LEADER 01001nam2-2200349---450- 001 990000547100203316 035 $a0054710 035 $aUSA010054710 035 $a(ALEPH)000054710USA01 035 $a0054710 100 $a20010706d1976----km-y0itay0103----ba 101 $aita 102 $aIT 105 $a||||||||001yy 200 1 $a<> civiltà feudale$fdiretta da Lucio Lombardo radice 210 $aRoma$cEditori Riuniti$d1976 215 $a357 p.$cill.$d30 cm 410 $12001 461 $10010054703$12001$aUlisse. Enciclopedia della ricerca e della scoperta 610 0 $aEnciclopedie 676 $a035. 702 1$aLOMBARDO RADICE,$bLucio 801 0$aIT$bsalbc$gISBD 912 $a990000547100203316 951 $a035 ULI 2$b12552 SM$c035$d00107144 959 $aBK 969 $aSCI 979 $aPATTY$b90$c20010706$lUSA01$h1033 979 $c20020403$lUSA01$h1704 979 $aPATRY$b90$c20040406$lUSA01$h1638 996 $aCiviltà feudale$9885036 997 $aUNISA LEADER 03348nam 22005295 450 001 9910300548003321 005 20200704172540.0 010 $a3-319-92672-1 024 7 $a10.1007/978-3-319-92672-8 035 $a(CKB)3810000000358880 035 $a(MiAaPQ)EBC5450464 035 $a(DE-He213)978-3-319-92672-8 035 $a(PPN)229492126 035 $a(EXLCZ)993810000000358880 100 $a20180616d2018 u| 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aScalar Fields in Numerical General Relativity $eInhomogeneous Inflation and Asymmetric Bubble Collapse /$fby Katy Clough 205 $a1st ed. 2018. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2018. 215 $a1 online resource (207 pages) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 311 $a3-319-92671-3 327 $aPart I: Background Material -- Introduction -- Technical Background -- Part II: Code Development Work -- GRChombo - Code Development and Testing -- Part III: Research Work -- Inhomogeneous Inflation -- Critical Bubble Collapse -- Conclusions and Further Work. 330 $aThis book explores the use of numerical relativity (NR) methods to solve cosmological problems, and describes one of the first uses of NR to study inflationary physics. NR consists in the solution of Einstein?s Equation of general relativity, which governs the evolution of matter and energy on cosmological scales, and in systems where there are strong gravitational effects, such as around black holes. To date, NR has mainly been used for simulating binary black hole and neutron star mergers like those detected recently by LIGO. Its use as a tool in fundamental problems of gravity and cosmology is novel, but rapidly gaining interest. The author investigates the initial condition problem in early universe cosmology ? whether an inflationary expansion period could have ?got going? from initially inhomogeneous conditions ? and identifies criteria for predicting the robustness of particular models. Further, it develops state-of-the-art numerical relativity tools in order to address this question, which are now publicly available. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aCosmology 606 $aGravitation 606 $aPhysics 606 $aCosmology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22049 606 $aClassical and Quantum Gravitation, Relativity Theory$3https://scigraph.springernature.com/ontologies/product-market-codes/P19070 606 $aNumerical and Computational Physics, Simulation$3https://scigraph.springernature.com/ontologies/product-market-codes/P19021 615 0$aCosmology. 615 0$aGravitation. 615 0$aPhysics. 615 14$aCosmology. 615 24$aClassical and Quantum Gravitation, Relativity Theory. 615 24$aNumerical and Computational Physics, Simulation. 676 $a530.11015153 700 $aClough$b Katy$4aut$4http://id.loc.gov/vocabulary/relators/aut$01060608 906 $aBOOK 912 $a9910300548003321 996 $aScalar Fields in Numerical General Relativity$92514572 997 $aUNINA