LEADER 03324nam 22006612 450 001 9910814689903321 005 20151005020622.0 010 $a1-107-17943-2 010 $a1-281-04051-7 010 $a9786611040512 010 $a0-511-33487-7 010 $a0-511-33427-3 010 $a0-511-33359-5 010 $a0-511-57351-0 010 $a0-511-61128-5 010 $a0-511-33545-8 035 $a(CKB)1000000000478701 035 $a(EBL)307423 035 $a(OCoLC)417252320 035 $a(SSID)ssj0000145391 035 $a(PQKBManifestationID)11163587 035 $a(PQKBTitleCode)TC0000145391 035 $a(PQKBWorkID)10156719 035 $a(PQKB)11060902 035 $a(UkCbUP)CR9780511611285 035 $a(MiAaPQ)EBC307423 035 $a(Au-PeEL)EBL307423 035 $a(CaPaEBR)ebr10193776 035 $a(CaONFJC)MIL104051 035 $a(PPN)261313169 035 $a(EXLCZ)991000000000478701 100 $a20090910d2007|||| uy| 0 101 0 $aeng 135 $aur||||||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aElements of string cosmology /$fMaurizio Gasperini$b[electronic resource] 210 1$aCambridge :$cCambridge University Press,$d2007. 215 $a1 online resource (xv, 552 pages) $cdigital, PDF file(s) 300 $aTitle from publisher's bibliographic system (viewed on 05 Oct 2015). 311 $a0-521-18798-2 311 $a0-521-86875-0 320 $aIncludes bibliographical references and index. 327 $aA short review of standard and inflationary cosmology -- The basic string cosmology equations -- Conformal invariance and string effective actions -- Duality symmetries and cosmological solutions -- Inflationary kinematics -- The string phase -- The cosmic background of relic gravitational waves -- Scalar perturbations and the anistropy of the CMB radiation -- Dilaton phenomenology -- Elements of brane cosmology. 330 $aThe standard cosmological picture of our Universe emerging from a 'big bang' leaves open many fundamental questions which string theory, a unified theory of all forces of nature, should be able to answer. This 2007 text was the first dedicated to string cosmology, and contains a pedagogical introduction to the basic notions of the subject. It describes the possible scenarios suggested by string theory for the primordial evolution of our Universe. It discusses the main phenomenological consequences of these scenarios, stresses their differences from each other, and compares them to the more conventional models of inflation. The book summarises over 15 years of research in this field and introduces advances. It is self-contained, so it can be read by astrophysicists with no knowledge of string theory, and high-energy physicists with little understanding of cosmology. Detailed and explicit derivations of all the results presented provide a deeper appreciation of the subject. 606 $aCosmology 606 $aString models 615 0$aCosmology. 615 0$aString models. 676 $a530.14 700 $aGasperini$b Maurizio$040394 801 0$bUkCbUP 801 1$bUkCbUP 906 $aBOOK 912 $a9910814689903321 996 $aElements of string cosmology$93913632 997 $aUNINA