Zobrazeno 1 - 10
of 512
pro vyhledávání: '"Goerres, J."'
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
Autor:
Lee, H.Y., Kuvin, S.A., Mosby, S.M., Prokop, C.J., Long, A.M., Votaw, D., Georgiadou, A., Görres, J., Stech, E., Wiescher, M.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A December 2024 1069
Publikováno v:
In Agricultural Water Management 1 November 2024 304
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
Akademický článek
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Autor:
Halász, Z., Somorjai, E., Gyürky, Gy., Elekes, Z., Fülöp, Zs., Szücs, T., Kiss, G. G., Szegedi, N., Rauscher, T., Görres, J., Wiescher, M.
Publikováno v:
Phys. Rev. C 94, 045801 (2016)
The synthesis of heavy, proton rich isotopes in the astrophysical gamma-process proceeds through photodisintegration reactions. For the improved understanding of the process, the rates of the involved nuclear reactions must be known. The reaction 128
Externí odkaz:
http://arxiv.org/abs/1609.05612
Autor:
Quinn, S. J., Spyrou, A., Bravo, E., Rauscher, T., Simon, A., Battaglia, A., Bowers, M., Bucher, B., Casarella, C., Couder, M., DeYoung, P. A., Dombos, A. C., Görres, J., Kontos, A., Li, Q., Long, A., Moran, M., Paul, N., Pereira, J., Robertson, D., Smith, K., Smith, M. K., Stech, E., Talwar, R., Tan, W. P., Wiescher, M.
Publikováno v:
Phys. Rev. C 89, 054611 (2014)
Cross section measurements of the $^{58}$Ni($\alpha$,$\gamma$)$^{62}$Zn reaction were performed in the energy range $E_{\alpha}=5.5-9.5$ MeV at the Nuclear Science Laboratory of the University of Notre Dame, using the NSCL Summing NaI(Tl) detector an
Externí odkaz:
http://arxiv.org/abs/1405.6149
Autor:
Kiss, G. G., Mohr, P., Fülöp, Zs., Gyürky, Gy., Elekes, Z., Farkas, J., Somorjai, E., Yalcin, C., Galaviz, D., Güray, R. T., Özkan, N., Görres, J.
Publikováno v:
Physical Review C 83, 065807 (2011)
The elastic scattering cross sections for the reactions $^{110,116}$Cd($\alpha,\alpha$)$^{110,116}$Cd at energies above and below the Coulomb barrier are presented to provide a sensitive test for the alpha-nucleus optical potential parameter sets. Ad
Externí odkaz:
http://arxiv.org/abs/1312.2260
Autor:
Bisterzo, S., Travaglio, C., Wiescher, M., Gallino, R., Kaeppeler, F., Straniero, O., Cristallo, S., Imbriani, G., Goerres, J., deBoer, R. J.
We study the s-process abundances at the epoch of the Solar-system formation as the outcome of nucleosynthesis occurring in AGB stars of various masses and metallicities. The calculations have been performed with the Galactic chemical evolution (GCE)
Externí odkaz:
http://arxiv.org/abs/1311.5381
Autor:
Simon, A., Spyrou, A., Rauscher, T., Fröhlich, C., Quinn, S. J., Battaglia, A., Best, A., Bucher, B., Couder, M., DeYoung, P. A., Fang, X., Görres, J., Kontos, A., Li, Q., Lin, L. -Y., Long, A., Lyons, S., Roberts, A., Robertson, D., Smith, K., Smith, M. K., Stech, E., Stefanek, B., Tan, W. P., Tang, X. D., Wiescher, M.
Publikováno v:
Phys. Rev. C 87 (2013) 055802
A systematic study of the radiative proton capture reaction for all stable nickel isotopes is presented. The results were obtained using 2.0 - 6.0 MeV protons from the 11 MV tandem Van de Graaff accelerator at the University of Notre Dame. The \gamma
Externí odkaz:
http://arxiv.org/abs/1305.1213