In the flat slicing of de Sitter spacetime, , , a Fourier mode of a minimally coupled massless scalar field obeys . Substitution verifies the displayed positive-frequency branch. The Canonically rescaled de Sitter scalar mode is , a different variable satisfying . For nonzero , the opposite-frequency branch completes the time solution; at the solutions are and . This separation avoids losing the homogeneous decaying mode by taking a restricted ansatz literally at zero wave number.
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