000 | 01937nam a22002537a 4500 | ||
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001 | sulb2011132041 | ||
003 | BD-SySUS | ||
005 | 20180711154854.0 | ||
008 | 180711s2012 ii a b 001 0 eng d | ||
020 | _a9780199662869 (pbk.) | ||
040 |
_aUKMGB _beng _cUKMGB _dOCLCO _dBTCTA _dYDXCP _dCDX _dYNK _dMNW _dVMY _dDLC _dBD-SySUS |
||
050 | 0 | 0 | _b.S73 2012 |
082 | 0 | 4 |
_a530.11 _222 _bSTR |
100 | 1 |
_aSteane, Andrew M. _929196 |
|
245 | 1 | 0 |
_aRelativity made relatively easy / _cAndrew M. Steane. |
260 |
_adelhi : _bOxford University Press, _c2012. |
||
300 |
_axv, 419 p. : _bill. ; _c26 cm. |
||
504 | _aIncludes bibliographical references (p. [413]) and index | ||
520 | _aRelativity Made Relatively Easy presents an extensive study of Special Relativity and a gentle (but exact) introduction to General Relativity for undergraduate students of physics. Assuming almost no prior knowledge, it allows the student to handle all the Relativity needed for a university course, with explanations as simple, thorough, and engaging as possible. | ||
520 | _aThe aim is to make manageable what would otherwise be regarded as hard; to make derivations as simple as possible and physical ideas as transparent as possible. Lorentz invariants and four-vectors are introduced early on, but tensor notation is postponed until needed. In addition to the more basic ideas such as Doppler effect and collisions, the text introduces more advanced material such as radiation from accelerating charges, Lagrangian methods, the stress-energy tensor, and introductory General Relativity, including Gaussian curvature, the Schwarzschild solution, gravitational lensing, and black holes. A second volume will extend the treatment of General Relativity somewhat more thoroughly, and also introduce Cosmology, spinors, and some field theory. | ||
650 | 0 |
_aSpecial relativity (Physics) _929197 |
|
650 | 0 |
_aRelativity (Physics) _929198 |
|
942 |
_2ddc _cBK |
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999 |
_c73175 _d73175 |