Peaks and rings on the cosmic microwave background

被引:11
作者
Amendola, L
Baccigalupi, C
Occhionero, F
机构
[1] Osservatorio Astron Roma, I-00136 Rome, Italy
[2] Ist Nazl Fis Nucl, I-44100 Ferrara, Italy
[3] Univ Ferrara, Dipartimento Fis, I-44100 Ferrara, Italy
关键词
cosmic microwave background; early universe;
D O I
10.1086/311081
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 I similar to 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.
引用
收藏
页码:L5 / L8
页数:4
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