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Neutron stars are ideal astrophysical sources to probe general relativity due to their large compactnesses and strong gravitational fields.
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F. M. Ramazanoğlu, “Spontaneous tensorization from curvature coupling and beyond,” Phys. Rev. D99
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B. P. Abbott et al. (Virgo, LIGO Scientific), “GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral,” Phys. Rev. Lett. 119
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B. Z. Foster, “Strong field effects on binary systems in Einstein-aether theory,” Phys. Rev. D76
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F. M. Ramazanoğlu, “Spontaneous growth of vector fields in gravity,” Phys. Rev. D96
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B. P. Abbott et al. (LIGO Scientific, Virgo), “GW170817: Measurements of neutron star radii and equation of state,” Phys. Rev. Lett. 121
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F. M. Ramazanoğlu, “Spontaneous growth of spinor fields in gravity,” Phys. Rev. D98
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