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arxiv: 1405.3838 · v2 · pith:3FMTD6QR · submitted 2014-05-15 · astro-ph.SR · gr-qc

In what sense a neutron star-black hole binary is the holy grail for testing gravity?

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classification astro-ph.SR gr-qc
keywords neutronbinaryholesensestar-blacksystemswhatapply
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Pulsars in binary systems have been very successful to test the validity of general relativity in the strong field regime. So far, such binaries include neutron star-white dwarf (NS-WD) and neutron star-neutron star (NS-NS) systems. It is commonly believed that a neutron star-black hole (NS-BH) binary will be much superior for this purpose. But in what sense is this true? Does it apply to all possible deviations?

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Cited by 1 Pith paper

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