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Energy, strength, and alpha width measurements of $E_{\rm{c.m.}} = 1323$ and $1487$ keV resonances in $^{15}$N($\alpha,\gamma$)$^{19}$F

Autor: Fang, R., Görres, J., deBoer, R. J., Moylan, S., Sanchez, A., Bailey, T. L., Carmichael, S., Koros, J., Lee, K., Manukyan, K., Matney, M., McDonaugh, J. P., Robertson, D., Rufino, J., Stech, E., Couder, M.

The $^{15}$N($\alpha,\gamma$)$^{19}$F reaction produces $^{19}$F in asymptotic giant branch (AGB) stars, where the low energy tails of two resonances at $E_{\rm{c.m.}} = 1323 \pm 2$ and $1487 \pm 1.7$ keV are estimated to contribute about $30\%$ of t

Externí odkaz: http://arxiv.org/abs/2404.01271

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First Measurement of the $B(E2; 3/2^- \rightarrow 1/2^-)$ Transition Strength in $^7$Be: Testing Ab Initio Predictions for $A=7$ Nuclei

Autor: Henderson, S. L., Ahn, T., Caprio, M. A., Fasano, P. J., Simon, A., Tan, W., O'Malley, P., Allen, J., Bardayan, D. W., Blankstein, D., Frentz, B., Hall, M. R., Kolata, J. J., McCoy, A. E., Moylan, S., Reingold, C. S., Strauss, S. Y., Torres-Isea, R. O.

Publikováno v: Phys. Rev. C 99, 064320 (2019)

Electromagnetic observables are able to give insight into collective and emergent features in nuclei, including nuclear clustering. These observables also provide strong constraints for ab initio theory, but comparison of these observables between th

Externí odkaz: http://arxiv.org/abs/2109.07312

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Akademický článek

Elimination of restrictive practices from acute adult mental health care services: A qualitative evidence synthesis of the lived experience literature.

Autor: Bennetts, S.L. ^{a, b, ⁎}, Pepin, G. ^{a, c}, Moylan, S. ^b, Carolin, R. ^b, Lucas, J.J. ^{a, c}

Publikováno v: In SSM - Mental Health June 2024 5

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Lifetime measurements of excited states in $^{15}$O

Autor: Frentz, B., Aprahamian, A., Clark, A. M., Dulal, C., Enright, J. D., deBoer, R. J., Görres, J., Henderson, S. L., Howard, K. B., Kelmar, R., Lee, K., Morales, L., Moylan, S., Raman, Z., Tan, W., Weghorn, L. E., Wiescher, M.

Publikováno v: Phys. Rev. C 103, 045802 (2021)

The CNO cycle is the main energy source in stars more massive than our sun, it defines the energy production and the cycle time that lead to the lifetime of massive stars, and it is an important tool for the determination of the age of globular clust

Externí odkaz: http://arxiv.org/abs/2012.13029

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New measurement of $^{12}$C+$^{12}$C fusion reaction at astrophysical energies

Publikováno v: Phys. Rev. Lett. 124, 192702 (2020)

Carbon and oxygen burning reactions, in particular, $^{12}$C+$^{12}$C fusion, are important for the understanding and interpretation of the late phases of stellar evolution as well as the ignition and nucleosynthesis in cataclysmic binary systems suc

Externí odkaz: http://arxiv.org/abs/2005.03196

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