Gravitational Waves from Metastable Cosmic Strings in Supersymmetric New Inflation Model
Akifumi Chitose, Masahiro Ibe, Shunsuke Neda, Satoshi Shirai

TL;DR
This paper introduces a supersymmetric inflation model with metastable cosmic strings that can produce gravitational waves matching PTA observations, while also addressing gravitino production, leptogenesis, and dark matter.
Contribution
It proposes a novel two-step symmetry breaking supersymmetric model with metastable cosmic strings, predicting detectable gravitational wave signatures consistent with PTA data.
Findings
Predicts string tension $G_N u_{str} \u2248 10^{-5}$ compatible with PTA data.
Requires low reheating temperature to suppress gravitino production.
Provides a framework compatible with non-thermal leptogenesis and supersymmetric dark matter.
Abstract
Recent observations by pulsar timing arrays (PTAs) indicate a potential detection of a stochastic gravitational wave (GW) background. Metastable cosmic strings have been recognized as a possible source of the observed signals. In this paper, we propose an -invariant supersymmetric new inflation model. It is characterized by a two-step symmetry breaking , incorporating metastable cosmic strings. The field responsible for the initial symmetry breaking acts as the inflaton, while the second symmetry breaking occurs post-inflation, ensuring the formation of the cosmic string network without monopole production. Our model predicts symmetry breaking scales consistent with the string tensions favored by PTA data, , where is the Newton constant. Notably, a low reheating…
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
