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Cross sections of the <math><mrow><mmultiscripts><mi>Rb</mi><mprescripts/><none/><mn>83</mn></mmultiscripts><mo>(</mo><mi>p</mi><mo>,</mo><mi>γ</mi><mo>)</mo><mmultiscripts><mi>Sr</mi><mprescripts/><none/><mn>84</mn></mmultiscripts></mrow></math> and <math><mrow><mmultiscripts><mi>Kr</mi><mprescripts/><none/><mn>84</mn></mmultiscripts><mo>(</mo><mi>p</mi><mo>,</mo><mi>γ</mi><mo>)</mo><mmultiscripts><mi>Rb</mi><mprescripts/><none/><mn>85</mn></mmultiscripts></mrow></math> reactions at energies characteristic of the astrophysical <math><mi>γ</mi></math> process / Williams, M. (TRIUMF ; York U., England) ; Davids, B. (TRIUMF ; Simon Fraser U.) ; Lotay, G. (Surrey U.) ; Nishimura, N. (Wako, RIKEN ; Nishina Ctr., RIKEN) ; Rauscher, T. (Basel U. ; Hertfordshire U.) ; Gillespie, S.A. (TRIUMF ; Michigan State U.) ; Alcorta, M. (TRIUMF) ; Amthor, A.M. (Bucknell U.) ; Ball, G.C. (TRIUMF) ; Bhattacharjee, S.S. (TRIUMF) et al.
We have measured the cross section of the $^{83}$Rb(p,$\gamma)^{84}$Sr radiative capture reaction in inverse kinematics using a radioactive beam of $^{83}$Rb at incident energies of 2.4 and $2.7 A$ MeV. Prior to the radioactive beam measurement, the $^{84}$Kr(p,$\gamma)^{85}$Rb radiative capture reaction was measured in inverse kinematics using a stable beam of $^{84}$Kr at an incident energy of $2.7 A$ MeV. [...]
arXiv:2303.10282.- 2023-03-13 - 10 p. - Published in : Phys. Rev. C 107 (2023) 035803 Fulltext: PDF;

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Heavy element Nucleosynthesis in the MHD Jet Explosions of Core-Collapse Supernovae / Nishimura, N ; Hashimoto, M A ; Fujimoto, S I ; Kotake, K ; Yamada, S
2006 - Published in : PoS: NIC-IX (2006) , pp. 151 Published version from PoS: PDF;
In : 9th International Symposium on Nuclear Astrophysic: Nuclei in the Cosmos, CERN, Geneva, Switzerland, 25 - 30 Jun 2006, pp.151

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Heavy Element Nucleosynthesis in the MHD Jet Explosions of Core-Collapse Supernovae / Nishimura, Nobuya ; Hahimoto, Masa-aki ; Fujimoto, Shin-ichirou ; Kotake, Kei ; Yamada, Shoichi
For the rst time heavy element nucleosynthesis in the magneto-hydrodynamical (MHD) explosions of core-collapse supernovae are investigated using a massive star of 13M. in a main sequence stage. [...]
2006 - Published in : AIP Conf. Proc.: 847 (2006) , pp. 452-454 External link: Published version from AIP
In : International Symposium on Origin of Matter and Evolution of Galaxies, Tokyo, Japan, 8 - 11 Nov 2005, pp.452-454

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7	Nishimura, N
12	Nishimura, Nobuya

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