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

Published 15 May 2014 in astro-ph.SR and gr-qc | (1405.3838v2)

Abstract: 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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