S.B. Sakuta
Ism variantlari: S B Sakuta
- Soʻnggi maʼlum muassasa:
- Laboratory No. 2 of the USSR Academy of Sciences
- ORCID:
- 0000-0001-7303-0049
5
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0
i10-indeksi
54
Iqtiboslar
26
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- Indirect determination of the astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor for the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction using the asymptotic normalization coefficient method20218 iqtibos
- Asymptotic normalization coefficients for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mspace width="0.16em"/><mml:mo>+</mml:mo><mml:mspace width="0.16em"/><mml:mi>p</mml:mi><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> from the peripheral <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction and their astrophysical application20168 iqtibos
- Asymptotic normalization coefficient for $${{}^{12}\mathrm{C}}+p\rightarrow {{}^{13}\mathrm{N}}$$ from the $${}^{12}{\mathrm{C}}({}^{10}\mathrm{B},{}^{9}{\mathrm{Be}}){}^{13}\mathrm{N}$$ reaction and the $${}^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$ astrophysical S factor20227 iqtibos
- Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method20205 iqtibos
- Effects of t- and α-transfer on the spectroscopic information from the reaction20135 iqtibos
- Deuteron scattering on 6Li at an energy of 25 MeV20103 iqtibos
- Measurement and analysis of 10B +12C elastic scattering at energy of 41.3MeV20193 iqtibos
- Role of channel coupling and deuteron-exchange mechanisms in anomalous alpha-particle scattering on 6Li20092 iqtibos
- Complex analysis of scattering 1p-shell nuclei in the framework of coupled channel method20161 iqtibos
- Scattering of $$^{10}$$B ions on $$^{11}$$B nuclei at an energy of 41.3 MeV20241 iqtibos
Hammualliflar
- N. Burtebayev15 ta umumiy asarSkelet yozuvlar: 32010–2025
- S. V. Artemov13 ta umumiy asarSkelet yozuvlar: 12009–2025
- M. Nassurlla9 ta umumiy asarSkelet yozuvlar: 22013–2025
- S. B. Igamov9 ta umumiy asar2013–2024
- C. Spitaleri9 ta umumiy asar2016–2023
- К. Rusek8 ta umumiy asarSkelet yozuvlar: 22003–2024
- E. Piasecki8 ta umumiy asarSkelet yozuvlar: 12015–2024
- R. Yarmukhamedov8 ta umumiy asar2009–2023
- A. Trzcińska7 ta umumiy asarSkelet yozuvlar: 12015–2024
- Marzhan Nassurlla6 ta umumiy asarSkelet yozuvlar: 32015–2025