Probing the Presence of a Single or Binary Black Hole in the Globular Cluster Ngc 6752 with Pulsar Dynamics

The five millisecond pulsars that inhabit NGC 6752 display locations or accelerations that are quite unusual compared to all other pulsars known in globular clusters. In particular PSR-A, a binary pulsar, lives in the cluster halo, while PSR-B and PSR-E, located in the core, show remarkably high negative spin derivatives. This is suggestive that some uncommon dynamical process is at play in the cluster core that we attribute to the presence of a massive perturber. We here investigate whether a single intermediate-mass black hole, lying on the extrapolation of the mass MBH versus σ relation observed in galaxy spheroids, or a less massive binary black hole could play the requested role. To this purpose we simulated binary-binary encounters involving PSR-A, its companion star, and the black hole(s). A “stellar-mass binary” black hole of (50M⊙, 10M⊙) can imprint the right thrust to propel PSR-A in the halo during a flyby. The flyby is gentle and does not alter the internal properties of the binary pulsar. An “intermediate-mass binary” black hole of (200M⊙, 10M⊙) tends to impart a recoil speed larger than the escape speed: It can release PSR-A on the right orbit if its separation is wide. A “single intermediatemass” black hole of mass MBH ∼ 500M⊙ may have ejected PSR-A at the periphery of NGC 6752 in a close dynamical encounter involving the binary pulsar, the black hole and a star belonging to its cusp. The encounter gives correct speeds but alters significantly the eccentricity of the impinging binary, so that it must occur before the neutron star of PSR-A is recycled via accretion torques. The influence of an intermediate-mass binary black hole on the acceleration of the two core pulsars is studied, and the ejection of stars by the binary is shortly explored. In inspecting our close 4-body encounters, we have found that a single or binary black hole may attract on a long-term stable orbit a millisecond pulsar. Timing measurements on the captured “satellite” pulsar, either member of a hierarchical triple or of the cusp, could unambiguously unveil the presence of a black hole(s) in the core of a globular cluster. Subject headings: stars: neutron stars: black hole pulsars: general stars: globular clusters