“…(See also already [130,131] where a first start was made to treat the phase noise problem in the time-domain.) In [46,49] it is argued that, in first order, (20.37) has a solution of the form y(t) + z(t), with α determined by (20.42), and where the orbital deviation z(t) satisfies ||z|| ∞ < Const.||b|| ∞ (and even z(t) → 0 (t → ∞)).…”