| 000 | 03231nam a22005175i 4500 | ||
|---|---|---|---|
| 001 | 978-3-540-85146-2 | ||
| 003 | DE-He213 | ||
| 005 | 20140220084520.0 | ||
| 007 | cr nn 008mamaa | ||
| 008 | 100304s2010 gw | s |||| 0|eng d | ||
| 020 |
_a9783540851462 _9978-3-540-85146-2 |
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| 024 | 7 |
_a10.1007/978-3-540-85146-2 _2doi |
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| 050 | 4 | _aQB495-500.269 | |
| 072 | 7 |
_aTTDS _2bicssc |
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| 072 | 7 |
_aSCI005000 _2bisacsh |
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| 082 | 0 | 4 |
_a520 _223 |
| 082 | 0 | 4 |
_a500.5 _223 |
| 100 | 1 |
_aCelletti, Alessandra. _eauthor. |
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| 245 | 1 | 0 |
_aStability and Chaos in Celestial Mechanics _h[electronic resource] / _cby Alessandra Celletti. |
| 264 | 1 |
_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c2010. |
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| 300 | _bonline resource. | ||
| 336 |
_atext _btxt _2rdacontent |
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| 337 |
_acomputer _bc _2rdamedia |
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| 338 |
_aonline resource _bcr _2rdacarrier |
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| 347 |
_atext file _bPDF _2rda |
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| 490 | 1 | _aSpringer Praxis Books | |
| 505 | 0 | _aOrder and chaos -- Numerical dynamical methods -- Kepler’s problem -- The three-body problem and the Lagrangian solutions -- Rotational dynamics -- Perturbation theory -- Invariant tori -- Long-time stability -- Determination of periodic orbits -- Regularization theory. | |
| 520 | _aThis book presents classical celestial mechanics and its interplay with dynamical systems in a way suitable for advance level undergraduate students as well as postgraduate students and researchers. First paradigmatic models are used to introduce the reader to the concepts of order, chaos, invariant curves, cantori. Next the main numerical methods to investigate a dynamical system are presented. Then the author reviews the classical two-body problem and proceeds to explore the three-body model in order to investigate orbital resonances and Lagrange solutions. In rotational dynamics the author details the derivation of the rigid body motion, and continues by discussing related topics, from spin-orbit resonances to dumbbell satellite dynamics. Perturbation theory is then explored in full detail including practical examples of its application to finding periodic orbits, computation of the libration in longitude of the Moon. The main ideas of KAM theory are provided including a presentation of long-term stability and converse KAM results. Celletti then explains the implementation of computer-assisted techniques, which allow the user to obtain rigorous results in good agreement with the astronomical expectations. Finally the study of collisions in the solar system is approached. | ||
| 650 | 0 | _aPhysics. | |
| 650 | 0 | _aMathematical physics. | |
| 650 | 0 | _aMechanics. | |
| 650 | 0 | _aAstrophysics. | |
| 650 | 1 | 4 | _aPhysics. |
| 650 | 2 | 4 | _aExtraterrestrial Physics, Space Sciences. |
| 650 | 2 | 4 | _aAstrophysics and Astroparticles. |
| 650 | 2 | 4 | _aMechanics. |
| 650 | 2 | 4 | _aStatistical Physics, Dynamical Systems and Complexity. |
| 650 | 2 | 4 | _aMathematical Methods in Physics. |
| 710 | 2 | _aSpringerLink (Online service) | |
| 773 | 0 | _tSpringer eBooks | |
| 776 | 0 | 8 |
_iPrinted edition: _z9783540851455 |
| 830 | 0 | _aSpringer Praxis Books | |
| 856 | 4 | 0 | _uhttp://dx.doi.org/10.1007/978-3-540-85146-2 |
| 912 | _aZDB-2-EES | ||
| 999 |
_c111253 _d111253 |
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