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Dynamical Evolution of Galaxies
By (author) Xiaolei Zhang
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| book description |
This 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. Contents Dynamical Drivers of Galaxy Evolution N-Body Simulations of Galaxy Evolution Astrophysical Implications of the Dynamical Theory Putting It All Together Concluding Remarks Appendix: Relation to Kinetics and Fluid Mechanics
| product details |
Normally shipped |
Publisher | De Gruyter
Published date | 4 Dec 2017
Language |
Format | Digital (delivered electronically)
Pages | 337
Dimensions | 0 x 0 x 0mm (L x W x H)
Weight | 0g
ISBN | 978-3-1105-2742-1
Readership Age |
BISAC | science / astronomy
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