Trapped electrons produced in ethanol glass at 40K
Description
Optical absorption and ESR measurements were carried out on et− produced in ethanol at 4°K. The same et− yield for γ radiolysis at 4 and 77°K indicates that electrons are stabilized in pre-existing traps at 4°K where molecular dipoles remain unrelaxed. et− prior to solvation can be classified into two groups. One with λmax = 1500 nm, W1/2= 4 × 103 cm−1 and Δ Hpp = 5.5 ± 0.5 G is easily photobleached by the infrared light. The other with broad absorption band in the visible and Δ Hpp = 13.5 ± 1.5 G is not photobleached by the infrared light. The successive shift of the absorption spectrum to the higher energy side on warming is interpreted by the molecular reorientation mechanism. et− decay is observed during the solvation process, depending on time required for the solvation. The blue shift of the absorption spectrum on reducing the temperature is attributed to contraction of electron traps.
Additional details
Identifiers
- DOI
- 10.1063/1.1678355;
Publishing Information
- Journal Title
- The Journal of Chemical Physics
- Journal Volume
- 57
- Journal Issue
- 3
- Series
- J. Chem. Phys.
- Journal Page Range
- 1039-1045
- ISSN
- 0021-9606
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 4042521
- Subject category
- S38: RADIATION CHEMISTRY, RADIOCHEMISTRY AND NUCLEAR CHEMISTRY;
- Descriptors DEI
- ABSORPTION SPECTRA; ELECTRON SPIN RESONANCE; ETHANOL; GAMMA RADIATION; LOW TEMPERATURE; RADIOLYSIS; TRAPPED ELECTRONS
- Descriptors DEC
- ALCOHOLS; CHEMICAL RADIATION EFFECTS; CHEMICAL REACTIONS; DECOMPOSITION; ELECTROMAGNETIC RADIATION; ELECTRONS; ELEMENTARY PARTICLES; FERMIONS; HYDROXY COMPOUNDS; LEPTONS; MAGNETIC RESONANCE; ORGANIC COMPOUNDS; RADIATION EFFECTS; RADIATIONS; RESONANCE; SPECTRA
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent