LEADER 03741nam 22006135 450 001 9910741195803321 005 20250609112111.0 010 $a981-13-2935-4 024 7 $a10.1007/978-981-13-2935-7 035 $a(CKB)4100000007181105 035 $a(MiAaPQ)EBC5606716 035 $a(DE-He213)978-981-13-2935-7 035 $a(MiAaPQ)EBC6237243 035 $a(EXLCZ)994100000007181105 100 $a20181127d2018 u| 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aBig-Bang Nucleosynthesis $eThermonuclear History in the Early Universe /$fby Masa-aki Hashimoto, Riou Nakamura, E. P. Berni Ann Thushari, Kenzo Arai 205 $a1st ed. 2018. 210 1$aSingapore :$cSpringer Singapore :$cImprint: Springer,$d2018. 215 $a1 online resource (93 pages) 225 1 $aSpringerBriefs in Physics,$x2191-5423 311 08$a981-13-2934-6 327 $aIntroduction -- The Standard Model of Cosmology -- Theories Beyond The Standard Model -- Modified Brans-Dicke Theory -- Appendix A: Einstein Tensor -- Appendix B: Thermal History in an Early Universe -- Appendix C: Numerical Approach to Calculate Nucleosynthesis -- Appendix D: Some Useful Numbers. 330 $aThe book reviews theories of nucleosynthesis in big-bang cosmology. It introduces the standard model of cosmology, astronuclear reactions, numerical techniques for nucleosynethsis, and describes in detail the theories that go beyond the standard models, enabling readers to grasp the physics of big-bang nucleosynthesis on the basis of cosmology, general relativity and nuclear physics. In addition, the authors provide insights into the theoretical constrains required by observations. As a consequence, readers find out that big-bang nucleosynthesis still has windows opened to another cosmology. Although the book focuses on highly advanced topics, it is concisely written and mathematical derivations are explained step-by-step, making it accessible to graduate readers. Thus it is a short monograph appealing to a variety of readers interested in nucleosynthesis of big-bang cosmology. 410 0$aSpringerBriefs in Physics,$x2191-5423 606 $aAstrophysics 606 $aMathematical physics 606 $aNuclear physics 606 $aCosmology$3http://scigraph.springernature.com/things/product-market-codes/P22049 606 $aTheoretical Astrophysics$3http://scigraph.springernature.com/things/product-market-codes/P22080 606 $aNuclear Physics, Heavy Ions, Hadrons$3http://scigraph.springernature.com/things/product-market-codes/P23010 606 $aAstrophysics and Astroparticles$3http://scigraph.springernature.com/things/product-market-codes/P22022 606 $aClassical and Quantum Gravitation, Relativity Theory$3http://scigraph.springernature.com/things/product-market-codes/P19070 615 0$aAstrophysics. 615 0$aMathematical physics. 615 0$aNuclear physics. 615 14$aCosmology. 615 24$aTheoretical Astrophysics. 615 24$aNuclear Physics, Heavy Ions, Hadrons. 615 24$aAstrophysics and Astroparticles. 615 24$aClassical and Quantum Gravitation, Relativity Theory. 676 $a523.18 700 $aHashimoto$b Masa-aki$4aut$4http://id.loc.gov/vocabulary/relators/aut$01424119 702 $aNakamura$b Riou$4aut$4http://id.loc.gov/vocabulary/relators/aut 702 $aThushari$b E. P. Berni Ann$4aut$4http://id.loc.gov/vocabulary/relators/aut 702 $aArai$b Kenzo$4aut$4http://id.loc.gov/vocabulary/relators/aut 906 $aBOOK 912 $a9910741195803321 996 $aBig-Bang Nucleosynthesis$93553000 997 $aUNINA