Zobrazeno 1 - 10
of 238
pro vyhledávání: '"Gorres, J."'
Autor:
Shahina, S., Gorres, J., Robertson, D., Couder, M., Gomez, O., Gula, A., Hanhardt, M., Kadlecek, T., Kelmar, R., Scholz, P., Simon, A., Stech, E., Strieder, F., Wiescher, M.
The $^{22}\rm{Ne}(\alpha,\gamma)^{26}\rm{Mg}$ is an important reaction in stellar helium burning environments as it competes directly with one of the main neutron sources for the s-process, the $^{22}\rm{Ne}(\alpha,n)^{25}\rm{Mg}$ reaction. The react
Externí odkaz:
http://arxiv.org/abs/2208.07885
Autor:
Sagara, Issaka, Healy, Sara A, Assadou, Mahamadoun H, Kone, Mamady, Swihart, Bruce J, Kwan, Jennifer L, Fintzi, Jonathan, Sissoko, Kourane, Kamate, Bourama, Samake, Yacouba, Guindo, Merepen A, Doucoure, M'Bouye, Niaré, Karamoko, Dolo, Amagana, Diarra, Balla, Rausch, Kelly M, Narum, David L, Jones, David S, MacDonald, Nicholas J, Zhu, Daming, Gorres, J Patrick, Imeru, Alemush, Mohan, Rathy, Thera, Ismaila, Zaidi, Irfan, Salazar-Miralles, Fernando, Duan, Junhui, Neal, Jillian, Morrison, Robert D, Muratova, Olga, Sylla, Daman, O'Connell, Elise M, Wu, Yimin, Hume, Jen C C, Coulibaly, Mamadou B, Anderson, Charles F, Traore, Sekou F, Doumbo, Ogobara K, Duffy, Patrick E *
Publikováno v:
In The Lancet Infectious Diseases November 2023 23(11):1266-1279
Autor:
Rausch, Kelly M., Barnafo, Emma K., Lambert, Lynn E., Muratova, Olga, Gorres, J. Patrick, Anderson, Charles, Narum, David L., Wu, Yimin, Morrison, Robert D., Zaidi, Irfan, Duffy, Patrick E.
Publikováno v:
In iScience 21 July 2023 26(7)
Akademický článek
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Autor:
deBoer, R. J., Gorres, J., Wiescher, M., Azuma, R. E., Best, A., Brune, C. R., Fields, C. E., Jones, S., Pignatari, M., Sayre, D., Smith, K., Timmes, F. X., Uberseder, E.
Publikováno v:
Reviews of Modern Physics 89, 035007 (2017)
The creation of carbon and oxygen in our universe is one of the forefront questions in nuclear astrophysics. The determination of the abundance of these elements is key to both our understanding of the formation of life on earth and to the life cycle
Externí odkaz:
http://arxiv.org/abs/1709.03144
Autor:
Talwar, R., Adachi, T., Berg, G. P. A., Bin, L., Bisterzo, S., Couder, M., deBoer, R. J., Fang, X., Fujita, H., Fujita, Y., Gorres, J., Hatanaka, K., Itoh, T., Kadoya, T., Long, A., Miki, K., Patel, D., Pignatari, M., Shimbara, Y., Tamii, A., Wiescher, M., Yamamoto, T., Yosoi, M.
The $^{22}$Ne($\alpha$,n)$^{25}$Mg reaction is the dominant neutron source for the slow neutron capture process ($s$-process) in massive stars and contributes, together with the $^{13}$C($\alpha$,n)$^{16}$O, to the production of neutrons for the $s$-
Externí odkaz:
http://arxiv.org/abs/1508.05660
Akademický článek
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Autor:
Spyrou, A., Quinn, S. J., Simon, A., Rauscher, T., Battaglia, A., Best, A., Bucher, B., Couder, M., DeYoung, P. A., Dombos, A. C., Fang, X., Gorres, J., Kontos, A., Li, Q., Lin, L. Y., Long, A., Lyons, S., Meyer, B. 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 88 (2013) 045802
Cross section measurements of the reactions $^{90, 92}$Zr(p,$\gamma$)$^{91,93}$Nb were performed using the NSCL SuN detector at the University of Notre Dame. These reactions are part of the nuclear reaction flow for the synthesis of the light p nucle
Externí odkaz:
http://arxiv.org/abs/1310.5667
Autor:
Gyurky, Gy., Kiss, G. G., Elekes, Z., Fulop, Zs., Somorjai, E., Palumbo, A., Gorres, J., Lee, H. Y., Rapp, W., Wiescher, M., Ozkan, N., Guray, R. T., Efe, G., Rauscher, T
Publikováno v:
Phys.Rev. C74 (2006) 025805
The 106Cd(alpha,gamma)110Sn reaction cross section has been measured in the energy range of the Gamow window for the astrophysical p-process scenario. The cross sections for 106Cd(alpha,n)109Sn and for 106Cd(alpha,p)109In below the (alpha,n) threshol
Externí odkaz:
http://arxiv.org/abs/nucl-ex/0605034
Publikováno v:
Mon.Not.Roy.Astron.Soc.360:375-379,2005
In the light of recent recalculations of the \el{19}{F}(alpha,p)\el{22}{Ne} reaction rate we present results of the expected yield of \el{19}{F} from Wolf-Rayet (WR) stars. We have computed models using the upper and lower limits for the rate in addi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0504163