Hydrogen
interstitials are expected to be important in organic–inorganic
hybrid perovskites; however, the characteristics and behaviors of
hydrogen in perovskites remain poorly understood. Here, on the basis
of density functional theory calculations, we quantitatively reported
that both atomic and molecular hydrogen interstitials can form in
hybrid MAPbI3 and MASnI3 perovskites. Whereas
molecular hydrogen interstitial, H2, is chemically inert,
atomic hydrogen interstitial, H
i
, serves
as an electrically active negative-U defect. We identify
high-density H
i
+ as a significant origin of ionic conductivity
in p-type MAPbI3 under the hydrogen-rich conditions, with
the calculated activation energy being comparable to that measured
in experiments. The highly diffusive H
i
+ ions are expected
to impact hysteresis, charge separation, device polarization, and
photogenerated field-screening effect and consequently degrade the
solar cell performance. We evaluated approaches for mitigating such
detrimental effects and suggested that synthesizing the perovskites
with slightly extra iodine addition or tin alloying can effectively
suppress the concentration of H
i
+. Our results are important to
understand the fundamental aspects of hydrogen in perovskites in general
and offer valuable insight for further improving the performance of
perovskite solar cells and other optoelectronic devices via defect
engineering.