Robert M. Wald – författare
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6 produkter
Space, Time, and Gravity
The Theory of the Big Bang and Black Holes
Häftad, 1992
230 kr
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Writing for the general reader or student, Wald has completely revised and updated this highly regarded work to include recent developments in black hole physics and cosmology. Nature called the first edition "a very readable and accurate account of modern relativity physics for the layman within …
Quantum Field Theory in Curved Spacetime and Black Hole Thermodynamics
Häftad, 1994
325 kr
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In this book, Robert Wald provides a pedagogical introduction to the formulation of quantum field theory in curved spacetime. He begins with a treatment of the ordinary one-dimensional quantum harmonic oscillator, progresses through the construction of quantum field theory in flat spacetime to …
General Relativity
Häftad, 1984
557 kr
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"Wald's book is clearly the first textbook on general relativity with a totally modern point of view; and it succeeds very well where others are only partially successful. The book includes full discussions of many problems of current interest which are not treated in any extant book, and all these …
Black Holes and Relativistic Stars
Inbunden, 1998
858 kr
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The inevitability of gravitational collapse for stellar bodies of sufficient mass was convincingly demonstarted by S. Chandrasekhar in the 1930s, black holes and neutron stars played a minor role in serious analyses of physical or astrophysical phenomena until the discovery of quasars and pulsars …
Space, Time, and Gravity
The Theory of the Big Bang and Black Holes
Inbunden, 1992
437 kr
Tillfälligt slut
Writing for the general reader or student, Wald has completely revised and updated this highly regarded work to include recent developments in black hole physics and cosmology. Nature called the first edition "a very readable and accurate account of modern relativity physics for the layman within …
Black Holes and Relativistic Stars
Häftad, 1999
428 kr
Tillfälligt slut
The inevitability of gravitational collapse for stellar bodies of sufficient mass was convincingly demonstrated by S. Chandrasekhar in the 1930s, black holes and neutron stars played a minor role in serious analyses of physical or astrophysical phenomena until the discovery of quasars and pulsars …
