Hindered E4 decay of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:msup><mml:mn>12</mml:mn><mml:mo>+</mml:mo></mml:msup></mml:math> yrast trap in 52Fe

Gadea, A.; Lenzi, S. M.; Napoli, D. R.; Axiotis, M.; Ur, C. A.; Martı́nez-Pinedo, G.; Górska, M.; Roeckl, E.; Caurier, E.; Nowacki, F.; Angelis, G. de; Batist, L.; Borcea, R.; Brandolini, F.; Cano‐Ott, D.; Döring, J.; Fahlander, C.; Farnea, E.; Grawe, H.; Hellström, M.; Janas, Z.; Kirchner, R.; Commara, M. La; Mazzocchi, C.; Nácher, E.; Plettner, C.; Płochocki, A.; Rubio, B.; Schmidt, K.; Schwengner, R.; Taín, J. L.; Ż̷ylicz, J.

doi:10.1016/j.physletb.2005.05.073

Cited by 14 publications

(1 citation statement)

References 22 publications

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“…7). The excitation energy for the isomer, E x = 6960.7(9) keV, determined in this work differs by 2.7(10) keV from the literature value E x = 6958.0(4) keV [18] based on the observation of an E4 γ transitions from this 12 + yrast trap in 52 Fe [49]. It should be noted that the relative uncertainties of the measured frequency ratios, 2.8 × 10 −9 and 5.6 × 10 −9 for 52 Fe + and 52 Fe m+ , respectively, are much smaller than the relative uncertainty in the reference mass δm/m( 52 Cr) = 1.2 × 10 −8 .…”

Section: Resultscontrasting

confidence: 89%

High-precision mass measurements for the isobaric multiplet mass equation atA= 52

Nesterenko¹,

Kankainen²,

Cañete³

et al. 2017

J. Phys. G: Nucl. Part. Phys.

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Masses ofCo m have been experimentally determined for the first time and found to be more bound than predicted by extrapolations. The isobaric multiplet mass equation for the T = 2 quintet at A = 52 has been studied employing the new mass values. No significant breakdown (beyond the 3σ level) of the quadratic form of the IMME was observed (χ 2 /n = 2.4). The cubic coefficient was 6.0(32) keV (χ 2 /n = 1.1). The excitation energies for the isomer and the T = 2 isobaric analogue state in 52 Co have been determined to be 374(13) keV and 2922(13) keV, respectively. The Q value for the proton decay from the 19/2 − isomer in 53 Co has been determined with an unprecedented precision, Qp = 1558.8(17) keV. The proton separation energies of 52 Co and 53 Ni relevant for the astrophysical rapid proton capture process have been experimentally determined for the first time.

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Section: Resultscontrasting

confidence: 89%