2021
DOI: 10.48550/arxiv.2104.12914
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Inflationary evolution in quantum cosmology from FRLW supersymmetric models

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“…In [39], we performed a qualitative discussion of several superpotentials that have diverse drawbacks, as phantom matter. Here, we consider a family of superpotentials…”
Section: Inflationary Modelmentioning
confidence: 99%
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“…In [39], we performed a qualitative discussion of several superpotentials that have diverse drawbacks, as phantom matter. Here, we consider a family of superpotentials…”
Section: Inflationary Modelmentioning
confidence: 99%
“…Following this procedure, we adjusted µ and λ, so that t exit ≈ t R and N = ln a(t exit )/a(t in ) ≈ 60. With these data, we computed the tensor to scalar ratio (39), and the scalar spectral index (41). We performed these steps for p = 1, 2, 3, 4, 5.…”
Section: Inflationary Modelmentioning
confidence: 99%