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We explore the suggestion that the neutron lifetime puzzle might be resolved by neutrons decaying into dark matter through the process, n \rightarrow \chi\chi\chi, with \chi having a mass one third of that of the neutron.
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2013
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2016
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2016
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2019
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2020
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2020
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2020
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K. M. L. Martinez, A. W. Thomas, P. A. M. Guichon, and J. R. Stone, “Tensor and pairing interactions within the quark-meson coupling energy-density functional,” Phys. Rev. C
2020
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2021
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2021
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2021
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W. Husain and A. W. Thomas, “Hybrid Stars with Hyperons and Strange Quark Matter,” AIP Conf. Proc
2021
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T. F. Motta, P. A. M. Guichon, and A. W. Thomas, “On the sound speed in hyperonic stars,” Nucl. Phys. A
2021
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T. E. Riley et al
2021
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W. Husain and A. W. Thomas, “Possible nature of dark matter,” Journal of Cosmology and Astroparticle Physics
2021
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2021
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A. Strumia, “Dark matter interpretation of the neutron decay anomaly,” Journal of High Energy Physics
2022
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T. F. Motta and A. W. Thomas, “The role of baryon structure in neutron stars,” Mod. Phys. Lett. A
2022
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Y. Yamamoto, N. Yasutake, and T. A. Rijken, “Quark-quark interaction and quark matter in neutron stars,” Physical Review C
2022
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J. M. Berryman, S. Gardner, and M. Zakeri, “Neutron stars with baryon number violation, probing dark sectors,” 2022
2022
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D. Rafiei Karkevandi, S. Shakeri, V. Sagun, and O. Ivanytskyi, “Bosonic dark matter in neutron stars and its effect on gravitational wave signal,” Phys. Rev. D
2022
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W. Husain, T. F. Motta, and A. W. Thomas, “Consequences of neutron decay inside neutron stars,” 3 2022
2022
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