The newly observed state Ds0(2590)

We choose the Reduction Formula, PCAC and Low Energy Theory to reduce the S matrix of a OZI allowed two-body strong decay involving a light pseudoscalar, the covariant transition amplitude formula with relativistic wave functions as input is derived. After confirm this method by the decay D ∗ ( 2010 ) → D π , we study the newly observed D s 0 ( 2590 ) + with supposing it to be the state D s ( 2 1 S 0 ) + , we find its decay width Γ is highly sensitive to the D s 0 ( 2590 ) + mass, which result in the meaningless comparison of widths by different models with various input masses. Instead of width, we studied the overlap integral over the wave functions of initial and final states, here we parameterized it as X which is model-independent, and the ratio Γ / | P f | 3 , both are almost mass independent, to give us useful information. The results show that, all the existing theoretical predictions X D s ( 2 S ) → D ∗ K = 0.25 ∼ 0.41 and Γ / | P f | 3 = 0.81 ∼ 1.77 MeV - 2 are smaller than experimental data 0 . 585 - 0.035 + 0.015 and 4 . 54 - 0.52 + 0.25 MeV - 2 . Further compared with X D ∗ ( 2010 ) → D π ex = 0.540 ± 0.009 , the current data X D s ( 2 S ) → D ∗ K ex = 0 . 585 - 0.035 + 0.015 is too big to be an reasonable value, so it is early to say D s 0 ( 2590 ) + is the conventional D s ( 2 1 S 0 ) + meson.