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The focus of our study is on the Bianchi-type VI₀ inflationary universe and how it behaves when a massless scalar field with a flat potential is present. Our goal is to identify an inflationary solution, which we achieved by identifying a flat region where the potential V remains constant. We have thoroughly examined the inflationary scenario of this model.
Maheshwari et al. (2024) studied this question.
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