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The dispersion relations [15, 22] imply that the fastest growing mode for the potential ((1)) has the Floquet exponent αmax = φ(A−2λφ) 4 √ m2−Aφ+λφ2

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hep-th 1

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2019 1

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CONDITIONAL 1

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Fundamental Forces and Scalar Field Dynamics in the Early Universe

hep-th · 2019-08-28 · conditional · novelty 7.0

The paper shows that generalized scalar weak gravity conjectures imply the parameter conditions for early-universe scalar condensates to fragment into solitonic lumps, which could form dark matter or primordial black holes.

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  • Fundamental Forces and Scalar Field Dynamics in the Early Universe hep-th · 2019-08-28 · conditional · none · ref 2

    The paper shows that generalized scalar weak gravity conjectures imply the parameter conditions for early-universe scalar condensates to fragment into solitonic lumps, which could form dark matter or primordial black holes.