K. I. Tursunmakhatov

Энг кўп иқтибос қилинган асарлар

1. Determination of nuclear vertex constants (asymptotic normalization coefficients) for the virtual decays 3He → d + p and 17F → 16O + p and their use for extrapolating astrophysical S-factors of the radiative proton capture by the deuteron and the 16O nucleus at very low energies20098 иқтибос
2. 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 method20217 иқтибос
3. Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method20205 иқтибос
4. Asymptotic normalization coefficient for the ⁶Li+n→7Li from the ⁶Li(d,p)7Li reaction and cross-section for the ⁶Li(n,γ)7Li reaction20255 иқтибос
5. Detailed study of the astrophysical direct capture reaction <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><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> in a potential model approach20235 иқтибос
6. Extrapolation of astrophysical S factors for the reaction 14N((p, γ) 15O to near-zero energies20124 иқтибос
7. Asymptotic normalization coefficient for⁶He+p→7Li from the proton transfer d(⁶He,⁷Li)n reaction20234 иқтибос
8. 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 factor20224 иқтибос
9. Asymptotic theory of charged particle transfer reactions at low energies and nuclear astrophysics20192 иқтибос
10. Determination of the asymptotic normalization coefficient for ¹⁶O+n→¹⁷O from the ¹⁶O(d,p)¹⁷O reaction20251 иқтибос