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Double-graviton production from Standard Model plasma

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arxiv 2401.08766 v2 pith:MV4QDWUW submitted 2024-01-16 hep-ph astro-ph.COgr-qc

Double-graviton production from Standard Model plasma

classification hep-ph astro-ph.COgr-qc
keywords productionmodelstandardalphacontributionsdouble-gravitongravitonplasma
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The thermal plasma filling the early universe generated a stochastic gravitational wave background that peaks in the microwave frequency range today. If the graviton production rate is expressed as a series in a fine-structure constant, $\alpha$, and the temperature over the Planck mass, $T^2_{ } / m_{\rm pl}^2$, then the lowest-order contributions come from single ($\sim \alpha T^2_{ }/m_{\rm pl}^2$) and double ($\sim T^4_{ }/m_{\rm pl}^4$) graviton production via $2\to 2$ scatterings. We show that in the Standard Model, single-graviton production dominates if the maximal temperature is smaller than $4\times 10^{18}_{ }$ GeV. This justifies previous calculations which relied solely on single-graviton production. We mention Beyond the Standard Model scenarios in which the single and double-graviton contributions could be of comparable magnitudes. Finally, we elaborate on what these results imply for the range of applicability of General Relativity as an effective theory.

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