Please use this identifier to cite or link to this item:
https://olympias.lib.uoi.gr/jspui/handle/123456789/15923| Title: | Is the CMB shift parameter connected with the growth of cosmological perturbations? |
| Institution and School/Department of submitter: | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών |
| Keywords: | cosmic microwave background,large-scale structure of universe,dark energy,lambda,component,universe,models,matter |
| URI: | https://olympias.lib.uoi.gr/jspui/handle/123456789/15923 |
| ISSN: | 0035-8711 |
| Link: | <Go to ISI>://000256732700015 http://onlinelibrary.wiley.com/store/10.1111/j.1365-2966.2008.13303.x/asset/j.1365-2966.2008.13303.x.pdf?v=1&t=h0xqy3ky&s=d4db6361e654ff96c46d4f62cba72dbf1582cedb |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Basilakos-2008-Is the CMB shift par.pdf | 506.16 kB | Adobe PDF | View/Open |
This item is licensed under a Creative Commons License
