Zobrazeno 1 - 6
of 6
pro vyhledávání: '"J. M. Fetter"'
Autor:
J. W. Jänecke, Daniel A. Butts, M. Belbot, J. M. Fetter, K. Lamkin, D.A. Roberts, K. Ieki, R. E. Warner, A. Muthukrishnan, P. D. Zecher, M. Zahar, Aaron Galonsky, C. L. Carpenter, J. J. Kolata, F. D. Becchetti
Publikováno v:
Physical Review C. 51:178-181
A radioactive nuclear beam of 10.2 MeV $^{6}\mathrm{He}$, with typical intensity 5\ifmmode\times\else\texttimes\fi{}${10}^{4}$ ${\mathrm{s}}^{\mathrm{\ensuremath{-}}1}$, was produced via the $^{9}\mathrm{Be}$${(}^{7}$Li${,}^{6}$He${)}^{10}$B reaction
Autor:
R. E. Warner, Akira Okihana, Jirohta Kasagi, Mamoru Fujiwara, T. Yoshimura, R. A. Swartz, Norihiko Koori, T. Hayashi, P. D. Kunz, S. Kakigi, J. M. Fetter, Takehiko Konishi, Kiyoji Fukunaga
Publikováno v:
Physical Review C. 49:1534-1539
Publikováno v:
Physical Review C. 48:245-249
A magnetic spectrograph and position-sensitive detectors were used to measure the total nuclear reaction probability [eta][sub [ital R]] for [alpha]+CsI at 116 MeV, [sup 14]N+CsI at 265 and 385 MeV, and [sup 14]N+Si at 271 and 390 MeV. From these [et
Publikováno v:
Astroparticle Physics, vol 18, iss 5
Fetter, J; McLaughlin, GC; Balantekin, AB; & Fuller, GM. (2003). Active–sterile neutrino conversion: consequences for the r-process and supernova neutrino detection. Astroparticle Physics, 18(5), 433-448. doi: 10.1016/s0927-6505(02)00156-1. UC Office of the President: Research Grants Program Office (RGPO). Retrieved from: http://www.escholarship.org/uc/item/31j1j2w3
Fetter, J; McLaughlin, GC; Balantekin, AB; & Fuller, GM. (2003). Active–sterile neutrino conversion: consequences for the r-process and supernova neutrino detection. Astroparticle Physics, 18(5), 433-448. doi: 10.1016/s0927-6505(02)00156-1. UC Office of the President: Research Grants Program Office (RGPO). Retrieved from: http://www.escholarship.org/uc/item/31j1j2w3
We examine active-sterile neutrino conversion in the late time post-core-bounce supernova environment. By including the effect of feedback on the Mikheyev-Smirnov-Wolfenstein (MSW) conversion potential, we obtain a large range of neutrino mixing para
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d9a69c0710477688ed31baa6c9d200b5
https://escholarship.org/uc/item/31j1j2w3
https://escholarship.org/uc/item/31j1j2w3
Publikováno v:
McLaughlin, GC; Fetter, JM; Balantekin, AB; & Fuller, GM. (1999). Active-sterile neutrino transformation solution forr-process nucleosynthesis. Physical Review C, 59(5), 2873-2887. doi: 10.1103/physrevc.59.2873. UC Office of the President: Research Grants Program Office (RGPO). Retrieved from: http://www.escholarship.org/uc/item/86x6092f
We discuss how matter-enhanced active-sterile neutrino transformation in both neutrino and antineutrino channels could enable the production of the rapid neutron capture (r-process) nuclei in neutrino-heated supernova ejecta. In this scheme the light
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5a1e64c6719865a50ec5e8a55b9b996d
http://www.escholarship.org/uc/item/86x6092f
http://www.escholarship.org/uc/item/86x6092f
We consider the effect on matter-enhanced neutrino flavor transformation of a randomly fluctuating, delta-correlated matter density. The fluctuations will produce a distribution of neutrino survival probabilities. We find the mean and variance of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ba9c1bb77f16c245fd4a27695d8c4bbf