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NSR database version of April 11, 2024.

Search: Author = K.I.Tursunmakhatov

Found 6 matches.

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2023TU03      Int.J.Mod.Phys. E32, 2350035 (2023)

K.I.Tursunmakhatov, E.Sh.Ikromkhonov

Asymptotic normalization coefficient for6He+p → 7Li from the proton transfer d(6He, 7Li)n reaction

RADIOACTIVITY 6He(p) [from 2H(6He, 7Li), E=36.4 MeV]; analyzed available data; deduced values of the asymptotic normalization coefficients for the virtual decays, σ(θ), optical model potential parameters.

doi: 10.1142/S0218301323500350
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2023TU06      Phys.Rev. C 108, 065801 (2023)

E.M.Tursunov, S.A.Turakulov, K.I.Tursunmakhatov

Detailed study of the astrophysical direct capture reaction 6Li(p, γ)7Be in a potential model approach

doi: 10.1103/PhysRevC.108.065801
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2022AR03      Eur.Phys.J. A 58, 24 (2022)

S.V.Artemov, R.Yarmukhamedov, N.Burtebayev, B.K.Karakozov, F.Kh.Ergashev, M.Nassurlla, S.B.Igamov, N.Amangeldi, A.Morzabayev, J.Burtebayeva, V.S.Zhdanov, G.Yergaliuly, E.Piasecki, K.Rusek, S.B.Sakuta, A.Demyanova, O.R.Tojiboev, A.Trzcinska, A.Sabidolda, R.Khojayev, K.I.Tursunmakhatov, M.Nassurlla, M.Wolinska-Cichocka, T.Kh.Sadykov, N.Saduyev

Asymptotic normalization coefficient for 12C + p → 13N from the 12C(10B, 9Be)13N reaction and the 12C(p, γ)13N astrophysical S factor

NUCLEAR REACTIONS 12C(10B, 9Be), E=41.3 MeV; measured reaction products. 13N; deduced σ(θ), S factor and thermonuclear reaction rates for 12C(p, γ) reaction, the "indirectly determined" ANC. The modified distorted wave Born approximation (MDWBA) method. The U-200P cyclotron (HIL of the University of Warsaw).

doi: 10.1140/epja/s10050-021-00652-z
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD1017.


2021KI06      Phys.Rev. C 104, 015807 (2021)

G.G.Kiss, M.La Cognata, R.Yarmukhamedov, K.I.Tursunmakhatov, I.Wiedenhover, L.T.Baby, S.Cherubini, A.Cvetinovic, G.D'Agata, P.Figuera, G.L.Guardo, M.Gulino, S.Hayakawa, I.Indelicato, L.Lamia, M.Lattuada, F.Mudo, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, C.Spitaleri, O.Trippella, A.Tumino, M.Anastasiou, S.A.Kuvin, N.Rijal, B.Schmidt, S.B.Igamov, S.B.Sakuta, Zs.Fulop, Gy.Gyurky, T.Szucs, Z.Halasz, E.Somorjai, Z.Hons, J.Mrazek, R.E.Tribble, A.M.Mukhamedzhanov

Indirect determination of the astrophysical S factor for the 6Li (p, γ)7Be reaction using the asymptotic normalization coefficient method

NUCLEAR REACTIONS 6Li(3He, d)7Be, E=3, 5 MeV; measured E(d), I(d), σ(θ) using ΔE-E silicon detector telescopes at the University of Catania and the FN tandem accelerator of Florida State University. 7Be; deduced levels, asymptotic normalization coefficient (ANCs) for the g.s. and the first excited state at 429 keV of 7Be from DWBA analysis of angular distributions. 6Li(p, γ)7Be, E=0.05-0.35 MeV; deduced asymptotic normalization coefficient (ANCs) using results from the 6Li(3He, d) reaction. 6Li(p, γ)7Be, E<1.0 MeV; analyzed available experimental data; deduced astrophysical S factor from direct experimental data, as well as present indirect method from ANCs determined in 6Li(3He, d) experiment. Relevance to big-bang and stellar nucleosynthesis.

doi: 10.1103/PhysRevC.104.015807
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Data from this article have been entered in the XUNDL database. For more information, click here.


2020KI11      Phys.Lett. B 807, 135606 (2020)

G.G.Kiss, M.La Cognata, C.Spitaleri, R.Yarmukhamedov, I.Wiedenhover, L.T.Baby, S.Cherubini, A.Cvetinovic, G.D'Agata, P.Figuera, G.L.Guardo, M.Gulino, S.Hayakawa, I.Indelicato, L.Lamia, M.Lattuada, F.Mudo, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, O.Trippella, A.Tumino, M.Anastasiou, S.A.Kuvin, N.Rijal, B.Schmidt, S.B.Igamov, S.B.Sakuta, K.I.Tursunmakhatov, Zs.Fulop, G.Gyurky, T.Szucs, Z.Halasz, E.Somorjai, Z.Hons, J.Mrazek, R.E.Tribble, A.M.Mukhamedzhanov

Astrophysical S-factor for the 3He(α, γ)7Be reaction via the asymptotic normalization coefficient (ANC) method

NUCLEAR REACTIONS 6Li(3He, d)7Be, E=3, 5 MeV; measured reaction products; deduced σ(θ), S-factor, external capture contribution using the Asymptotic Normalization Coefficient (ANC) technique.

doi: 10.1016/j.physletb.2020.135606
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2598. Data from this article have been entered in the XUNDL database. For more information, click here.


2009AR02      Bull.Rus.Acad.Sci.Phys. 73, 165 (2009); Izv.Akad.Nauk RAS, Ser.Fiz. 73, 176 (2009)

S.V.Artemov, S.B.Igamov, K.I.Tursunmakhatov, R.Yarmukhamedov

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 energies

NUCLEAR REACTIONS 2H(p, γ), E < 50 keV; 16O(p, γ), E < 1.2 MeV; analyzed S-factors; deduced asymptotic normalization coefficients.

doi: 10.3103/S1062873809020075
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Note: The following list of authors and aliases matches the search parameter K.I.Tursunmakhatov: , K.I.TURSUNMAKHATOV