Dark Radiation from Inflationary Fluctuations

Abstract

Light new vector bosons can be produced gravitationally through quantum fluctuations during inflation; if these particles are feebly coupled and cosmologically metastable, they can account for the observed dark matter abundance. However, in minimal anomaly free $U(1)$ extensions to the Standard Model, these vectors generically decay to neutrinos if at least one neutrino mass eigenstate is sufficiently light. If these decays occur between neutrino decoupling and CMB freeze out, the resulting radiation energy density can contribute to $\Delta N_{\mathrm{eff}}$ at levels that can ameliorate the Hubble tension and be discovered with future CMB and relic neutrino detection experiments. Since the additional neutrinos are produced from vector decays after BBN, this scenario predicts $\Delta N_{\mathrm{eff}}>0$ at recombination, but $\Delta N_{\mathrm{eff}}=0$ during BBN. Furthermore, due to a fortuitous cancellation, the contribution to $\Delta N_{\mathrm{eff}}$ is approximately mass independent.

6 pages, 3 figures. Expanded discussion of PTOLEMY signals, conclusions unchanged. Matches published version

References in corpus (8)

• The Hubble Hunter's Guide
• Bosonic super-WIMPs as keV-scale dark matter
• Cosmology With a Very Light $L_{\mu }-L_{\tau }$ Gauge Boson
• Cosmological Constraints on Very Dark Photons
• Gravitational Effects on Inflaton Decay
• BBN constraints on the annihilation of MeV-scale dark matter
• Searching for dilepton resonances below the Z mass at the LHC
• Irruption of massive particle species during inflation

Cited by in corpus (3)

• Probing Physics Beyond the Standard Model: Limits from BBN and the CMB Independently and Combined
• Sterile neutrino dark matter catalyzed by a very light dark photon
• Two sides of the same coin: sterile neutrinos and dark radiation. Status and perspectives