1985
DOI: 10.1002/prop.2190330102
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Beta Decay Far from Stability and Its Role in Nuclear Physics and Astrophysics

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Cited by 23 publications
(5 citation statements)
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“…The measurement of ν spectra from reactors, correlated with β spectra, is currently developing as a technique of monitoring nuclear facilities and would enable direct access to the amount of fissile material produced for military use [10]. The β decays are also known to play an important role in astrophysics, e.g., for the r process, in cosmochronology or for galatic neutrinos [11]. In elementary particle physics, measured ν spectra could highlight possible physics beyond the standard model leading to a hypothetical fourth neutrino coupled only to the gravity field [12].…”
Section: Introductionmentioning
confidence: 99%
“…The measurement of ν spectra from reactors, correlated with β spectra, is currently developing as a technique of monitoring nuclear facilities and would enable direct access to the amount of fissile material produced for military use [10]. The β decays are also known to play an important role in astrophysics, e.g., for the r process, in cosmochronology or for galatic neutrinos [11]. In elementary particle physics, measured ν spectra could highlight possible physics beyond the standard model leading to a hypothetical fourth neutrino coupled only to the gravity field [12].…”
Section: Introductionmentioning
confidence: 99%
“…where S p (n) is the number of pile-ups in channel 'n', S(j ) is the counting rate in the j th channel of the experimental spectrum and K is the maximum channel of the spectrum. The high-energy region of the spectrum near Q EC was used to determine the 'constant' in equation (6). Actually, the amplitude A 1+2 depends on the time between the nuclear decays and varies from A 1 , A 2 to A 1 + A 2 , which results in a spread-out shape of the pile-up spectrum in the low-energy region (where pile-ups are less than 1% of the experimental spectrum) while in the high-energy region (near Q EC ) the shape of the pile-up spectrum remains practically unchanged.…”
Section: Data Processingmentioning
confidence: 99%
“…Information on the 0954-3899/98/040831+15$19.50 c 1998 IOP Publishing Ltd structure of S β (E) is important for different fields of nuclear physics. Prediction of nuclear half-lives [4], analysis of delayed processes [5], analysis of element yields in astrophysical processes [6], in thermonuclear processes [7], in cosmochronology [8], and in technological calculations [5,8] require knowledge of the structure of strength functions for β-transitions.…”
Section: Introductionmentioning
confidence: 99%
“…Additionally, the integrated spectrum shape value is an essential ingredient in astrophysical research such as the r-process [42,43,44]. Here, typically only the Fermi function is included when calculating the Gamow-Teller strength function.…”
Section: Applicationsmentioning
confidence: 99%