Zobrazeno 1 - 10
of 396
pro vyhledávání: '"Kolbe, E."'
Autor:
Stansfield, C.R., Somerville, R.F., Hassan, V.R., Kolbe, E., Partington, H.K., Walsh, K.A.J., Johnson, C.S.
Publikováno v:
In Forensic Science International November 2020 316
Autor:
Johnson, C.S. ⁎, Stansfield, C.R., Hassan, V.R., Kolbe, E., Partington, H.K., Kappatos, D.C., Somerville, R.F.
Publikováno v:
In Forensic Science International February 2020 307
Autor:
Somerville, R.F., Hassan, V.R., Kolbe, E., Partington, H.K., Walsh, K.A.J., Kappatos, D.C., Johnson, C.S.
Publikováno v:
In Forensic Science International July 2019 300:19-27
Publikováno v:
Nucl.Phys. A747 (2005) 633-654
Fission plays an important role in the r-process which is responsible not only for the yields of transuranium isotopes, but may have a strong influence on the formation of the majority of heavy nuclei due to fission recycling. We present calculations
Externí odkaz:
http://arxiv.org/abs/astro-ph/0412654
Publikováno v:
J.Phys.G29:2569-2596,2003
The methods used in the evaluation of the neutrino-nucleus cross section are reviewed. Results are shown for a variety of targets of practical importance. Many of the described reactions are accessible in future experiments with neutrino sources from
Externí odkaz:
http://arxiv.org/abs/nucl-th/0311022
Publikováno v:
Phys.Rev.Lett.92:111101,2004
We calculate neutrino-induced fission cross sections for selected nuclei with Z=84-92. We show that these reactions populate the daughter nucleus at excitation energies where shell effects are significantly washed out, effectively reducing the fissio
Externí odkaz:
http://arxiv.org/abs/astro-ph/0308350
Publikováno v:
Phys.Lett.B606:258-264,2005
We study neutrino process nucleosynthesis in massive stars using newly calculated cross sections, an expanded reaction network, and complete and self-consistent models of the progenitor star. We reevaluate the production of light isotopes from abunda
Externí odkaz:
http://arxiv.org/abs/astro-ph/0307546
Publikováno v:
Nucl.Phys. A718 (2003) 440-442
Electron capture rates on neutron-rich nuclei (A>65) were calculated within the Random Phase Approximation with partial number formalism, including allowed and forbidden transitions. The partial occupation numbers were provided as a function of tempe
Externí odkaz:
http://arxiv.org/abs/nucl-th/0209057
Autor:
Thielemann, F. -K., Brachwitz, F., Freiburghaus, C., Kolbe, E., Martinez-Pinedo, G., Rauscher, T., Rembges, F., Hix, W. R., Liebendoerfer, M., Mezzacappa, A., Kratz, K. -L., Pfeiffer, B., Langanke, K., Nomoto, K., Rosswog, S., Schatz, H., Wiescher, M.
Publikováno v:
Prog.Part.Nucl.Phys.46:5-22,2001
Except for 1H, 2H, 3He, 4He, and 7Li, originating from the Big Bang, all heavier elements are made in stellar evolution and stellar explosions. Nuclear physics, and in many cases nuclear structure far from stability, enters in a crucial way. Therefor
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101476
Publikováno v:
Phys.Rev. C63 (2001) 032801
We propose a new model to calculate stellar electron capture rates for neutron-rich nuclei. These nuclei are encountered in the core-collapse of a massive star. Using the Shell Model Monte Carlo approach, we first calculate the finite temperature occ
Externí odkaz:
http://arxiv.org/abs/nucl-th/0012036