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Searching for cosmic string induced stochastic gravitational wave background with the Parkes Pulsar Timing Array

Ligong Bian^1,2,*, Jing Shu ^{3,2,4,5,6,7,†}, Bo Wang⁷, Qiang Yuan^8,9,‡, and Junchao Zong^10,4

¹Department of Physics and Chongqing Key Laboratory for Strongly Coupled Physics, Chongqing University, Chongqing 401331, China
²Center for High Energy Physics, Peking University, Beijing 100871, China
³School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China
⁴CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China
⁵School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
⁶School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China
⁷International Centre for Theoretical Physics Asia-Pacific, University of Chinese Academy of Sciences, 100190 Beijing, China
⁸Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China
⁹School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China
¹⁰Department of Physics, Nanjing University, Nanjing 210093, China

^*lgbycl@cqu.edu.cn
^†jshu@pku.edu.cn
^‡yuanq@pmo.ac.cn

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Articles Citing

Searching for cosmic string induced stochastic gravitational wave background with the Parkes Pulsar Timing Array

Gravitational wave standard sirens: A brief review of cosmological parameter estimation

Testing the Nambu–Goto approximation of cosmic string by lattice field theory simulations

Imprint of domain wall annihilation on induced gravitational waves

From U(1)×U(1) symmetry breaking to Majoron cosmology: Insights from NANOGrav 15-year data

Searching for anisotropy in the gravitational wave background using the Parkes Pulsar Timing Array

Fundamental physics and cosmology with TianQin

Quantitative analysis of the gravitational wave spectrum sourced from a first-order chiral phase transition of QCD

Fermion-antifermion pairs in magnetized spacetime generated by a point source

Prospects for constraining interacting dark energy cosmology with gravitational-wave bright sirens detected by future FAST/SKA-era pulsar timing arrays

Cosmic simulations of axion: probing dark matter and gravitational waves

Scalar and spinor fields in gravitating cosmic string spacetimes

Imprints of an early matter-dominated era arising from dark matter dilution mechanism on cosmic string dynamics and gravitational wave signatures*

Exact solution of the Pauli equation in the presence of a magnetic field in a spinning cosmic string spacetime

Domain wall network: A dual solution for gravitational waves and Hubble tension?

Footprints of axion-like particle in pulsar timing array data and James Webb Space Telescope observations

Cosmological interpretation for the stochastic signal in pulsar timing arrays

Can Supercooled Phase Transitions Explain the Gravitational Wave Background Observed by Pulsar Timing Arrays?

Stochastic gravitational wave background detection using NANOGrav 15-year data set in the context of massive gravity

Cosmological scaling of precursor domain walls

Quantum gravity effects on dark matter and gravitational waves

From quantum gravity to gravitational waves through cosmic strings

Primordial magnetic field as a common solution of nanohertz gravitational waves and the Hubble tension

Gravitational wave sources for pulsar timing arrays

Prospects for Taiji to detect a gravitational-wave background from cosmic strings

Dynamical simulations of colliding superconducting strings

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