3 problems
Let be the quotient spacetime, future null infinity, and interpret “sub-extremal in the limit” as the limiting black-hole condition stated in the pa…
Consider smooth, spherically symmetric initial data with two asymptotically flat ends for the Einstein-Maxwell-scalar field equation, and suppose the data are globally close to Rei…
Consider the data and maximal development covered by the stability theorem for the two-ended Reissner–Nordström interior, and let the additional lower bounds on the scalar field al…