Peaks and rings on the cosmic microwave background
We simulate maps of the microwave background radiation for a model of inflationary primordial voids plus standard cold dark matter. For some values of the parameters, we find in the angular power spectrum a well-defined second peak at l 1000, correlated with the size, amplitude, and number of the pr...
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| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
1997 November 14
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| In: |
The astrophysical journal. Part 2, Letters
Year: 1998, Jahrgang: 492, Heft: 1, Pages: L5-L8 |
| ISSN: | 2041-8213 |
| DOI: | 10.1086/311081 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1086/311081 Verlag, Volltext: http://stacks.iop.org/1538-4357/492/i=1/a=L5 
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| Verfasserangaben: | Luca Amendola, Carlo Baccigalupi, and Franco Occhionero |
MARC
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| 520 | |a We simulate maps of the microwave background radiation for a model of inflationary primordial voids plus standard cold dark matter. For some values of the parameters, we find in the angular power spectrum a well-defined second peak at l 1000, correlated with the size, amplitude, and number of the primordial voids. The next generation of microwave background maps will be able to test the scenario of inflationary first-order phase transitions. | ||
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