Abstract
All the popular models for structure formation are based on three key ingredients: (a) a model for the background universe (b) some mechanism for generating small perturbations in the early universe and (c) specification of the nature of the dark matter.
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© 1996 International Astronomical Union
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Padmanabhan, T. (1996). Structure Formation: Models, Dynamics and Status. In: Kochanek, C.S., Hewitt, J.N. (eds) Astrophysical Applications of Gravitational Lensing. International Astronomical Union / Union Astronomique Internationale, vol 173. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0221-3_14
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DOI: https://doi.org/10.1007/978-94-009-0221-3_14
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