TY - JOUR
T1 - Unique Applications of para-Hydrogen Matrix Isolation to Spectroscopy and Astrochemistry
AU - Weber, Isabelle
AU - Joshi, Prasad Ramesh
AU - Anderson, David T.
AU - Lee, Yuan Pern
N1 - Publisher Copyright:
© 2024 The Authors. Published by American Chemical Society.
PY - 2024/11/14
Y1 - 2024/11/14
N2 - Cryogenic solid para-hydrogen (p-H2) exhibits pronounced quantum effects, enabling unique experiments that are typically not possible in noble-gas matrices. The diminished cage effect facilitates the production of free radicals via in situ photolysis or photoinduced reactions. Electron bombardment during deposition readily produces protonated and hydrogenated species, such as polycyclic aromatic hydrocarbons, that are important in astrochemistry. In addition, quantum diffusion delocalizes hydrogen atoms in solid p-H2, allowing efficient H atom reactions with astrochemical species and introducing new concepts in astrochemical models. Some H atom reactions display anomalous temperature behaviors, highlighting the rich chemistry in p-H2. The investigation on quantum diffusion of heavier atoms and molecules is also important for our understanding of the chemistry in interstellar ice. Additionally, matrix shifts of electronic transitions of polycyclic aromatic hydrocarbons in p-H2 are less divergent than those in solid Ne such that systematic measurements in p-H2 might help in the assignment of diffuse interstellar bands.
AB - Cryogenic solid para-hydrogen (p-H2) exhibits pronounced quantum effects, enabling unique experiments that are typically not possible in noble-gas matrices. The diminished cage effect facilitates the production of free radicals via in situ photolysis or photoinduced reactions. Electron bombardment during deposition readily produces protonated and hydrogenated species, such as polycyclic aromatic hydrocarbons, that are important in astrochemistry. In addition, quantum diffusion delocalizes hydrogen atoms in solid p-H2, allowing efficient H atom reactions with astrochemical species and introducing new concepts in astrochemical models. Some H atom reactions display anomalous temperature behaviors, highlighting the rich chemistry in p-H2. The investigation on quantum diffusion of heavier atoms and molecules is also important for our understanding of the chemistry in interstellar ice. Additionally, matrix shifts of electronic transitions of polycyclic aromatic hydrocarbons in p-H2 are less divergent than those in solid Ne such that systematic measurements in p-H2 might help in the assignment of diffuse interstellar bands.
UR - http://www.scopus.com/inward/record.url?scp=85208696781&partnerID=8YFLogxK
U2 - 10.1021/acs.jpclett.4c02733
DO - 10.1021/acs.jpclett.4c02733
M3 - Review article
C2 - 39503286
AN - SCOPUS:85208696781
SN - 1948-7185
VL - 15
SP - 11361
EP - 11373
JO - Journal of Physical Chemistry Letters
JF - Journal of Physical Chemistry Letters
IS - 45
ER -