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- W2783446990 abstract "In the past 15–20 years N-body simulations have been widely used for galactic evolution studies. However, despite this great potential, their applications to studies of galactic habitability are still in their infancy. This is largely because the necessary tools for analysis and quantification of habitability from N-body simulation data are not developed. The aim of this chapter is to help bridge this gap. The main areas of N-body simulation application for galactic evolution studies are discussed in the context of habitability. The great dynamical range of N-body simulations gives an opportunity for analyzing habitability relevant phenomena on both small (collision of two galaxies) and large (interactions within groups of galaxies) scales. This approach provides an opportunity to connect the galactic habitability studies to cosmological phenomena. We also discuss how the already quantified galactic habitability can be related to a local scale phenomenon such as the habitability of particular stellar systems." @default.
- W2783446990 created "2018-01-26" @default.
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- W2783446990 date "2018-01-01" @default.
- W2783446990 modified "2023-09-26" @default.
- W2783446990 title "N-Body Simulations and Galactic Habitability" @default.
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- W2783446990 doi "https://doi.org/10.1016/b978-0-12-811940-2.00008-3" @default.
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