000			03625nam a22003855i 4500
001			293742
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005			20160429155118.0
007			cr nn 008mamaa
008			150903s2005 gw | o |||| 0|eng d
020			_a9783540269991 _99783540269991
024	7		_a10.1007/b138455 _2doi
035			_avtls000346808
039		9	_a201509031101 _bVLOAD _c201405070512 _dVLOAD _y201402070906 _zstaff
040			_aMX-SnUAN _bspa _cMX-SnUAN _erda
100	1		_aGabrielli, Andrea. _eautor _9315579
245	1	0	_aStatistical Physics for Cosmic Structures / _cby Andrea Gabrielli, Francesco Sylos Labini, Michael Joyce, Luciano Pietronero.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c2005.
300			_axiii, 424 páginas 119 ilustraciones _brecurso en línea.
336			_atexto _btxt _2rdacontent
337			_acomputadora _bc _2rdamedia
338			_arecurso en línea _bcr _2rdacarrier
347			_aarchivo de texto _bPDF _2rda
500			_aSpringer eBooks
505	0		_aStatistical Methods -- Uniform and Correlated Mass Density Fields -- The Power Spectrum and the Classification of Stationary Stochastic Fields -- Fractals -- Multifractals and Mass Distributions -- Applications to Cosmology -- Fluctuations in Standard Cosmological Models: A Real Space View -- Discrete Representation of Fluctuations in Cosmological Models -- Galaxy Surveys: An Introduction to Their Analysis -- Characterizing the Observed Distribution of Visible Matter I: The Conditional Average Density in Galaxy Catalogs -- Characterizing the Observed Distribution of Visible Matter II: Number Counts and Their Fluctuations -- Luminosity in Galaxy Correlations -- The Distribution of Galaxy Clusters -- Biasing a Gaussian Random Field and the Problem of Galaxy Correlations -- The Gravitational Field in Stochastic Particle Distributions.
520			_aThe physics of scale-invariant and complex systems is a novel interdisciplinary field. Its ideas allow us to look at natural phenomena in a radically new and original way, eventually leading to unifying concepts independent of the detailed structure of the systems. The objective is the study of complex, scale-invariant, and more general stochastic structures that appear both in space and time in a vast variety of natural phenomena, which exhibit new types of collective behaviors, and the fostering of their understanding. This book has been conceived as a methodological monograph in which the main methods of modern statistical physics for cosmological structures and density fields (galaxies, Cosmic Microwave Background Radiation, etc.) are presented in detail. The main purpose is to present clearly, to a workable level, these methods, with a certain mathematical accuracy, providing also some paradigmatic examples of applications. This should result in a new and more general framework for the statistical analysis of the many new data concerning the different cosmic structures which characterize the large scale Universe and for their theoretical interpretation and modeling.
590			_aPara consulta fuera de la UANL se requiere clave de acceso remoto.
700	1		_aLabini, Francesco Sylos. _eautor _9326645
700	1		_aJoyce, Michael. _eautor _9326646
700	1		_aPietronero, Luciano. _eautor _9326647
710	2		_aSpringerLink (Servicio en línea) _9299170
776	0	8	_iEdición impresa: _z9783540407454
856	4	0	_uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/b138455 _zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999			_c293742 _d293742