Please use this identifier to cite or link to this item:
http://hdl.handle.net/123456789/2787Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Bagla, J.S. | - |
| dc.date.accessioned | 2020-12-08T05:28:21Z | - |
| dc.date.available | 2020-12-08T05:28:21Z | - |
| dc.date.issued | 2015 | - |
| dc.identifier.citation | Resonance, 20(9) | en_US |
| dc.identifier.other | 10.1007/s12045-015-0239-7 | - |
| dc.identifier.uri | https://link.springer.com/article/10.1007/s12045-015-0239-7 | - |
| dc.identifier.uri | http://hdl.handle.net/123456789/2787 | - |
| dc.description | Only IISERM authors are available in the record. | - |
| dc.description.abstract | We use Newtonian formalism to motivate the form of Friedmann equations that describe the expansion of the universe in the standard cosmological model. We use the same formalism to study the evolution of density perturbations in the universe. We show that a simple model like spherical collapse can be used to estimate the characteristics of halos of galaxies and clusters of galaxies | en_US |
| dc.language.iso | en_US | en_US |
| dc.publisher | Springer India | en_US |
| dc.subject | Cosmology | en_US |
| dc.subject | galaxy formation | en_US |
| dc.subject | gravitational collapse | en_US |
| dc.title | Gravitational collapse and structure formation in an expanding universe | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | Research Articles | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Need to add pdf.odt | 8.63 kB | OpenDocument Text | View/Open |
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