2010
DOI: 10.1016/j.cplett.2010.02.022
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Kinetic study on the photoabsorption process of gaseous O2 dimol at 630 nm in a wide pressure range

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Cited by 9 publications
(8 citation statements)
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“…Basically it is the dimol counterpart of the 1270 nm monomol transition (two 1270 nm photons have the same energy as one 633 nm photon), with an energy of 1.96 eV. This transition has been employed to assess physical and/or chemical parameters, mainly in high pressure oxygen although there are studies in organic solvents too [99], [101], [123], [173], [174], [175], [176].…”
Section: Direct Optical Excitation Of 1o2mentioning
confidence: 99%
“…Basically it is the dimol counterpart of the 1270 nm monomol transition (two 1270 nm photons have the same energy as one 633 nm photon), with an energy of 1.96 eV. This transition has been employed to assess physical and/or chemical parameters, mainly in high pressure oxygen although there are studies in organic solvents too [99], [101], [123], [173], [174], [175], [176].…”
Section: Direct Optical Excitation Of 1o2mentioning
confidence: 99%
“…We term such a band a twomolecule combination band, which is also known in the literature as a "dimol absorption band," dimol meaning "two-molecule." For example, see Ida et al (2010) and Tajti et al (2017). Previous identifications of twomolecule combination bands in spectra of ice samples include single photons exciting the fundamental mode of adjacent N 2 molecules (Grundy et al 1993) and adjacent N 2 and O 2 molecules (Minenko & Jodl 2006) as well as single photons exciting an electronic tran-…”
Section: Introductionmentioning
confidence: 99%
“…According to [22], the concentration of O 2 (a):O 2 (a) pairs of two free molecules in which radiative transition (4) is possible is n aa = K(n a ) 2 , where K ≈ 1.47 × 10 -22 cm 3 at a temperature of about 300 K. Assume that the concentration of O 2 (a):O 2 (X) complexes consisting of two free molecules in which radiative process (2) is possible can also be determined as n aX = Kn X n a with the same value of the constant K. Then, for the radiative transition O 2 (a):O 2 (X) → O 2 (X):O 2 (X) + hν (1268 nm), which corresponds to CIE (2), the Einstein coefficient will be A aX = k С n a n X /n aX = k С /K ≈ 850A a ≈ 0.19 s -1 at A a = 2.19 × 10 -4 s -1 .…”
Section: Resultsmentioning
confidence: 99%