Molecular inversion
The umbrella motion of NH₃ and related molecules, reduced to a 1D double well: the central atom crosses the plane of the three hydrogens through the planar form (the barrier). Each level splits into a tunnelling doublet — the transition of the ammonia maser (0.79 cm⁻¹). Effective coordinate solved by finite differences in the Python backend (via gw2py).It is literally the abstract double well rendered in a real molecule: tunnelling through the planar configuration opens the parity doublet. Same physics as the doublet of pear-shaped nuclei.
A pyramidal molecule can flip like an umbrella in the wind, passing through the planar form.
A single coordinate
The inversion motion of NH₃ is dominated by one large-amplitude coordinate: the central atom crossing the plane of the three hydrogens. Along it the potential is a symmetric double well: two minima (the two mirror pyramids) separated by a barrier (the planar configuration).
\[ -B\,\frac{d^2\psi}{dq^2} + V(q)\,\psi = E\,\psi,\qquad V(q)=V_b\Big[(q/q_0)^2-1\Big]^2. \]The tunnelling doublet
Each level splits into a pair (symmetric / antisymmetric) by tunnelling through the barrier. The ground-state doublet of NH₃ is at 0.79 cm⁻¹ (23.87 GHz): it is the transition of the ammonia maser, the first maser (1954).
The thread
It is the double well rendered in a real molecule — and the same physics as the parity doublet of pear-shaped nuclei.
Molecule
State to represent
Why it works
Isotope effect and barrier
Tunnelling depends exponentially on \(\sqrt{\mu V_b}\): ND₃ (larger mass) has a much smaller doublet than NH₃; PH₃ and AsH₃, with much higher barriers, do not invert on observable timescales. The same formula explains why tetrahedral carbon does not racemize spontaneously.
What is missing (honesty)
We neglect the coupling with the other modes and the coordinate dependence of the reduced mass (\(G(q)\)); the parameters are adopted. An accurate computation uses an ab initio potential energy surface and a multidimensional vibrational Hamiltonian (backend).
References
- C. H. Townes, A. L. Schawlow, Microwave Spectroscopy, McGraw-Hill, 1955.
- J. D. Swalen, J. A. Ibers, «Potential Function for the Inversion of Ammonia», J. Chem. Phys. 36, 1914 (1962). doi.
WebNIR · CNR-IFAC | demo interface — numerical work is provided by the Python backend (gw2py).
Keywords: inversion, ammonia, NH3, maser, double well, tunnelling, effective coordinate, isotope effect, spectroscopy