Abstract
Abstract
The data recently released by the North American Nanohertz Observatory for Gravitational
Waves (NANOGrav) provides compelling evidence supporting the existence of a stochastic signal that
aligns with a gravitational-wave background. We show that the scalar-induced gravitational waves
from the Higgs inflation model with the parametric amplification mechanism can explain this
signal. Such a gravitational-wave background naturally predicts the substantial existence of
planet-mass primordial black holes, which can be planet 9 in our solar system and the lensing
objects for the ultrashort-timescale microlensing events observed by the Optical Gravitational
Lensing Experiment. Therefore, the NANOGrav signal, the potential Planet 9 in our solar system,
and the Optical Gravitational Lensing Experiment can be explained within the framework of Higgs
inflation.
Reference183 articles.
1. Observation of Gravitational Waves from a Binary Black Hole Merger;LIGO Scientific, Virgo Collaboration;Phys. Rev. Lett.,2016
2. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral;LIGO Scientific, Virgo Collaboration;Phys. Rev. Lett.,2017
3. GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs;LIGO Scientific, Virgo Collaboration;Phys. Rev. X,2019
4. GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run;LIGO Scientific, Virgo Collaboration;Phys. Rev. X,2021
5. GWTC-2.1: Deep extended catalog of compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run;LIGO Scientific, VIRGO Collaboration;Phys. Rev. D,2024
Cited by
5 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献