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NSR database version of April 11, 2024.

Search: Author = S.B.Igamov

Found 19 matches.

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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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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.


2017IG01      Phys.Atomic Nuclei 80, 251 (2017); Yad.Fiz. 80, 127 (2017)

S.B.Igamov

Asymptotic three-particle approach to the Coulomb breakup process 6Li + 208Pb → 208Pb + α + d

doi: 10.1134/S1063778817010082
Citations: PlumX Metrics


2013BU09      Nucl.Phys. A909, 20 (2013)

N.Burtebayev, J.T.Burtebayeva, N.V.Glushchenko, Zh.K.Kerimkulov, A.Amar, M.Nassurlla, S.B.Sakuta, S.V.Artemov, S.B.Igamov, A.A.Karakhodzhaev, K.Rusek, S.Kliczewski

Effects of t- and α-transfer on the spectroscopic information from the 6Li(3He, d)7Be reaction

NUCLEAR REACTIONS 6Li(3He, 3He), (3He, 3He'), (3He, d), E=34, 50, 60, 72$ MeV; measured E(particle), I(particle, θ); deduced spectroscopic factor for t+3He configuration of 6Li, σ(θ), spectroscopic factor, asymptotical normalization coefficients; calculated folding optical potential, elastic scattering σ(θ), deuteron emission σ(θ) using DWBA and CC (coupled channels) with 15 sets of parameters.

doi: 10.1016/j.nuclphysa.2013.04.008
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0712. Data from this article have been entered in the XUNDL database. For more information, click here.


2012AR03      Phys.Atomic Nuclei 75, 291 (2012); Yad.Fiz. 75, 320 (2012)

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

Extrapolation of astrophysical S factors for the reaction 14N((p, γ) 15O to near-zero energies

NUCLEAR REACTIONS 14N(p, γ), E not given; calculated S-factors. R-matrix approach.

NUCLEAR REACTIONS 14N(3He, d), E=20, 33.3, 26.3 MeV; analyzed available data; deduced contribution of direct radiation capture to bound states of 15O.

doi: 10.1134/S1063778812020032
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0945.


2010AR03      Int.J.Mod.Phys. E19, 1102 (2010)

S.V.Artemov, S.B.Igamov, A.A.Karakhodzhaev, G.K.Nie, R.Yarmukhamedov, E.A.Zaparov, N.Burtebaev, K.E.Rehm

Estimates of the astrophysical S-factors for proton radiative capture by 10B and 24Mg nuclei using the ANCs from proton transfer reactions

NUCLEAR REACTIONS 10B, 24Mg(p, γ), E<2.5 MeV; analyzed nucleon transfer reactions 10B, 24Mg(3He, d); deduced S-factors, partial resonance widths, branching ratios. R-matrix formalism, empirical proton asymptotical normalization coefficients (ANC).

doi: 10.1142/S0218301310015540
Citations: PlumX Metrics


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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2008AR04      Phys.Atomic Nuclei 71, 998 (2008); Yad.Fiz. 71, 1025 (2008)

S.V.Artemov, A.G.Bajajin, S.B.Igamov, G.K.Nie, R.Yarmukhamedov

Nuclear asymptotic normalization coefficients for 14N → 13C + p configurations and astrophysical S factor for radiative proton capture

NUCLEAR REACTIONS 13C(3He, d), E=15-40 MeV; analyzed σ. 14N; deduced asymptotic normalization coefficients for proton bound states. 13C(p, γ); deduced S-factor.

doi: 10.1134/S1063778808060045
Citations: PlumX Metrics


2008BU19      Phys.Rev. C 78, 035802 (2008)

N.Burtebaev, S.B.Igamov, R.J.Peterson, R.Yarmukhamedov, D.M.Zazulin

New measurements of the astrophysical S factor for 12C(p, γ)13N reaction at low energies and the asymptotic normalization coefficient (nuclear vertex constant) for the p+12C → 13N reaction

NUCLEAR REACTIONS 12C(p, γ), E=354, 390, 460, 463, 565, 750, 1061 keV; measured Eγ, Iγ, σ, σ(θ). Deduced astrophysical S-factors, asymptotic normalization coefficients.

doi: 10.1103/PhysRevC.78.035802
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0819.


2008IG03      Phys.Atomic Nuclei 71, 1740 (2008)

S.B.Igamov, R.Yarmukhamedov

Asymptotic normalization coefficients (nuclear vertex constants) for p + 7Be → 8B and the direct 7Be(p, γ)8B astrophysical S factors at solar energies

NUCLEAR REACTIONS 7Be(p, γ), E ≤ 1200 keV; analyzed S-factors; deduced asymptotic normalized coefficients, nuclear vertex constants.

doi: 10.1134/S1063778808100098
Citations: PlumX Metrics


2007IG01      Nucl.Phys. A781, 247 (2007); Erratum Nucl.Phys. A832, 346 (2010)

S.B.Igamov, R.Yarmukhamedov

Modified two-body potential approach to the peripheral direct capture astrophysical α + A → B + γ reaction and asymptotic normalization coefficients

NUCLEAR REACTIONS 4He(t, γ), E=0.055, 0.560, 1.200 MeV; calculated asymptotic normalization coefficients, astrophysical S-factors, related features. Modified two-body potential approach.

doi: 10.1016/j.nuclphysa.2006.10.041
Citations: PlumX Metrics


2007IG04      Phys.Atomic Nuclei 70, 1694 (2007)

S.B.Igamov, M.S.Nadirbekov, R.Yarmukhamedov

Influence of the three-body Coulomb effects on the values of asymptotic normalization coefficients (nuclear vertex constants) of astrophysical interest extracted from the modified DWBA approach for the peripheral proton-transfer reactions

NUCLEAR REACTIONS 13C(p, γ), E = low; calculated asymptotic normalization factors using the 3-body DWBA approach.

doi: 10.1134/S1063778807100031
Citations: PlumX Metrics


2006BL07      Phys.Atomic Nuclei 69, 433 (2006); Yad.Fiz. 69, 456 (2006)

L.D.Blokhintsev, S.B.Igamov, M.M.Nishonov, R.Yarmukhamedov

Calculation of the Nuclear Vertex Constant (Asymptotic Normalization Coefficient) for the Virtual Decay 6Li → α + d on the Basis of the Three-Body Model and Application of the Result in Describing the Astrophysical Nuclear Reaction d(α, γ)6Li at Ultralow Energies

NUCLEAR REACTIONS 2H(α, γ), E=0-600 keV; calculated nuclear vertex constant, astrophysical S-factor. Three-body model.

doi: 10.1134/S1063778806030069
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2003TI01      Nucl.Phys. A713, 217 (2003)

N.K.Timofeyuk, S.B.Igamov

Direct capture contribution to the 11C(p, γ)12N reaction at astrophysical energies

NUCLEAR REACTIONS 11C(p, γ), E(cm)=0-1.5 MeV; calculated overlap integral, local potential, astrophysical S-factor, direct capture contribution.

doi: 10.1016/S0375-9474(02)01292-7
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2000IG03      Nucl.Phys. A673, 509 (2000)

S.B.Igamov, R.Yarmukhamedov

Triple-Differential Cross Section of the 208Pb(6Li, αd)208Pb Coulomb Breakup and Astrophysical S-Factor of the d(α, γ)6Li Reaction at Extremely Low Energies

NUCLEAR REACTIONS 208Pb(6Li, dα), E=156 MeV; calculated σ(E, θ). 2H(α, γ), E < 250 MeV; calculated astrophysical S-factors. Three-body Coulomb effects, nuclear vertex constant. Astrophysical implications discussed.

doi: 10.1016/S0375-9474(00)00132-9
Citations: PlumX Metrics


1997IG01      Yad.Fiz. 60, No 7, 1252 (1997); Phys.Atomic Nuclei 60, 1126 (1997)

S.B.Igamov, T.M.Tursunmuratov, R.Yarmukhamedov

Nuclear Vertex Constants for the Virtual-Disintegration Reactions 7Li → α + t and 7Be → α + 3He and for the Direct-Radiative-Capture Processes T(α, γ)7Li and 3He(α, γ)7Be at Astrophysical Energies

NUCLEAR REACTIONS, ICPND 3H, 3He(γ, γ), E ≤ 600 keV; analyzed astrophysical S-factor vs E. α-cluster model based 7Li, 7Be virtual decay vertex constants.


1997IG03      Yad.Fiz. 60, No 12, 2194 (1997); Phys.Atomic Nuclei 60, 2012 (1997)

S.B.Igamov, B.F.Irgaziev, R.Yarmukhamedov

Three-Body Coulomb Effects in the Coulomb Breakup of Light Nuclei Into Two Fragments in the Field of a Heavy Multiply Charged Ion

NUCLEAR REACTIONS 208Pb(6Li, dα), E=156 MeV; calculated σ(E(dα), θ); deduced E1 transition role. Coulomb breakup, three-body effects.


1995IG06      Yad.Fiz. 58, No 8, 1400 (1995); Phys.Atomic Nuclei 58, 1317 (1995)

S.B.Igamov, R.Yarmukhamedov

Analysis of the Nuclear Astrophysical Reaction α + d → 6Li + γ

NUCLEAR REACTIONS, ICPND 2H(α, γ), E(cm)=0.0-0.4 MeV; calculated astrophysical S-factor vs E. 2H(α, γ), E(cm)=50-350 keV; calculated σ(E). Compound system virtual decay considered.


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Note: The following list of authors and aliases matches the search parameter S.B.Igamov: , S.B.IGAMOV