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Collective Effects In Disk Galaxies | 79942
ISSN: 2329-6542

Journal of Astrophysics & Aerospace Technology
Open Access

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Collective effects in disk galaxies

2nd International Conference on Astrophysics and Particle Physics

Xiaolei Zhang

George Mason University, USA

ScientificTracks Abstracts: J Astrophys Aerospace Technol

DOI: 10.4172/2329-6542-C1-011

Collective effects originate in physical systems going through non-equilibrium phase transitions, which produce selforganised global structures that often serve to accelerate the rates of entropy-increasing thermodynamical evolution of their parent systems. The examples of such emergence behavior and the resulting hierarchical organization of physical laws and phenomena, ranging from models of spontaneous breaking of gauge symmetry in high-energy physics, to the emergence of quasi-particle behavior in condensed matter physics. Emergent behaviors can also be exhibited by classical many-body systems governed by Newtonian laws of gravity. In the case of disk galaxies, we show that the spontaneous emergence of spiral modes is an example of non-equilibrium phase transition, accompanied by the condition of collisionless-shock at the density wave crest. This condition further allows the interaction of matter with the basic state of the galactic disk with the density wave modes, which leads to the stabilization of the modal amplitude growth and the secular radial mass redistribution on the basic state, giving rise to galaxy morphological evolution along the Hubble sequence. It is shown further that well-known classical approaches of applying the Boltzmann kinetic equation, as well as its moment-equation descendants the Euler and NavierStokes fluid equations for studying galactic dynamics problems, are inadequate for treating the maintenance of density wave modes as well as the long-term evolution of the morphology of disk galaxies. A global and synthetic approach, incorporating the correlated fluctuations of stars and gas cloud, is adopted to supplement the continuum approach.

Xiaolei Zhang obtained her PhD from the University of California, Berkeley, in 1992 and was a Post-doctoral fellow at the Harvard-Smithsonian Center for Astrophysics (CfA) from 1992-1995. She subsequently worked at the CFA as a Staff Scientist, at NASA's Goddard Space Flight Center as a Contractor and at the US Naval Research Lab as a Civil Servant Astrophysicist. She took an early retirement in order to devote more time to her interests in the foundations of physics, in astrophysics, as well as in art. She is currently an Affiliate Faculty at the George Mason University.