Terahertz-visible two-photon rotational spectroscopy of cold OD-
arXiv:1602.08303 · doi:10.1103/PhysRevA.93.032513
Abstract
We present a method to measure rotational transitions of molecular anions in the terahertz domain by sequential two-photon absorption. Ion excitation by bound-bound terahertz absorption is probed by absorption in the visible on a bound-free transition. The visible frequency is tuned to a state-selective photodetachment transition of the excited anions. This provides a terahertz action spectrum for just few hundred molecular ions. To demonstrate this we measure the two lowest rotational transitions, J=1<-0 and J =2<-1 of OD- anions in a cryogenic 22-pole trap. We obtain rotational transition frequencies of 598596.08(19) MHz for J=1<-0 and 1196791.57(27) MHz for J=2<-1 of OD-, in good agreement with their only previous measurement. This two-photon scheme opens up terahertz rovibrational spectroscopy for a range of molecular anions, in particular for polyatomic and cluster anions.
arXiv commentPhysical Review A (in press)
References in corpus (13)
- Astronomical identification of CN-, the smallest observed molecular anion
- Detection of C5N- and vibrationally excited C6H in IRC +10216
- Detection of a Noble Gas Molecular Ion, {36}ArH^+, in the Crab Nebula
- Interstellar OH+, H2O+ and H3O+ along the sight-line to G10.6-0.4
- Radiofrequency multipole traps: Tools for spectroscopy and dynamics of cold molecular ions
- Internal state thermometry of cold trapped molecular anions
- Chemical probing spectroscopy of H3+ above the barrier to linearity
- Herschel observations of the hydroxyl radical (OH) in young stellar objects
- Observation of a rotational transition in trapped and sympathetically cooled molecular ions
- Late Stages of Stellar Evolution - Herschel's contributions
- An observational investigation of the identity of B11244 (-CH/CH)
- Laboratory Measurement of the Pure Rotational Transitions of the HCNH+ and its Isotopic Species
- Upper limits to interstellar NH+ and para-NH2- abundances. Herschel-HIFI observations towards Sgr B2 (M) and G10.6-0.4 (W31C)