Planck constraints and gravitational wave forecasts for primordial black hole dark matter seeded by multifield inflation

Qin, Wenzer; Geller, Sarah R.; Balaji, Shyam; McDonough, Evan; Kaiser, David I.

doi:10.1103/physrevd.108.043508

Title: Planck constraints and gravitational wave forecasts for primordial black hole dark matter seeded by multifield inflation

Journal Article · Thu Aug 03 00:00:00 UTC 2023 · Physical Review. D.

DOI: https://doi.org/10.1103/physrevd.108.043508 · OSTI ID:2420212

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Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States); OSTI
Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
Centre National de la Recherche Scientifique-Mixed Organizations (CNRS-UMR), Paris (France); Sorbonne Univ., Paris (France)
University of Winnipeg, Winnipeg, MB (Canada)

Here, we perform a Markov Chain Monte Carlo analysis of a simple yet generic multifield inflation model characterized by two scalar fields coupled to each other and nonminimally coupled to gravity, fit to Planck 2018 cosmic microwave background (CMB) data. In particular, model parameters are constrained by data on the amplitude of the primordial power spectrum of scalar curvature perturbations on CMB scales A_s, the spectral index n_s, and the ratio of power in tensor to scalar modes r, with a prior that the primordial power spectrum should also lead to primordial black hole (PBH) production sufficient to account for the observed dark matter abundance. We find that n_s in particular controls the constraints on our model. Whereas previous studies of PBH formation from an ultraslow-roll phase of inflation have highlighted the need for at least one model parameter to be highly fine-tuned, we identify a degeneracy direction in parameter space such that shifts by ~10% of one parameter can be compensated by comparable shifts in other parameters while preserving a close fit between model predictions and observations. Furthermore, we find this allowed parameter region produces observable gravitational wave signals in the frequency ranges to which upcoming experiments are projected to be sensitive, including Advanced LIGO and Virgo, the Einstein Telescope, Cosmic Explorer, DECIGO, and LISA.

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Research Organization:: Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: SC0012567

OSTI ID:: 2420212

Journal Information:: Physical Review. D., Journal Name: Physical Review. D. Journal Issue: 4 Vol. 108; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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