Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/679
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dc.contributor.authorMulani, Imrankhan B.-
dc.date.accessioned2016-09-05T13:31:33Z-
dc.date.available2016-09-05T13:31:33Z-
dc.date.issued2016-09-05-
dc.identifier.urihttp://hdl.handle.net/123456789/679-
dc.description.abstractLarge scale properties of the universe can be explained by Einstein's general theory of relativity. A-CDM model incorporating general relativity predicts the accelerated expansion of universe and large scale distribution of galaxies. Structure formation equation obtained from this model are non linear and difficult to solve. Newtonian theory of gravity can be applied to situations after decoupling of matter and radiation. Newton himself tried to apply his theory to universe but failed. Reason for failure is that he considered static model with infinite stars. This result in divergences. The divergences can be avoided by assuming finite number of particles interacting only through gravitational attraction. This thesis is review of Newtonian cosmological theory of finite number of discrete particles interacting through gravitational attraction, also with Newtonian version of cosmological constant. Exact solution we get for Newtonian equations are homothetically expanding background with comoving positions constituting a central configuration. The scale factor satisfy Rauchaudhuri and Friedmann equations without making any uid approximation. These solutions can be linearised to get perturbation theory for structure formation calculations.en_US
dc.description.sponsorshipIISER-Men_US
dc.language.isoenen_US
dc.publisherIISER-Men_US
dc.subjectPhysicsen_US
dc.subjectAstronomyen_US
dc.subjectCosmologyen_US
dc.subjectDiscrete Newtonian Cosmologyen_US
dc.titleReview of Discrete Newtonian Cosmologyen_US
dc.typeThesisen_US
dc.guideBagla, J.S.-
Appears in Collections:MS Dissertation by MP-2012

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