Reaction dynamics of P(S) O(X) O(P) PO(X) on a global CHIPR potential energy surface of PO(XA): implications for atmospheric …
G Chen, Z Qin, X Li, L Liu - Atmospheric Chemistry and Physics, 2023 - acp.copernicus.org
The reaction dynamics of P (4 S)+ O 2 (X 3 Σ g-)→ O (3 P)+ PO (X 2 Π) are thought to be
important in atmospheric and interstellar chemistry. Based on the state-of-the-art ab initio …
important in atmospheric and interstellar chemistry. Based on the state-of-the-art ab initio …
A Novel Abiotic Pathway for Phosphine Synthesis over Acidic Dust in Venus' Atmosphere
Recent ground-based observations of Venus have detected a single spectral feature
consistent with phosphine (PH3) in the middle atmosphere, a gas which has been …
consistent with phosphine (PH3) in the middle atmosphere, a gas which has been …
Reaction dynamics of P(4S) + O2(X ³Σ- ) → O(³ P) + PO(X²Π) on a global CHIPR potential energy surface of PO2(X 2 A1): implication for atmospheric modelling.
G Chen, Z Qin, X Li, L Liu - Atmospheric Chemistry & …, 2023 - search.ebscohost.com
Reaction dynamics of P (< sup> 4 S)+ O< sub> 2(X ³Σ-)→ O (³ P)+ PO (X²Π) is thought to be
important in atmospheric and interstellar chemistry. Based on the state-of-the-art ab initio …
important in atmospheric and interstellar chemistry. Based on the state-of-the-art ab initio …
Reaction dynamics of P(4S) + O2(X 3Σ-) → O(3P) + PO(X 2Π) on a global CHIPR potential energy surface of PO2(X 2A1): implication for atmospheric …
G Chen, Z Qin, X Li, L Liu - EGUsphere, 2023 - egusphere.copernicus.org
Reaction dynamics of P (4 S)+ O 2 (X 3 Σ-)→ O (3 P)+ PO (X 2 Π) is thought to be important
in atmospheric and interstellar chemistry. Based on the state-of-the-art ab initio energy …
in atmospheric and interstellar chemistry. Based on the state-of-the-art ab initio energy …