Gravitational waves from cosmic strings after a first-order phase transition * *This work is supported in part by the National Key Research and Development Program of China (2021YFC2203004), in part by the National Natural Science Foundation of China (12075041, 12047564), and the Fundamental Research Funds for the Central Universities of China (2021CDJQY-011, 2020CDJQY-Z003), and Chongqing Natural Science Foundation (cstc2020jcyj-msxmX0814)

Ruiyu Zhou,Ligong Bian

doi:10.1088/1674-1137/ac424c

Gravitational waves from cosmic strings after a first-order phase transition * *This work is supported in part by the National Key Research and Development Program of China (2021YFC2203004), in part by the National Natural Science Foundation of China (12075041, 12047564), and the Fundamental Research Funds for the Central Universities of China (2021CDJQY-011, 2020CDJQY-Z003), and Chongqing Natural Science Foundation (cstc2020jcyj-msxmX0814)

Ruiyu Zhou, Ligong Bian

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Journal: Chinese Physics C	Publication Date: Mar 1, 2022
Citations: 5	License type: cc-by

Affiliation: Chongqing University, Chongqing University of Posts and Telecommunications

#Natural Science Foundation Of China #Cosmic Strings #First-order Phase Transition #National Key Research #Space-based Interferometers #Natural Science Foundation #Phase Transition #Phase Transition Temperature #Key Research Program #Gravitational Waves

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We study the possibility of probing high scale phase transitions that are inaccessible by LIGO. Our study shows that the stochastic gravitational-wave radiation from cosmic strings that are formed after the first-order phase transition can be detected by space-based interferometers when the phase transition temperature is GeV.

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