LEADER 00704nam0-22002771i-450- 001 990000996560403321 035 $a000099656 035 $aFED01000099656 035 $a(Aleph)000099656FED01 035 $a000099656 100 $a20000920d1964----km-y0itay50------ba 101 0 $aeng 200 1 $aInventing the Future$fDennis Gabor 210 $aNew York$cAlfred A. Knopf$d1964 215 $a237 p.$d21 cm 610 0 $aMiscellanea 676 $a082 700 1$aGabor,$bDennis$026012 801 0$aIT$bUNINA$gRICA$2UNIMARC 901 $aBK 912 $a990000996560403321 952 $a41-001$b5274$fFI1 959 $aFI1 996 $aInventing the Future$9354151 997 $aUNINA DB $aING01 LEADER 02975nam 2200517 450 001 9910467392203321 005 20200520144314.0 010 $a3-11-052544-5 024 7 $a10.1515/9783110527421 035 $a(CKB)4100000001501832 035 $a(MiAaPQ)EBC5158159 035 $a(DE-B1597)474551 035 $a(OCoLC)1015880558 035 $a(DE-B1597)9783110527421 035 $a(Au-PeEL)EBL5158159 035 $a(CaPaEBR)ebr11480463 035 $a(EXLCZ)994100000001501832 100 $a20171215h20182018 uy| 0 101 0 $aeng 135 $aurcnu|||||||| 181 $2rdacontent 182 $2rdamedia 183 $2rdacarrier 200 10$aDynamical evolution of galaxies /$fZiaolei Zhang 210 1$aBerlin ;$aBoston :$cDe Gruyter,$d[2018] 210 4$dİ2018 215 $a1 online resource (338 pages) 311 $a3-11-052519-4 311 $a3-11-052742-1 320 $aIncludes bibliographical references and index. 327 $tFrontmatter -- $tPreface -- $tContents -- $t1. Introduction -- $t2. Dynamical Drivers of Galaxy Evolution -- $t3. N-Body Simulations of Galaxy Evolution -- $t4. Astrophysical Implications of the Dynamical Theory -- $t5. Putting It All Together -- $t6. Concluding Remarks -- $t7. Appendix: Relation to Kinetics and Fluid Mechanics -- $tReferences -- $tIndex 330 $aThis research monograph presents a new dynamical framework for the study of secular morphological evolution of galaxies along the Hubble sequence. Classical approaches based on Boltzmann's kinetic equation, as well as on its moment-equation descendants the Euler and Navier-Stokes fluid equations, are inadequate for treating the maintenance and long-term evolution of systems containing self-organized structures such as galactic density-wave modes. A global and synthetic approach, incorporating correlated fluctuations of the constituent particles during a nonequilibrium phase transition, is adopted to supplement the continuum treatment. The cutting-edge research combining analytical, N-body simulational, and observational aspects, as well as the fundamental-physics connections it provides, make this work a valuable reference for researchers and graduate students in astronomy, astrophysics, cosmology, many-body physics, complexity theory, and other related fields. ContentsDynamical Drivers of Galaxy EvolutionN-Body Simulations of Galaxy EvolutionAstrophysical Implications of the Dynamical TheoryPutting It All TogetherConcluding RemarksAppendix: Relation to Kinetics and Fluid Mechanics 606 $aGalaxies$xEvolution 606 $aNucleosynthesis 607 $aMilky Way 608 $aElectronic books. 615 0$aGalaxies$xEvolution. 615 0$aNucleosynthesis. 700 $aZhang$b Xiaolei$01035879 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910467392203321 996 $aDynamical evolution of galaxies$92455820 997 $aUNINA LEADER 01269nas 2200409-a 450 001 996207349903316 005 20240413025831.0 011 $a1848-6061 035 $a(DE-599)ZDB2703756-3 035 $a(CKB)991042732562226 035 $a(CONSER)---97646424- 035 $a(EXLCZ)99991042732562226 100 $a19970228a19899999 --- - 101 0 $ahrv 200 00$aActa turistica /$fEkonomski fakultet Zagreb 210 $aZagreb $cFakultet 215 $a1 online resource 300 $aRefereed/Peer-reviewed 311 08$aPrint version: Acta turistica / 0353-4316 (DLC) 97646424 (OCoLC)299071501 606 $aTourism$zCroatia$vPeriodicals 606 $aTourism$2fast$3(OCoLC)fst01153142 606 $aTourismus$2stw 606 $aTourismuswirtschaft$2stw 606 $aKroatien$2stw 607 $aCroatia$2fast$1https://id.oclc.org/worldcat/entity/E39PBJqBvTfkJyB3h3MYHMm8G3 608 $aPeriodicals.$2fast 615 0$aTourism 615 7$aTourism. 615 7$aTourismus 615 7$aTourismuswirtschaft 615 7$aKroatien 712 02$aSveu?ili?te u Zagrebu.$bEkonomski fakultet. 906 $aJOURNAL 912 $a996207349903316 920 $aexl_impl conversion 996 $aActa turistica$92106514 997 $aUNISA