We describe the isolation and spectroscopic characterization of the heavier phosphorus-containing analogue of isocyanic acid (HPCO), and its isotopologue (DPCO). This fundamental small molecule,which has been postulated to exist in interstellar space,has thus far only been observed at low gas phase concentrations or in inert gas matrices.Inthis report we describe its synthesis,spectroscopic properties,and reactivity in solution.
In1830,WçhlerandLiebiginvestigatedcyanicacid(HOCN)and its reactivity towards ammonia in an effort to synthesize ammonium cyanate,w hich was found to afford urea on mild heating.[1] Given the technological limitations at the time, very little was deduced about the constitution of the species studied. However these discoveries were fundamental in defining the concept of isomerism, for example,t he authors discovered that the silver salts of cyanate and fulminate have the same composition. Historic interest in such simple acids has largely focused on fulminic acid (and salts of its conjugate base) in large part due to its explosive properties. [2,3] The molecular structures of isocyanic (HNCO) and fulminic acid (HCNO), were not determined until 1950 by Herzberg and Reid, [4] and 1966 by Beck, respectively.[5] Nowadays,spectroscopic evidence for all four isomeric species isocyanic acid, [6] cyanic acid, [7] fulminic acid, [5] and isofulminic acid is available (Scheme 1).[8] HNCO, [9] HOCN, [10] and HCNO have even been detected in interstellar space. [11] In contrast, analytical data for the heavier phosphoruscontaining homologues HPCO are scarce.Several reports by Matveev claim to have synthesized HOCP from phosphaalkyne precursors, [12,13] however these studies were found to not be reproducible by the group of Becker and others. [14] Becker and co-workers suggested the existence of HOCP after protonation of the 2-phosphaethynolate anion, PCO À , [14,15] but clearly emphasized that this hypothesis was doubtful because the compound could neither be isolated nor further characterized. [16] Numerous theoretical studies have focused on the different isomers of the HPCO system, predicting HPCO to be 23 kcal mol À1 more stable than HOCP,w ith an activation barrier for interconversion of 70 kcal mol À1 . [17][18][19][20][21][22] These computational studies have stimulated further research, indicating that HPCO might be stable in interstellar space.All successful experimental HPCO studies thus far have tried to mimic interstellar conditions,such as low gas-phase concentration of HPCO or the use of noble gas matrices.T hus,t here are two studies of the generation of HPCO by gas discharges of highly dilute PH 3 /CO mixtures (in He or Ar), which allowed the recording of infrared [23] and microwave spectra of HPCO. [24,25] These studies have corroborated the presence of HPCO and not the isomeric HOCP.M ore recently,H PCO has been proposed as an intermediate in the formation of phosphinecarboxamides and phosphinidene-carbene adducts in the reaction of PCO À with ammonium and imidazolium salts, ...