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NSR database version of April 27, 2024.

Search: Author = S.B.Igamov

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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
Citations: PlumX Metrics
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.

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
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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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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.

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