Now that the mass of the central black hole in the galaxy M87 has been measured with great precision using different methods , the remaining parameter of the Kerr metric that needs to be estimated is the spin a _ { * } .
We have modeled measurements of the average power of the relativistic jet and an upper limit to the mass accretion rate onto the black hole with general relativistic magnetohydrodynamic models of jet formation .
This allows us to derive constraints on a _ { * } and the black hole magnetic flux \phi .
We find a lower limit on M87* ’ s spin and magnetic flux of |a _ { * } | \geq 0.4 and \phi \gtrsim 6 in the prograde case , and |a _ { * } | \geq 0.5 and \phi \gtrsim 10 in the retrograde case , otherwise the black hole is not able to provide enough energy to power the observed jet .
These results indicate that M87* has a moderate spin at minimum and disfavor a variety of models typified by low values of \phi known as “ SANE ” , indicating that M87* prefers the magnetically arrested disk state .
We discuss how different estimates of the jet power and accretion rate can impact a _ { * } and \phi .