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Isomer depletion as experimental evidence of nuclear excitation by electron capture
Author(s) -
C. J. Chiara,
J. J. Carroll,
M. P. Carpenter,
J. P. Greene,
D. J. Hartley,
R. V. F. Janssens,
G. J. Lane,
J. C. D. Marsh,
D. A. Matters,
M. Polasik,
J. Rzadkiewicz,
D. Seweryniak,
S. Zhu,
S. Bottoni,
A. B. Hayes,
S. A. Karamian
Publication year - 2018
Publication title -
nature
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 15.993
H-Index - 1226
eISSN - 1476-4687
pISSN - 0028-0836
DOI - 10.1038/nature25483
Subject(s) - atomic physics , excited state , electron capture , electron , kinetic energy , excitation , physics , isotope , atom (system on chip) , atomic nucleus , chemistry , nuclear physics , quantum mechanics , computer science , embedded system
The atomic nucleus and its electrons are often thought of as independent systems that are held together in the atom by their mutual attraction. Their interaction, however, leads to other important effects, such as providing an additional decay mode for excited nuclear states, whereby the nucleus releases energy by ejecting an atomic electron instead of by emitting a γ-ray. This 'internal conversion' has been known for about a hundred years and can be used to study nuclei and their interaction with their electrons. In the inverse process-nuclear excitation by electron capture (NEEC)-a free electron is captured into an atomic vacancy and can excite the nucleus to a higher-energy state, provided that the kinetic energy of the free electron plus the magnitude of its binding energy once captured matches the nuclear energy difference between the two states. NEEC was predicted in 1976 and has not hitherto been observed. Here we report evidence of NEEC in molybdenum-93 and determine the probability and cross-section for the process in a beam-based experimental scenario. Our results provide a standard for the assessment of theoretical models relevant to NEEC, which predict cross-sections that span many orders of magnitude. The greatest practical effect of the NEEC process may be on the survival of nuclei in stellar environments, in which it could excite isomers (that is, long-lived nuclear states) to shorter-lived states. Such excitations may reduce the abundance of the isotope after its production. This is an example of 'isomer depletion', which has been investigated previously through other reactions, but is used here to obtain evidence for NEEC.

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