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In this paper, we analyse sound waves arising from a cosmic phase transition where the full velocity profile is taken into account as an explanation for the gravitational wave spectrum observed by multiple pulsar timing array groups.
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P.-H. Gu, E. Ma, and U. Sarkar, “Pseudo-Majoron as Dark Matter,” Phys. Lett. B
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X. Siemens, V. Mandic, and J. Creighton, “Gravitational wave stochastic background from cosmic (super)strings,” Phys. Rev. Lett
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Y. Bai and M. Korwar, “Cosmological constraints on first-order phase transitions,” Phys. Rev. D
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