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Probing reheating temperature of the universe with gravitational wave background

3 Pith papers cite this work. Polarity classification is still indexing.

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abstract

Thermal history of the universe after big-bang nucleosynthesis (BBN) is well understood both theoretically and observationally, and recent cosmological observations also begin to reveal the inflationary dynamics. However, the epoch between inflation and BBN is scarcely known. In this paper we show that the detection of the stochastic gravitational wave background around 1Hz provides useful information about thermal history well before BBN. In particular, the reheating temperature of the universe may be determined by future space-based laser interferometer experiments such as DECIGO and/or BBO if it is around 10^{6-9} GeV, depending on the tensor-to-scalar ratio $r$ and dilution factor $F$.

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hep-ph 3

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2026 3

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UNVERDICTED 3

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background 2

representative citing papers

Dilaton-Flattened Axion Inflation

hep-ph · 2026-04-16 · unverdicted · novelty 7.0

Dilaton backreaction on an anomaly-inspired axion potential generates a closed-form Lambert-W flattened hilltop, giving r ≈ 0.033–0.036 and α_s ≈ −4.6×10^{-4} at N=56 with strictly adiabatic dynamics.

High Frequency Spectrum of Primordial Gravitational Waves

hep-ph · 2026-01-01 · unverdicted · novelty 5.0

High-frequency primordial gravitational waves extend to higher frequencies due to post-inflation inflaton dynamics, and their detailed spectrum shape can distinguish inflation models.

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