Zobrazeno 1 - 10
of 303
pro vyhledávání: '"Blackmon, J. A."'
Autor:
Lauer-Coles, A., Deibel, C. M., Blackmon, J. C., Hood, A., Good, E. C., Macon, K. T., Santiago-Gonzalez, D., Schatz, H., Ahn, T., Browne, J., Montes, F., Schmidt, K., Ong, 4 W. J., Chipps, K. A., Pain, S. D., Wiedenhöver, I., Baby, L. T., Rijal, N., Anastasiou, M., Upadhyayula, S., Bedoor, S., Hooker, J., Koshchiy, E., Rogachev, G. V.
Background: Type I X-Ray bursts (XRBs) are energetic stellar explosions that occur on the surface of a neutron star in an accreting binary system with a low-mass H/He-rich companion. The rate of the $^{34}$Ar($\alpha,p$)$^{37}$K reaction may influenc
Externí odkaz:
http://arxiv.org/abs/2411.09918
Autor:
Tsintari, P., Dimitrakopoulos, N., Garg, R., Hermansen, K., Marshall, C., Montes, F., Perdikakis, G., Schatz, H., Setoodehnia, K., Arora, H., Berg, G. P. A., Bhandari, R., Blackmon, J. C., Brune, C. R., Chipps, K. A., Couder, M., Deibel, C., Hood, A., Gamage, M. Horana, Jain, R., Maher, C., Miskovitch, S., Pereira, J., Ruland, T., Smith, M. S., Smith, M., Sultana, I., Tinson, C., Tsantiri, A., Villari, A., Wagner, L., Zegers, R. G. T.
The synthesis of heavy elements in supernovae is affected by low-energy (n,p) and (p,n) reactions on unstable nuclei, yet experimental data on such reaction rates are scarce. The SECAR (SEparator for CApture Reactions) recoil separator at FRIB (Facil
Externí odkaz:
http://arxiv.org/abs/2411.03338
Autor:
Browne, J., Chipps, K. A., Schmidt, K., Schatz, H., Ahn, S., Pain, S. D., Montes, F., Ong, W. J., Greife, U., Allen, J., Bardayan, D. W., Blackmon, J. C., Blankstein, D., Cha, S., Chae, K. Y., Febbraro, M., Hall, M. R., Jones, K. L., Kontos, A., Meisel, Z., O'Malley, P. D., Schmitt, K. T., Smith, K., Smith, M. S., Thompson, P., Toomey, R., Vostinar, M., Walter, D.
Publikováno v:
Phys. Rev. Lett. 130 (2023) 212701
The rate of the final step in the astrophysical $\alpha$p-process, the $^{34}$Ar($\alpha$,\textit{p})$^{37}$K reaction, suffers from large uncertainties due to lack of experimental data, despite having a considerable impact on the observable light cu
Externí odkaz:
http://arxiv.org/abs/2305.19422
Autor:
Miskovich, S. A., Montes, F., Berg, G. P. A., Blackmon, J., Chipps, K. A., Couder, M., Deibel, C. M., Hermansen, K., Hood, A. A., Jain, R., Ruland, T., Schatz, H., Smith, M. S., Tsintari, P., Wagner, L.
The SEparator for CApture Reactions (SECAR) is a next-generation recoil separator system at the Facility for Rare Isotope Beams (FRIB) designed for the direct measurement of capture reactions on unstable nuclei in inverse kinematics. To maximize the
Externí odkaz:
http://arxiv.org/abs/2202.01978
Autor:
Anastasiou, M., Wiedenhöver, I., Blackmon, J. C., Baby, L. T., Caussyn, D. D., Hood, A. A., Koshchiy, E., Lighthall, J. C., Macon, K. T., Parker, J. J., Rauscher, T., Rijal, N.
Publikováno v:
Phys. Rev. C 105 (2022) 055806
The $^{18}$Ne($\alpha,p$)$^{21}$Na reaction plays a significant role in Type-I X-ray bursts. It is a major path in the breakout from the hot-CNO cycles to the synthesis of heavier elements in the $\alpha p$-- and $rp$-processes. An experiment to dete
Externí odkaz:
http://arxiv.org/abs/2107.11498
Autor:
Hall, M. R., Bardayan, D. W., Baugher, T., Lepailleur, A., Pain, S. D., Ratkiewicz, A., Ahn, S., Allen, J. M., Anderson, J. T., Ayangeakaa, A. D., Blackmon, J. C., Burcher, S., Carpenter, M. P., Cha, S. M., Chae, K. Y., Chipps, K. A., Cizewski, J. A., Febbraro, M., Hall, O., Hu, J., Jiang, C. L., Jones, K. L., Lee, E. J., O'Malley, P. D., Ota, S., Rasco, B. C., Santiago-Gonzalez, D., Seweryniak, D., Sims, H., Smith, K., Tan, W. P., Thompson, P., Thornsberry, C., Varner, R. L., Walter, D., Wilson, G. L., Zhu, S.
Publikováno v:
Phys. Rev. C 99, 035805, 2019
The $^{15}$O($\alpha$,$\gamma$)$^{19}$Ne reaction is responsible for breakout from the hot CNO cycle in Type I x-ray bursts. Understanding the properties of resonances between $E_x = 4$ and 5 MeV in $^{19}$Ne is crucial in the calculation of this rea
Externí odkaz:
http://arxiv.org/abs/1904.00603
Autor:
Paneru, S. N., Brune, C. R., Giri, R., Livesay, R. J., Greife, U., Blackmon, J. C., Bardayan, D. W., Chipps, K. A., Davids, B., Connolly, D. S., Chae, K. Y., Champagne, A. E., Deibel, C., Jones, K. L., Johnson, M. S., Kozub, R. L., Ma, Z., Nesaraja, C. D., Pain, S. D., Sarazin, F., Shriner Jr., J. F., Stracener, D. W., Smith, M. S., Thomas, J. S., Visser, D. W., Wrede, C.
Publikováno v:
Phys. Rev. C 99, 045807 (2019)
The astrophysical $S$-factor for the radiative proton capture reaction on $^7$Be ($S_{17}$) at low energies is affected by the $s$-wave scattering lengths. We report the measurement of elastic and inelastic scattering cross sections for the $^7$Be+p
Externí odkaz:
http://arxiv.org/abs/1902.00417
Autor:
Hall, M. R., Barbadian, D. W., Baugher, T., Lepailleur, A., Pain, S. D., Ratkiewicz, A., Ahn, S., Allen, J. M., Anderson, J. T., Ayangeakaa, A. D., Blackmon, J. C., Burcher, S., Carpenter, M. P., Cha, S. M., Chae, K. Y., Chipps, K. A., Cizewski, J. A., Febbraro, M., Hall, O., Hu, J., Jiang, C. L., Jones, K. L., Lee, E. J., O'Malley, P. D., Ota, S., Rasco, B. C., Santiago-Gonzalez, D., Seweryniak, D., Sims, H., Smith, K., Tan, W. P., Thompson, P., Thornsberry, C., Varner, R. L., Walter, D., Wilson, G. L., Zhu, S.
Publikováno v:
Phys. Rev. Lett. 122, 052701, 2019
Detection of nuclear-decay $\gamma$ rays provides a sensitive thermometer of nova nucleosynthesis. The most intense $\gamma$-ray flux is thought to be annihilation radiation from the $\beta^+$ decay of $^{18}$F, which is destroyed prior to decay by t
Externí odkaz:
http://arxiv.org/abs/1902.00106
Autor:
Rijal, N., Wiedenhöver, I., Blackmon, J. C., Anastasiou, M., Baby, L. T., Caussyn, D. D., Höflich, P., Kemper, K. W., Koshchiy, E., Rogachev, G. V.
Publikováno v:
Phys. Rev. Lett. 122, 182701 (2019)
The cross sections of nuclear reactions between the radioisotope $^7$Be and deuterium, a possible mechanism of reducing the production of mass-7 nuclides in Big-Bang nucleosynthesis, were measured at center-of-mass energies between 0.2 MeV and 1.5 Me
Externí odkaz:
http://arxiv.org/abs/1808.07893
Autor:
Wilson, G. L., Catford, W. N., Orr, N. A., Diget, C. Aa., Matta, A., Hackman, G., Williams, S. J., Celik, I. C., Achouri, N. L., Falou, H. Al, Ashley, R., Austin, R. A. E., Ball, G. C., Blackmon, J. C., Boston, A. J., Boston, H. C., Brown, S. M., Cross, D. S., Djongolov, M., Drake, T. E., Hager, U., Fox, S. P., Fulton, B. R., Galinski, N., Garnsworthy, A. B., Jamieson, D., Kanungo, R., Leach, K. G., Orce, J. N., Pearson, C. J., Porter-Peden, M., Sarazin, F., Simpson, E. C., Sjue, S., Smalley, D., Sumithrarachchi, C., Svensson, C. E., Triambak, S., Unsworth, C., Wadsworth, R.
The levels in 26Na with single particle character have been observed for the first time using the d(25Na,p gamma) reaction at 5 MeV/nucleon. The measured excitation energies and the deduced spectroscopic factors are in good overall agreement with (0+
Externí odkaz:
http://arxiv.org/abs/1508.01757