Abstract
We show that considering the torsion in early universe, we are led to an inflationary expansion with only a massless scalar field, so avoiding all physical questions that we are facing when working with massive scalar field.
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De Sabbata, V., Sivaram, C. Torsion and inflation. Astrophys Space Sci 176, 141–144 (1991). https://doi.org/10.1007/BF00643084
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DOI: https://doi.org/10.1007/BF00643084