000			02055 a2200313 4500
003			CL-VaUPLA
005			20251209145818.0
007			ta
008			251003s1997 xxu||||| |||| 00| 0 eng c
020			_a978-0-521-67352-5
040			_aCL-VaUPLA _bspa _cCL-VaUPLA _erda
082	0	4	_a523.101515352 D997s _221
245	1	0	_aDynamical systems in cosmology / _cedited by J. Wainwright, G.F.R. Ellis
264		1	_aCambridge : _aNew York : _bCambridge University Press, _c1997
300			_axiv, 343 páginas : _bgráficos, tablas
336			_2rdacontent _atexto _btxt
337			_2rdamedia _ano mediado _bn
338			_2rdacarrier _avolumen _bnc
504			_aIncluye bibliografía
505	0		_aPart I. background - Part II. Spatially homogeneous cosmologies - Part III. Inhomogeneous cosmologies - Part IV. Conclusion
520			_aThis authoritative volume shows how modern dynamical systems theory can help us in understanding the evolution of cosmological models. It also compares this approach with Hamiltonian methods and numerical studies. A major part of the book deals with the spatially homogeneous (Bianchi) models and their isotropic subclass, the Friedmann-Lemaitre models, but certain classes of inhomogeneous models (for example, 'silent universes') are also examined. The analysis leads to an understanding of how special (high symmetry) models determine the evolution of more general families of models; and how these families relate to real cosmological observations. This is the first book to relate modern dynamical systems theory to both cosmological models and cosmological observations. It provides an invaluable reference for graduate students and researchers in relativity, cosmology and dynamical systems theory.
546			_aTexto en inglés
650		4	_aCOSMOLOGIA _xMODELOS MATEMATICOS
650		4	_aSISTEMAS DINAMICOS DIFERENCIALES
700	1		_aWainwright, J. _q(John), _924483 _eeditor
700	1		_aEllis, George F. R. _q(George Francis Rayner), _924484 _eeditor
942			_cLB _n0 _2ddc
998			_cAAR _d03/10/25
999			_c226352 _d226352