The 25Mg(p, γ)26Al and 25Mg(p, p′) resonances for Ep = 0.31–1.84 MeV

Endt, P.M.; Wit, Pieter De; Alderliesten, C.

doi:10.1016/0375-9474(86)90056-4

Cited by 63 publications

(50 citation statements)

References 12 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…(2) The 25 Mg(p,␥) 26 Al reaction Surveys of resonances in the 25 Mg(p,␥) 26 Al reaction have been reported (Elix et al, 1979;Anderson et al, 1980;Endt et al, 1986;Iliadis et al, 1990) and results are tabulated in Endt90. A search for possible low-energy resonances was undertaken by Champagne et al (1983) using data obtained via the 25 Mg( 3 He,d) reaction.…”

Section: Reaction Ratesmentioning

confidence: 99%

“…Unfortunately, some of the conclusions that they drew from their data were in error. Motivated by the 25 Mg(p,␥␥) studies of Endt et al (1986), improved, higher-resolution ( 3 He,d) measurements were performed (Champagne et al, 1986a) that produced a more reliable set of spectroscopic factors and reaction rates. A notable outcome of this work was the identification of a strong s-wave resonance at an energy of E c.m.…”

Section: Reaction Ratesmentioning

confidence: 99%

See 1 more Smart Citation

Synthesis of the elements in stars: forty years of progress

et al. 1997

View full text Add to dashboard Cite

Forty years ago Burbidge, Burbidge, Fowler, and Hoyle combined what we would now call fragmentary evidence from nuclear physics, stellar evolution and the abundances of elements and isotopes in the solar system as well as a few stars into a synthesis of remarkable ingenuity. Their review provided a foundation for forty years of research in all of the aspects of low energy nuclear experiments and theory, stellar modeling over a wide range of mass and composition, and abundance studies of many hundreds of stars, many of which have shown distinct evidence of the processes suggested by B 2 FH. In this review we summarize progress in each of these fields with emphasis on the most recent developments. [S0034-6861(97)

show abstract

Section: Reaction Ratesmentioning

confidence: 99%

Section: Reaction Ratesmentioning

confidence: 99%

Synthesis of the elements in stars: forty years of progress

et al. 1997

View full text Add to dashboard Cite

show abstract

“…The (5,6) + assignment for the level at 7921 keV, based on two 25 Mg(p,γ) spectroscopy measurements [31,32], is not immediately compatible with the assignment of ℓ = (1, 2) from this work. However, ℓ ≥ 4 could not be ruled out due to a lack of telling features in the measured angular distribution, such that further constraint on the spin and parity assignment by this work was not possible.…”

Section: Methodsmentioning

confidence: 65%

28Si(p,3He) reaction for spectroscopy of
Chipps
¹
,
Bardayan
²
,
Chae
³

et al. 2012
Phys. Rev. C
15
0
6
0
View full text Add to dashboard Cite

The28 Si(p, 3 He) 26 Al reaction was utilized for the first time to study the levels in 26 Al, using a proton beam from the Holifield Radioactive Ion Beam Facility (HRIBF). Five previously unreported states in 26 Al are observed and discussed, including Distorted Wave Born Approximation (DWBA) analysis. Proton-decay branching ratios consistent with previous studies and theoretical expectations were found by detecting decay protons from highly excited 26 Al states in coincidence with the 3 He particles.

show abstract

“…The analysis of the experimental data [9][10][11][12][13][14][15][16][17] allowed us to obtain distributions of the M 1-transition probabilities for the ground state in the 22 N a, 30 P , 34 Cl nuclei (Fig.3). …”

Section: Ev Was Detectedmentioning

confidence: 99%