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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…

高能物理 - 唯象学 · 物理学 2025-04-04 Akifumi Chitose , Masahiro Ibe , Shunsuke Neda , Satoshi Shirai

Metastable cosmic strings (MSCSs) are among the best-fitting explanations of the 2023 pulsar timing array (PTA) signal for gravitational waves at nanohertz frequencies. We propose the novel possibility that a network of MSCSs generating…

高能物理 - 唯象学 · 物理学 2025-08-20 Stefan Antusch , Kevin Hinze , Shaikh Saad

Pulsar timing arrays (PTA) are a promising probe to the cosmologically novel nanohertz gravitational wave (GW) regime through the stochastic GW background. In this work, we consider subluminal GW modes as a possible source of correlations…

广义相对论与量子宇宙学 · 物理学 2023-05-26 Reginald Christian Bernardo , Kin-Wang Ng

We perform a phenomenological comparison of the gravitational wave (GW) spectrum expected from cosmic gauge string networks and superstring networks comprised of multiple string types. We show how violations of scaling behavior and the…

高能物理 - 唯象学 · 物理学 2024-07-25 Danny Marfatia , Ye-Ling Zhou

The pulsar timing array (PTA) collaborations have recently suggested the presence of a gravitational wave background at nano-Hertz frequencies. In this paper, we explore potential inflationary interpretation of this signal within the…

宇宙学与河外天体物理 · 物理学 2023-11-14 Chengjie Fu , Jing Liu , Xing-Yu Yang , Wang-Wei Yu , Yawen Zhang

Recent observations by pulsar timing arrays (PTAs) such as NANOGrav, EPTA, PPTA, and CPTA suggest the presence of nanohertz stochastic gravitational wave background (GWB). While such signals could be explained by gravitational waves from a…

宇宙学与河外天体物理 · 物理学 2025-01-31 Yifan Hu , Kohei Kamada

The observations from pulsar timing arrays (PTAs), led by the North American Nanohertz Observatory for Gravitational Waves (NANOGrav), have provided opportunities to constrain primordial gravitational waves at low frequencies. In this…

宇宙学与河外天体物理 · 物理学 2025-05-07 Lu Yin

We construct a realistic supersymmetric model for superheavy metastable cosmic strings (CSs) that can be investigated in the current pulsar timing array (PTA) experiments. It is based on shifted $\mu$-hybrid inflation in which the symmetry…

高能物理 - 唯象学 · 物理学 2025-10-28 Adeela Afzal , Maria Mehmood , Mansoor Ur Rehman , Qaisar Shafi

Pulsar timing arrays (PTAs) have recently provided compelling evidence for a stochastic gravitational wave background (SGWB) in the nanohertz frequency band, offering a unique window into fundamental physics. Here, we explore implications…

宇宙学与河外天体物理 · 物理学 2026-02-10 Mohammadreza Davari , Alireza Allahyari

We consider the sensitivity of the pulsar timing array (PTA) technique to specific kind of narrow-band stochastic signals in nano-Hz frequency range. Specifically, we examine the narrow-band signal produced by oscillating gravitational…

天体物理仪器与方法 · 物理学 2014-11-04 Konstantin A. Postnov , Nataliya K. Porayko

We estimate the stochastic gravitational wave spectrum emitted from a network of cosmic strings in which the latter are effectively stable against breaking by monopole pair creation. The monopoles are produced at a higher scale from an…

高能物理 - 唯象学 · 物理学 2022-08-24 George Lazarides , Rinku Maji , Qaisar Shafi

The recently released data by pulsar timing array (PTA) collaborations present strong evidence for a stochastic signal consistent with a gravitational-wave background. Assuming this signal originates from scalar-induced gravitational waves,…

宇宙学与河外天体物理 · 物理学 2025-03-27 Lang Liu , Zu-Cheng Chen , Qing-Guo Huang

The existence of a stochastic gravitational wave background is indicated by the recent pulsar timing array (PTA) experiments. We study the enhanced production of second-order gravitational waves from the scalar perturbations when the…

宇宙学与河外天体物理 · 物理学 2024-01-26 Masahiro Kawasaki , Kai Murai

We analyse the gravitational wave and low energy signatures of a Pati-Salam phase transition. For a Pati-Salam scale of $M_{PS} \sim 10^5$ GeV, we find a stochastic power spectrum within reach of the next generation of ground-based…

高能物理 - 唯象学 · 物理学 2019-02-21 Djuna Croon , Tomás E. Gonzalo , Graham White

In a recent paper (see https://doi.org/10.1103/PhysRevD.108.095053), we have demonstrated that the 2023 PTA results, which hint at a stochastic gravitational wave (GW) background at nanohertz frequencies, point towards a promising…

高能物理 - 唯象学 · 物理学 2024-09-18 Stefan Antusch , Kevin Hinze , Shaikh Saad

A realistic model of $SU(5) \times U(1)_{\chi}$, embedded in $SO(10)$ supersymmetric grand unified theory, is investigated for the emergence of a metastable cosmic string network. This network eventually decays via the Schwinger production…

高能物理 - 唯象学 · 物理学 2024-04-02 Waqas Ahmed , Mansoor Ur Rehman , Umer Zubair

Several pulsar-timing array (PTA) collaborations are finding tantalising hints for a stochastic gravitational wave background signal in the nano-Hertz regime. So far, though, no convincing evidence for the expected Hellings-Downs…

广义相对论与量子宇宙学 · 物理学 2022-04-20 Gianmassimo Tasinato

We have begun an exciting era for gravitational wave detection, as several world-leading experiments are breaching the threshold of anticipated signal strengths. Pulsar timing arrays (PTAs) are pan-Galactic gravitational wave detectors that…

天体物理仪器与方法 · 物理学 2015-11-26 Sarah Burke-Spolaor

Pulsar timing arrays (PTAs) are designed to detect nanohertz-frequency gravitational waves (GWs). Since GWs are anticipated from cosmic strings, PTAs offer a viable approach to testing their existence. We present the results of the first…

Metastable cosmic strings are a common prediction of grand unified theories and act as a source of a gravitational-wave background (GWB) that can explain the 2023 pulsar timing array (PTA) signal. In this paper, we revisit the GWB signal…

高能物理 - 唯象学 · 物理学 2026-05-01 Doa Hashemi Asl , Kai Schmitz
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