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Volumn 74, Issue 12, 2006, Pages

Predictions of dynamically emerging brane inflation models

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EID: 33751559201     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.74.123501     Document Type: Article
Times cited : (6)

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    • One way to avoid the defect overabundance problem is to enhance the symmetry which is broken during the annihilation; this can be achieved by having several overlapping branes instead of just one.
    • One way to avoid the defect overabundance problem is to enhance the symmetry which is broken during the annihilation; this can be achieved by having several overlapping branes instead of just one.
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    • Nevertheless, there are possibilities to enhance suppressed reheating channels by considering large vacuum expectation values of scalar matter fields after inflation, see e.g..
    • Nevertheless, there are possibilities to enhance suppressed reheating channels by considering large vacuum expectation values of scalar matter fields after inflation, see e.g..
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    • Notice that g is expected to be small in our model. As a consequence, condition 67 is not satisfied and preheating will not progress in the regime of narrow parametric resonance.
    • Notice that g is expected to be small in our model. As a consequence, condition 67 is not satisfied and preheating will not progress in the regime of narrow parametric resonance.
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