Gravitational waves from type II axion-like curvaton model and its implication for NANOGrav result

DOI10.1088/1475-7516/2021/05/023zbMath1485.83079arXiv2101.11244OpenAlexW3160145097MaRDI QIDQ5028118

Hiromasa Nakatsuka, Masahiro Kawasaki

Publication date: 8 February 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2101.11244

zbMATH Keywords

primordial black holesphysics of the early universeaxionsgravitational waves/sources

Mathematics Subject Classification ID

Other elementary particle theory in quantum theory (81V25) Black holes (83C57) Applications of stochastic analysis (to PDEs, etc.) (60H30) Perturbations in context of PDEs (35B20) Gravitational waves (83C35)

Related Items (2)

Non-gaussianities for primordial black hole formation ⋮ NANOGrav signal and LIGO-Virgo primordial black holes from the Higgs field

Cites Work

• Probing the scale of grand unification with gravitational waves
• Gravitational waves from binary supermassive black holes missing in pulsar observations
• Gravitational-Wave Constraints on the Abundance of Primordial Black Holes
• Primordial black holes—perspectives in gravitational wave astronomy
• Probing primordial features with the stochastic gravitational wave background
• Generating PBHs and small-scale GWs in two-field models of inflation

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