Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2007-06-19
JHEP 0706:080,2007
Physics
High Energy Physics
High Energy Physics - Phenomenology
12 pages, 0 tables, 4 figures, accepted for publication in JHEP
Scientific paper
10.1088/1126-6708/2007/06/080
In the present work we discuss cosmic strings in natural inflation. Our analysis is based entirely on the CMB quadrupole temperature anisotropy and on the existing upper bound on the cosmic string tension. Our results show that the allowed range for both parameters of the inflationary model is very different from the range obtained recently if cosmic strings are formed at the same time with inflation, while if strings are formed after inflation we find that the parameters of the inflationary model are similar to the ones obtained recently.
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