiplied 10th anniversary version
Pedagogical creation to numerical relativity for college kids and researchers getting into the sector, and scientists.
- Theories of Explanation
- Relativistic Density Functional For Nuclear Structure
- From Special Relativity to Feynman Diagrams: A Course of Theoretical Particle Physics for Beginners
- An Introduction to Relativistic Quantum Field Theory
- The Cauchy Problem in General Relativity (ESI Lectures in Mathematics and Physics)
- Relativity on curved manifolds
Extra resources for An introduction to the special theory of relativity
X p ) = 0 if one of X 1 , . . , X p is either L or L. Thus a general type T p S q tensorfield may be thought of as the specification of a type T p tensorfield intrinsic to Su,u for each (u, u). Let then ξ be an S 1-form. We define L / L ξ to be, for each (u, u) ∈ D, u > u, the restriction to T Su,u of L L ξ , the Lie derivative of ξ with respect to L, a notion intrinsic to / L ξ is an S 1-form as well. Note that in any case we have (L L ξ )(L) = 0. each Cu . Then L We define L / L ξ to be, for each (u, u) ∈ D, u > u, the restriction to T Su,u of L L ξ , the Lie derivative of ξ with respect to L, a notion intrinsic to each C u .
Q q Finally, a type T p S tensorfield θ is a type T p tensorfield defined on M \ 0 such that at each x ∈ M \ 0 and each X 1 , . . , X p ∈ Tx M we have θ (X 1 , . . , X p ) ∈ ⊗q Tx Su,u q and θ (X 1 , . . , X p ) = 0 if one of X 1 , . . , X p is either L or L. Thus a general type T p S q tensorfield may be thought of as the specification of a type T p tensorfield intrinsic to Su,u for each (u, u). Let then ξ be an S 1-form. We define L / L ξ to be, for each (u, u) ∈ D, u > u, the restriction to T Su,u of L L ξ , the Lie derivative of ξ with respect to L, a notion intrinsic to / L ξ is an S 1-form as well.
That is, for each point p ∈ M, each past-directed causal curve issuing from p is to terminate in the past at a point on Co . The generators of Co are the future-directed null geodesics issuing from o. These are affinely parametrized as follows. There is a future-directed unit timelike vector T at o such that the tangent vector at o to each generator has projection T along T . We denote by L the null geodesic vectorfield along Co , which is the tangent field to each generator. The parameter of this vectorfield, measured from o, is the affine parameter s.