Twenty
years ago two different polymorphs of carbonic acid, α-
and β-H2CO3, were isolated as thin, crystalline
films. They were characterized by infrared and, of late, by Raman
spectroscopy. Determination of the crystal structure of these two
polymorphs, using cryopowder and thin film X-ray diffraction techniques,
has failed so far. Recently, we succeeded in sublimating α-H2CO3 and trapping the vapor phase in a noble gas
matrix, which was analyzed by infrared spectroscopy. In the same way
we have now investigated the β-polymorph. Unlike α-H2CO3, β-H2CO3 was regarded
to decompose upon sublimation. Still, we have succeeded in isolation
of undecomposed carbonic acid in the matrix and recondensation after
removal of the matrix here. This possibility of sublimation and recondensation
cycles of β-H2CO3 adds a new aspect to
the chemistry of carbonic acid in astrophysical environments, especially
because there is a direct way of β-H2CO3 formation in space, but none for α-H2CO3. Assignments of the FTIR spectra of the isolated molecules unambiguously
reveal two different carbonic acid monomer conformers (C2v and Cs). In contrast to the earlier study on α-H2CO3, we do not find evidence for centrosymmetric
(C2h) carbonic acid dimers
here. This suggests that two monomers are entropically favored at
the sublimation temperature of 250 K for β-H2CO3, whereas they are not at the sublimation temperature of 210
K for α-H2CO3.