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http://hdl.handle.net/123456789/928Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Singh, KM Bharti | - |
| dc.date.accessioned | 2018-08-22T10:14:18Z | - |
| dc.date.available | 2018-08-22T10:14:18Z | - |
| dc.date.issued | 2018-08-22 | - |
| dc.identifier.uri | http://hdl.handle.net/123456789/928 | - |
| dc.description.abstract | Dynamics of universe can be described by Einstein’s field equations.FLRW metric is one of the solutions of Einstein’s field equations. In This work, I studied evolution equation of universe in flat geometry, observational evidences of dark energy. And Scalar field model of Dark Energy which can be the candidates of Dark energy. I mainly focused on Quintessence model; it’s phase plain analysis and parameterization of quintessence model to understand the cosmic dynamic of the universe. Quintessence is canonical scalar field which is introduced to explain late- time cosmic acceleration. The evolution of Dark Energy equation of state depends on the field potential and its properties :tracking and thawing. | en_US |
| dc.description.sponsorship | IISERM | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | IISERM | en_US |
| dc.subject | Stability analysis | en_US |
| dc.subject | Evidences of Dark Energy | en_US |
| dc.subject | Parameterization of Quintessence Model | en_US |
| dc.title | Stability analysis of Quintessence Dark Energy | en_US |
| dc.type | Thesis | en_US |
| dc.guide | Jassal, H.K. | - |
| Appears in Collections: | MS-13 | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| MS13024.pdf | 710.55 kB | Adobe PDF | View/Open |
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