Authors: Sylwester Kornowski
B. Kiziltan et al. (9 February 2017) showed that pulsars in 47 Tuc imply a central black hole (BH) with a mass of about 2,200 solar masses (the upper limit is 3,700 solar masses whereas the lower limit is 1,400). Predictive power correlates with number of observed pulsars. The inference flattens with decreasing number of randomly selected pulsars. Here, applying the Scale-Symmetric Theory (SST), we suggest that the BH consists of 16 neutron black holes (NBH) entangled with 16 pulsars. With time, the set of 16 pulsars changes its constituents. SST shows that then mass of the central BH should be 2,536 solar masses. To such mass lead as well the observational data for 16 randomly selected pulsars. More precise observational data should show whether predicted within SST the exact mass of the central BH is correct.
Comments: 2 Pages.
[v1] 2017-02-14 09:21:47
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