Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/3411
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Subrahmanyan, Ravi | - |
dc.date.accessioned | 2008-02-01T11:13:24Z | - |
dc.date.available | 2008-02-01T11:13:24Z | - |
dc.date.issued | 1997 | - |
dc.identifier.citation | Journal of Astrophysics and Astronomy, 1997, Vol.18, p251-255 | en |
dc.identifier.issn | 0250-6335 | - |
dc.identifier.uri | http://hdl.handle.net/2289/3411 | - |
dc.description | Open Access. Scanned images provided by the NASA ADS. | en |
dc.description.abstract | The discovery of the 3 K microwave background radiation (MBR) and its interpretation as a relict of the hot big bang was probably the most important observation that led to the elevation of the hot big bang model to the status of a 'Standard Model'. The temperature of this background is consistent with the primordial nucleosynthesis hypothesis. Detailed measurements of the spectrum and angular anisotropy of this radiation background have been found - within the measurement errors - to be consistent with the expectations of the Standard Model and with the formation of structure from the gravitational growth of primordial seed density perturbations within this framework. | en |
dc.format.extent | 537807 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Indian Academy of Sciences, Bangalore, India. | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1997JApA...18..251S | en |
dc.rights | 1997 The Indian Academy of Sciences. | en |
dc.subject | Cosmic microwave background | en |
dc.subject | cosmology: observations | en |
dc.subject | cosmology: theory | en |
dc.title | Microwave background radiation related evidence in favour of the standard model | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1997 JAA V18 p251S.pdf Restricted Access | Open Access | 525.2 kB | Adobe PDF | View/Open Request a copy |
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.