000			03388nam a22005055i 4500
001			u377806
003			SIRSI
005			20160812084521.0
007			cr nn 008mamaa
008			110209s2011 ne | s |||| 0|eng d
020			_a9789048186853 _9978-90-481-8685-3
040			_cMX-MeUAM
050		4	_aQC178
050		4	_aQC173.5-173.65
082	0	4	_a530.1 _223
100	1		_aMatarrese, Sabino. _eeditor.
245	1	0	_aDark Matter and Dark Energy _h[recurso electrónico] : _bA Challenge for Modern Cosmology / _cedited by Sabino Matarrese, Monica Colpi, Vittorio Gorini, Ugo Moschella.
264		1	_aDordrecht : _bSpringer Netherlands, _c2011.
300			_aXIV, 404 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aAstrophysics and Space Science Library, _x0067-0057 ; _v370
520			_aThis book brings together reviews from leading international authorities on the developments in the study of dark matter and dark energy, as seen from both their cosmological and particle physics side. Studying the physical and astrophysical properties of the dark components of our Universe is a crucial step towards the ultimate goal of unveiling their nature. The work developed from a doctoral school sponsored by the Italian Society of General Relativity and Gravitation. The book starts with a concise introduction to the standard cosmological model, as well as with a presentation of the theory of linear perturbations around a homogeneous and isotropic background. It covers the particle physics and cosmological aspects of dark matter and (dynamical) dark energy, including a discussion of how modified theories of gravity could provide a possible candidate for dark energy. A detailed presentation is also given of the possible ways of testing the theory in terms of cosmic microwave background, galaxy redshift surveys and weak gravitational lensing observations. Included is a chapter reviewing extensively the direct and indirect methods of detection of the hypothetical dark matter particles. Also included is a self-contained introduction to the techniques and most important results of numerical (e.g. N-body) simulations in cosmology. This volume will be useful to researchers, PhD and graduate students in Astrophysics, Cosmology Physics and Mathematics, who are interested in cosmology, dark matter and dark energy.
650		0	_aPhysics.
650		0	_aQuantum theory.
650	1	4	_aPhysics.
650	2	4	_aClassical and Quantum Gravitation, Relativity Theory.
650	2	4	_aElementary Particles, Quantum Field Theory.
650	2	4	_aAstrophysics and Astroparticles.
650	2	4	_aNumerical and Computational Physics.
650	2	4	_aMeasurement Science and Instrumentation.
700	1		_aColpi, Monica. _eeditor.
700	1		_aGorini, Vittorio. _eeditor.
700	1		_aMoschella, Ugo. _eeditor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9789048186846
830		0	_aAstrophysics and Space Science Library, _x0067-0057 ; _v370
856	4	0	_zLibro electrónico _uhttp://148.231.10.114:2048/login?url=http://link.springer.com/book/10.1007/978-90-481-8685-3
596			_a19
942			_cLIBRO_ELEC
999			_c205686 _d205686