Abstract
Potential energy curves have been calculated for the low-lying electronic states of AgH, correlating to the 4d10 5s1 (2S), 4d10 5p1 (2Po), 4d9 5s2 (2D), and 4d10 6s1 (2S) states of atomic silver, using the MRCI method with scalar relativistic and spin–orbit corrections. Spectroscopic constants were obtained for 24 individual Ω states, and several excited states of AgH observed in the ultraviolet absorption spectra, i.e., the C1Π, B1Σ+, b3Δ1, and D1Π states, were relabeled based on the new ab initio data. The calculated Einstein A coefficients indicated that almost all electronic transitions with ΔΩ = 0, ±1 are allowed.
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