Nanohertz gravitational waves from supergravity inflationary model with double-inflection-point

Author:

Gao Tie-JunORCID,Sun Ke-Sheng,Yang Xiu-Yi

Abstract

AbstractRecently, the worldwide pulsar timing array(PTA) collaborations, such as the Chinese Pulsar Timing Array (CPTA), the European PulsarTiming Array (EPTA), the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) and the Parkers Pulsar Timing Array (PPTA) published the analysis of PTA data, which is consistent with the Hellings–Downs curve, thus provides evidence for the existence of stochastic gravitational wave backgrounds (SGWB). In this paper, we will show that such SGWB signal observed by PTA can be explained by the gravitational waves (GWs) induced from double-inflection-point inflationary model in the framework of supergravity with a single chiral superfield. In this model, one of the inflection points leads to a large peak in the scalar power spectrum at small scales, and when this peak re-enters the horizon, it will induce GWs with the frequencies around nanohertz. In addition, we show that the high-density regions corresponding to the peak can collapse into planet-mass primordial black holes (PBHs), thus act as a component of dark matter (DM).

Funder

the Natural Science Foundation of Hebei Province

Department of Education of Liaoning Province

National Natural Science Foundation of China

Natural Science Basic Research Program of Shaanxi Province

Publisher

Springer Science and Business Media LLC

Reference71 articles.

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1. Development of generic no-scale inflation;Journal of Cosmology and Astroparticle Physics;2024-07-01

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