Primordial black holes and secondary gravitational waves from inflationary model with a non-canonical kinetic term

• Published in: arXiv.org
• Main Authors: Zhu, Yi, Gao, Qing, Gong, Yungui, Zong-hong, Zhu
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 10.04.2021
• Subjects: Curvature; Dark matter; Flux density; Gravitation; Gravitational waves; Peak frequency; Physics - Cosmology and Nongalactic Astrophysics; Physics - General Relativity and Quantum Cosmology; Pulsars
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.2011.10606

With the enhancement mechanism provided by a noncanonical kinetic term with a peak, the amplitude of primordial curvature perturbations can be enhanced by seven orders of magnitude at small scales while keeping to be consistent with observations at large scales. The peak function and inflationary potential are not restricted in this mechanism. We use the Higgs model and T-model as examples to show how abundant primordial black hole dark matter with different mass and scalar induced secondary gravitational waves with different peak frequency are generated. We also show that the enhanced power spectrum for the primordial curvature perturbations and the energy density of the scalar induced secondary gravitational waves can have either a sharp peak or a broad peak. The primordial black holes with the mass around \(10^{-14}-10^{-12} M_{\odot}\) produced with the enhancement mechanism can make up almost all dark matter, and the scalar induced secondary gravitational waves accompanied with the production of primordial black holes can be tested by the pulsar timing arrays and spaced based gravitational wave observatory. Therefore, the mechanism can be tested by primordial black hole dark matter and gravitational wave observations.