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NSR database version of April 26, 2024.

Search: Author = B.Irgaziev

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2024IR01 Chin.Phys.C 48, 045103 (2024)

B.F.Irgaziev, A.Kabir, J.-U.Nabi

Radiative capture of proton through the ¹⁴N(p, γ)¹⁵O reaction at low energy

NUCLEAR REACTIONS ¹⁴N(p, γ), E(cm)<1 MeV>; calculated partial components of the astrophysical S-factor for all possible electric and magnetic dipole transitions with a potential model to describe both non-resonant and resonant reactions in the channels where radiative capture occurs through electric transitions and R-matrix method. Comparison with available data.

doi: 10.1088/1674-1137/ad1b3c
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2022IR01 Nucl.Phys. A1021, 122422 (2022)

B.F.Irgaziev, A.Kabir, J.-U.Nabi

Application of ANCs for calculation of β⁺ decay of ¹⁷F nucleus

NUCLEAR STRUCTURE ¹⁷F, ¹⁷O; calculated values of the proton spectroscopic factor for ¹⁷F and the neutron one for ¹⁷O; deduced that these mirror nuclei have a pronounced single-particle structure.

doi: 10.1016/j.nuclphysa.2022.122422
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2022KA16 J.Phys.(London) G49, 075101 (2022)

A.Kabir, B.F.Irgaziev, J.-U.Nabi, S.Sagheer

Re-analysis of radiative capture ¹¹C(p, γ)¹²N at low energy

NUCLEAR REACTIONS ¹¹C(p, γ), E(cm)<0.8 MeV; analyzed available data; calculated S-factor within the framework of the modified potential model.

doi: 10.1088/1361-6471/ac6362
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2021IR01 Can.J.Phys. 99, 176 (2021)

B.F.Irgaziev, J.-U.Nabi, A.Kabir

Analysis of β⁺ decay of ¹³N nucleus using a modified one-particle approach

RADIOACTIVITY ¹³N(β⁺); analyzed available data on phase shifts, asymptotic normalization coefficients (ANCs) and spectroscopic factors; calculated wave functions, log ft, T_1/2.

doi: 10.1139/cjp-2020-0155
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2018IR01 Phys.Rev. C 98, 015803 (2018)

B.F.Irgaziev, Yu.V.Orlov

Resonance properties including asymptotic normalization coefficients deduced from phase-shift data without the effective-range function

NUCLEAR REACTIONS ³He(α, α'), E(cm)=0-7 MeV; ⁴He, ¹²C(α, α'), E(cm)=0-6 MeV; analyzed experimental data for phase-shifts and resonance energies using a new algorithm (Δ method) for the bound states ANC calculation; deduced asymptotic nuclear coefficients (ANCs). ^7,8Be, ¹⁶O; calculated resonances, widths of 5/2-, 7/2- states in ⁷Be, 0+ and 2+ states in ⁸Be, and 0+, 1-, 2+, and 3- states in ¹⁶O. Comparison with experimental values and other theoretical predictions. Possible application for (α, γ) reactions in nuclear astrophysics.

doi: 10.1103/PhysRevC.98.015803
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2017OR03 Phys.Rev. C 96, 025809 (2017)

Yu.V.Orlov, B.F.Irgaziev, J.-U.Nabi

Algorithm for calculations of asymptotic nuclear coefficients using phase-shift data for charged-particle scattering

NUCLEAR REACTIONS ¹²C(α, α)¹⁶O*, E<5 MeV; ⁴He(³He, ³He)⁷Be*, E<5 MeV; analyzed elastic phase-shift data with binding energies used as input; deduced asymptotic normalization coefficients (ANC), nuclear vertex constants, and scattering amplitude residues using effective-range expansion (ERE) theory (Delta-method), valid for large charges. Relevance to element creation in supernova explosions, and in the theory using Feynman diagrams to describe the amplitude of the direct nuclear reactions.

doi: 10.1103/PhysRevC.96.025809
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2016OR01 Phys.Rev. C 93, 014612 (2016), Erratum Phys.Rev. C 93, 059901 (2016)

Yu.V.Orlov, B.F.Irgaziev, L.I.Nikitina

Asymptotic normalization coefficients of resonant and bound states from the phase shifts for αα and α¹²C scattering

NUCLEAR REACTIONS ⁴He(α, α'), E(cm)<25 MeV; ¹²C(α, α'), E(cm)<6.0 MeV; analyzed fits of phase shifts of elastic scattering, analytical continuation of renormalized scattering amplitude. ⁸Be, ¹⁶O; calculated energies of levels and asymptotic normalization coefficients (ANC) for first 0+ and 2+ resonances in ⁸Be, 0+, 1-, and 2+ bound states and 1- and 3- resonances in ¹⁶O. S-matrix pole (SMP) and effective-range methods.

doi: 10.1103/PhysRevC.93.014612
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2016WE02 Phys.Rev. C 93, 035803 (2016); Pub Note Phys.Rev. C 93, 039902 (2016)

Q.-G.Wen, C.-B.Li, S.-H.Zhou, B.Irgaziev, Y.-Y.Fu, C.Spitaleri, M.La Cognata, J.Zhou, Q.-Y.Meng, L.Lamia, M.Lattuada

Experimental study to explore the ⁸Be-induced nuclear reaction via the Trojan horse method

NUCLEAR REACTIONS ⁹Be(d, nα)⁶Li, E=22.4 MeV; measured α and ⁶Li spectra, E_α versus θ_α plots at HI-13 accelerator of CIAE-Beijing; deduced experimental neutron momentum distribution inside ⁹Be. Deuterated polyethylene target CD₂. Trojan horse method for a 3-body reaction with assumption of ⁹Be as ⁸Be+n cluster structure. Comparison with theoretical calculations treating ⁸Be-n interaction with a Woods-Saxon potential.

doi: 10.1103/PhysRevC.93.035803
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2015IR01 Phys.Rev. C 91, 024002 (2015)

B.F.Irgaziev, Yu.V.Orlov

Resonance-state properties from a phase shift analysis with the S-matrix pole method and the effective-range method

NUCLEAR REACTIONS ⁴He(n, n), (p, p), E(cm)=0-16 MeV; ¹²C(α, α), E=2-7 MeV; analyzed experimental phase-shift data and effective-range functions by the S-matrix pole method and effective-range method. ⁵He, ⁵Li, ¹⁶O; deduced asymptotic normalization coefficients (ANCs), levels, J, π, energies and widths of resonance states. Possible application to reaction rates at low energy collisions.

doi: 10.1103/PhysRevC.91.024002
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2015SE08 Phys.Rev. C 91, 065803 (2015)

M.L.Sergi, C.Spitaleri, M.La Cognata, L.Lamia, R.G.Pizzone, G.G.Rapisarda, X.D.Tang, B.Bucher, M.Couder, P.Davies, R.deBoer, X.Fang, L.Lamm, C.Ma, M.Notani, S.O'Brien, D.Roberson, W.Tan, M.Wiescher, B.Irgaziev, A.Mukhamedzhanov, J.Mrazek, V.Kroha

Improvement of the high-accuracy ¹⁷O(p, α)¹⁴N reaction-rate measurement via the Trojan Horse method for application to ¹⁷O nucleosynthesis

NUCLEAR REACTIONS ²H(¹⁷O, α¹⁴N)n, E=41, 43.5 MeV; measured particle spectra, (¹⁴N)α-coin at LNS-Catania and NSL-Notre Dame accelerator facilities; deduced Q-value spectra, yields as function of ¹⁴N and α emission angles, E(¹⁴N-α) versus E(α-n) plots, neutron momentum distributions, (¹⁴N)α-coincidence yields for different neutron momentum ranges, differential σ(E) of the Trojan-Horse reaction. ¹⁸F; deduced parameters for the two resonance levels, resonance strengths for the 65-keV resonance. ¹⁷O(p, α)¹⁴N; deduced reaction rates via Trojan Horse Method (THM). ¹⁸F; compiled resonance energies, J, π, Γ_p, Γ_α, Γ_γ for 24 resonances from -3.12 keV to 1684.5 keV. Relevance to destruction of ¹⁷O and the formation of ¹⁸F in stellar sites.

doi: 10.1103/PhysRevC.91.065803
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2014SP03 Phys.Rev. C 90, 035801 (2014)

C.Spitaleri, L.Lamia, S.M.R.Puglia, S.Romano, M.La Cognata, V.Crucilla, R.G.Pizzone, G.G.Rapisarda, M.L.Sergi, M.Gimenez Del Santo, N.Carlin, M.G.Munhoz, F.A.Souza, A.Szanto de Toledo, A.Tumino, B.Irgaziev, A.Mukhamedzhanov, G.Tabacaru, V.Burjan, V.Kroha, Z.Hons, J.Mrazek, S.-H.Zhou, C.Li, Q.Wen, Y.Wakabayashi, H.Yamaguchi, E.Somorjai

Measurement of the 10 keV resonance in the ¹⁰B(p, α₀)⁷Be reaction via the Trojan Horse method

NUCLEAR REACTIONS ²H(¹⁰B, α⁷Be), E=24.5 MeV; measured particle spectra by ΔE-E method using ionization chambers and position-sensitive detectors at LNS-Catania accelerator facility; analyzed data by Trojan Horse method (THM); deduced E_α-Be and E_α-n two-dimensional plots, experimental momentum distribution and its comparison with DWBA and PWIA calculations, THM bare nucleus astrophysical S(E) factors using R-matrix formalism for 5-100 keV resonances in ¹¹C, dominated by 10-keV resonance corresponding to 8699-keV, 5/2+ level in ¹¹C. ¹¹C; deduced widths of three resonances.

doi: 10.1103/PhysRevC.90.035801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1765. Data from this article have been entered in the XUNDL database. For more information, click here.

2013IR01 Phys.Rev. C 87, 035804 (2013)

B.F.Irgaziev, V.B.Belyaev, J.-U.Nabi

Three-body calculation of the rate of the reaction p+p+e → d+ν_e in the Sun

NUCLEAR REACTIONS ¹H(p, ν), E<20 keV; calculated reaction rate and astrophysical S factor for p+p+e^- to d+ν_e reaction in sun using expansion of three-body wave function of p+e^-+p system in the initial state on hyperharmonic functions. Comparison with experimental data, and previous calculations.

doi: 10.1103/PhysRevC.87.035804
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2012LA08 Phys.Rev. C 85, 025805 (2012)

L.Lamia, M.La Cognata, C.Spitaleri, B.Irgaziev, R.G.Pizzone

Influence of the d-state component of the deuteron wave function on the application of the Trojan horse method

NUCLEAR REACTIONS ²H(¹¹B, α⁸Be), (¹⁸O, α¹⁵N), E not given; calculated neutron momentum distribution. ¹¹Be, ¹⁸O(p, α), E not given; analyzed discrepancy ϵ. Trojan horse method. Contribution of s-wave and d-wave components in deuteron wave function. Comparison with experimental data.

doi: 10.1103/PhysRevC.85.025805
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2011BL06 Bull.Rus.Acad.Sci.Phys. 75, 505 (2011); Izv.Akad.Nauk RAS, Ser.Fiz 75, 541 (2011)

L.D.Blokhintsev, V.O.Eremenko, B.F.Irgaziev, Yu.V.Orlov

Calculating the characteristics of neutron-deuteron and proton-deuteron systems in a two-body potential model

NUCLEAR STRUCTURE ³H, ³He; calculated binding energy, asymptotic normalization coefficients. Two-body potential model.

doi: 10.3103/S1062873811040095
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2011IR01 Bull.Rus.Acad.Sci.Phys. 75, 511 (2011); Izv.Akad.Nauk RAS, Ser.Fiz 75, 547 (2011)

B.F.Irgaziev, A.M.Mukhamedzhanov, Yu.V.Orlov, L.D.Blokhintsev

Extracting the complex energy of broad resonances by the S-matrix pole method

NUCLEAR REACTIONS ¹²C(α, α), ²⁶Mg(n, n), E not given; calculated energies and width for p-wave resonances, phase shifts. R-matrix and S-matrix pole fitting methods.

doi: 10.3103/S1062873811040204
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2011IR02 Phys.Rev. C 84, 065809 (2011)

B.F.Irgaziev, J.-U.Nabi, D.Khan

Coulomb breakup of ⁶Li into α + d in the field of a ²⁰⁸Pb ion

NUCLEAR REACTIONS ²⁰⁸Pb(⁶Li, dα), E=156 MeV; calculated astrophysical S factor, asymptotic normalization coefficient (ANC), triple differential σ(θ), nuclear distortion contribution using semiclassical and diffraction models with two-body approach and Woods-Saxon potential. Comparison with experimental data.

doi: 10.1103/PhysRevC.84.065809
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2011MU08 Phys.Rev. C 83, 055805 (2011)

A.M.Mukhamedzhanov, L.D.Blokhintsev, B.F.Irgaziev

Reexamination of the astrophysical S factor for the α+d → ⁶Li+γ reaction

NUCLEAR REACTIONS ²H(α, ⁶Li); analyzed α-d elastic scattering phase shift; deduced asymptotic normalization coefficient (ANC) for the decay of ⁶Li into α+d, reaction rates and astrophysical factor S₂₄(E) for the radiative capture process of α+d to ⁶Li+γ using α-d potential model.

doi: 10.1103/PhysRevC.83.055805
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2010LA12 Nucl.Phys. A834, 658c (2010)

M.La Cognata, C.Spitaleri, A.Mukhamedzhanov, V.Goldberg, B.Irgaziev, L.Lamia, R.G.Pizzone, M.L.Sergi, R.E.Tribble

DWBA momentum distribution and its effect on THM

NUCLEAR REACTIONS ²H(¹⁸O, α¹⁵N), E(cm)≈5.4 MeV; calculated wave function momentum distribution using DWBA. Comparison with data.

doi: 10.1016/j.nuclphysa.2010.01.116
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2010LA19 J.Phys.:Conf.Ser. 202, 012019 (2010)

M.La Cognata, C.Spitaleri, A.Mukhamedzhanov, R.E.Tribble, T.Al-Abdullah, A.Banu, S.Cherubini, A.Coc, V.Crucilla, V.Goldberg, M.Gulino, B.Irgaziev, G.G.Kiss, L.Lamia, J.Mrazek, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, G.Tabacaru, L.Trache, W.Trzaska, S.Tudisco, A.Tumino

First measurement of the ¹⁸O(p, α)¹⁵N cross section at astrophysical energies

NUCLEAR REACTIONS ²H(¹⁸O, α¹⁵N), E=54 MeV; measured Eα, Iα(θ), E(particle), I(particle, θ); deduced dσ, resonances. ¹⁸O(p, α), E=0-8 keV; calculated; deduced reaction rate, resonance strengths from ²H(¹⁸O, α¹⁵N) using Trojan Horse method.

doi: 10.1088/1742-6596/202/1/012019
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2010MU03 Phys.Rev. C 81, 054314 (2010)

A.M.Mukhamedzhanov, B.F.Irgaziev, V.Z.Goldberg, Yu.V.Orlov, I.Qazi

Bound, virtual, and resonance S-matrix poles from the Schrodinger equation

NUCLEAR STRUCTURE ¹¹Be, ¹¹N, ¹⁴N, ¹⁵F; calculated S-matrix pole parameters for lowest 1/2+, 1/2- and 5/2+ states in ¹¹Be and ¹¹N, 1/2+ resonance state in ¹¹N, 1+ ground state of ¹⁴N, 1/2+ and 5/2+ resonance states in ¹⁵F using the potential S-matrix pole method based on numerical solution to Schrodinger equation. Comparison of S-matrix and R-matrix methods for resonances in ¹⁴O+p and ²⁶Mg+n systems.

doi: 10.1103/PhysRevC.81.054314
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2010SE11 Nucl.Phys. A834, 676c (2010)

M.L.Sergi, C.Spitaleri, A.Coc, A.Mukhamedzhanov, S.V.Burjan, M.Gulino, F.Hammache, Z.Hons, B.Irgaziev, G.G.Kiss, V.Kroha, M.La Cognata, L.Lamia, R.G.Pizzone, N.de Sereville, E.Somorjai

The 65 keV resonance in the ¹⁷O(p, α)¹⁴N thermonuclear reaction

NUCLEAR REACTIONS ²H(¹⁷O, α¹⁴N), E=41 MeV; measured σ, σ(θ). ¹⁷O(p, α), E=0-0.7 MeV; deduced σ(θ). ¹⁸F; deduced levels using Trojan Horse Method.

doi: 10.1016/j.nuclphysa.2010.01.122
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2010SE13 Phys.Rev. C 82, 032801 (2010)

M.L.Sergi, C.Spitaleri, M.La Cognata, A.Coc, A.Mukhamedzhanov, S.V.Burjan, S.Cherubini, V.Crucilla, M.Gulino, F.Hammache, Z.Hons, B.Irgaziev, G.G.Kiss, V.Kroha, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, N.de Sereville, E.Somorjai, S.Tudisco, A.Tumino

New high accuracy measurement of the ¹⁷O(p, α)¹⁴N reaction rate at astrophysical temperatures

NUCLEAR REACTIONS ²H(¹⁷O, α¹⁴N), E=41 MeV; measured ¹⁴N spectrum, σ(θ), momentum distribution and differential σ for resonances above the ¹⁸F proton threshold. ¹⁸F; deduced resonances and levels. Comparison of experimental momentum distribution with plane-wave impulse approximation (PWIA) and distorted-wave Born approximation (DWBA) calculations. ¹⁷O(p, α)¹⁴N; deduced reaction rates of astrophysical relevance.

doi: 10.1103/PhysRevC.82.032801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1864. Data from this article have been entered in the XUNDL database. For more information, click here.

2010SE21 J.Phys.:Conf.Ser. 202, 012021 (2010)

M.L.Sergi, C.Spitaleri, A.Coc, A.Mukhamedzhanov, V.Burjan, S.Cherubini, V.Crucilla, M.Gulino, F.Hammache, V.Z.Hons, B.Irgaziev, G.Kiss, V.Kroha, M.La Cognata, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, N.de Sereville, E.Somorjai, S.Tudisco, A.Tumino

Indirect measurement of ¹⁷O(p, α)¹⁴N cross section at ultra-low energies

NUCLEAR REACTIONS ²H(¹⁷O, α¹⁴N), E=41 MeV; measured E(particle), I(particle, θ) using position sensitive detectors and ionization chambers; deduced neutron momentum distribution. ¹⁷O(p, α), E(cm)=0-0.7 MeV; deduced σ(θ) from ²H(¹⁷O, α¹⁴N), E=41 MeV using Trojan Horse method in PWIA approach.

doi: 10.1088/1742-6596/202/1/012021
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2009PI12 Phys.Rev. C 80, 025807 (2009)

R.G.Pizzone, C.Spitaleri, A.M.Mukhamedzhanov, L.D.Blokhintsev, C.A.Bertulani, B.F.Irgaziev, M.La Cognata, L.Lamia, S.Romano

Effects of distortion of the intercluster motion in ²H, ³He, ³H, ⁶Li, and ⁹Be on Trojan horse applications

NUCLEAR REACTIONS ²H(p, 2p), E=5, 6 MeV; ²H(t, pt), E=35.5 MeV; ²H(³He, p³He), E=17 MeV; ²H(⁶Li, ³Heα), E=25 MeV; ²H(⁹Be, α⁶Li), E=22 MeV; ²H(¹⁰B, α⁷Be), (¹¹B, α⁸Be), E=27 MeV; ²H(⁷Li, 2α), E=20 MeV; ²H(¹⁵N, α¹²C), E=60 MeV; ²H(¹⁸O, α¹⁵N), E=54 MeV; ³H(³He, d³He), (³He, p³He), E=65 MeV; ³H(³He, 2d), E=50, 65, 78 MeV; ³H(³He, pt), E=78 MeV; ³H(d, 2d), E=35 MeV; ³H(p, 2p), (p, pd), E=45.6 MeV; ³He(p, pd), E=65, 85, 100, 590 MeV; ³He(d, pt), E=17, 35, 52 MeV; ³He(d, p³He), E=18 MeV; ⁶Li(⁶Li, 2α)⁴He, E=2.1-44 MeV; ⁷Li(³He, 2α), E=11, 12, 33 MeV; ⁹Be(p, pα)⁵He, E=47, 55, 57, 160 MeV; ⁹Be(³He, 2α)⁴He, E=2.8, 3, 4 MeV; ⁹Be(p, dα), E=30 MeV; ⁹Be(⁷Li, α⁷Li), E=52 MeV; ⁹Be(α, 2α), E=140 MeV; calculated widths (FWHM) of momentum distributions of the spectator particles using the Trojan Horse method and compared with the experimental data.

doi: 10.1103/PhysRevC.80.025807
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2008BL07 Bull.Rus.Acad.Sci.Phys. 72, 295 (2008); Izv.Akad.Nauk RAS, Ser.Fiz. 72, 321 (2008)

L.D.Blokhintsev, B.F.Irgaziev, A.M.Mukhamedzhanov, A.N.Safronov, A.A.Safronov

Determination of the nuclear vertex constants for the ⁷Be <-> ³He⁴He vertex using the N/D equations and calculation of the astrophysical S factor for the ⁴He(³He, γ)⁷Be reaction

doi: 10.3103/S1062873808030064
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2008BL11 Bull.Rus.Acad.Sci.Phys. 72, 811 (2008)

L.D.Blokhintsev, V.O.Eremenko, B.F.Irgaziev, Yu.V.Orlov

Characteristics of scattering of Λ hyperons from nuclei within the potential model

NUCLEAR STRUCTURE ⁷He, ^6,7,8,9Be, ^6,7,8Li, ¹¹C, ¹⁴N, ¹⁵O, ³⁹Ca, ⁸⁸Zr, ²⁰⁷Pb; calculated scattering lengths, phase shifts, and effective radii for low energy Λ scattering using Woods-Saxon, Hulthen, and Yukawa potentials.

doi: 10.3103/S106287380806021X
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2008LA13 Phys.Rev.Lett. 101, 152501 (2008)

M.La Cognata, C.Spitaleri, A.M.Mukhamedzhanov, B.Irgaziev, R.E.Tribble, A.Banu, S.Cherubini, A.Coc, V.Crucilla, V.Z.Goldberg, M.Gulino, G.G.Kiss, L.Lamia, J.Mrazek, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, G.Tabacaru, L.Trache, W.Trzaska, A.Tumino

Measurement of the 20 and 90 keV Resonances in the ¹⁸O(p, α)¹⁵N Reaction via the Trojan Horse Method

NUCLEAR REACTIONS ²H(¹⁸O, nα), E=54 MeV; measured σ(θ, E). ¹⁸O(p, α), E=0-250 keV; deduced σ(θ). ¹⁹F; deduced low lying resonance strengths. Discussed astrophysical implications.

doi: 10.1103/PhysRevLett.101.152501
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1713. Data from this article have been entered in the XUNDL database. For more information, click here.

2008MU07 J.Phys.(London) G35, 014016 (2008)

A.M.Mukhamedzhanov, L.D.Blokhintsev, B.F.Irgaziev, A.S.Kadyrov, M.La Cognata, C.Spitaleri, R.E.Tribble

Trojan Horse as an indirect technique in nuclear astrophysics

NUCLEAR REACTIONS ¹⁵N(p, α), E=0-0.85 MeV; calculated astrophysical S-factor. Comparisons with experimental data. Trojan Horse Method.

doi: 10.1088/0954-3899/35/1/014016
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2007BL11 Bull.Rus.Acad.Sci.Phys. 71, 408 (2007); Izv.Akad.Nauk RAS, Ser.Fiz. 71, 423 (2007)

L.D.Blokhintsev, V.O.Eremenko, B.F.Irgaziev, Yu.V.Orlov

Vertex Constants (Asymptotic Normalization Coefficients) and Mean-Square Radii, of Hypernuclei in the Potential Model

NUCLEAR STRUCTURE A=7-208; calculated vertex constants, asymptotic normalization coefficients and mean-square radii for a number of hypernuclei using the potential approach.

doi: 10.3103/S1062873807030215
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2007LA37 Phys.Rev. C 76, 065804 (2007)

M.La Cognata, S.Romano, C.Spitaleri, S.Cherubini, V.Crucilla, M.Gulino, L.Lamia, R.G.Pizzone, A.Tumino, R.Tribble, C.Fu, V.Z.Goldberg, A.M.Mukhamedzhanov, D.Schmidt, G.Tabacaru, L.Trache, B.F.Irgaziev

Astrophysical S(E) factor of the ¹⁵N(p, α)¹²C reaction at sub-Coulomb energies via the Trojan horse method

NUCLEAR REACTIONS ²H(¹⁵N, nα), E=60 MeV; measured ¹²C energies, particle coincidences, momentum. ¹⁵N(p, α)¹²C, E(cm)=19.2-576.0 MeV; deduced angular distributions, excitation functions, astrophysical S-factors using Trojan horse method.

doi: 10.1103/PhysRevC.76.065804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1788.

2007MU10 Nucl.Phys. A787, 321c (2007)

A.M.Mukhamedzhanov, L.D.Blokhintsev, S.Brown, V.Burjan, S.Cherubini, V.Z.Goldberg, M.Gulino, B.F.Irgaziev, E.Johnson, K.Kemper, V.Kroha, M.La Cognata, L.Lamia, A.Momotyuk, R.G.Pizzone, B.Roeder, G.Rogachev, S.Romano, C.Spitaleri, R.E.Tribble, A.Tumino

Indirect Techniques in Nuclear Astrophysics. Asymptotic Normalization Coefficient and Trojan Horse

NUCLEAR REACTIONS ¹³C(α, n), E=0-0.9 MeV; calculated astrophysical S-factor. Asymptotic normalization coefficient method. Comparison with data. ⁶Li(d, α), ⁷Li(p, α), E=0-800 keV; calculated astrophysical S-factor. Trojan horse method.

doi: 10.1016/j.nuclphysa.2006.12.051
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2006IR01 Bull.Rus.Acad.Sci.Phys. 70, 254 (2006)

B.F.Irgaziev, Yu.V.Orlov

Virtual state in configuration space

NUCLEAR STRUCTURE ³H; calculated virtual state energy.

2006IR02 Bull.Rus.Acad.Sci.Phys. 70, 257 (2006)

B.F.Irgaziev, L.I.Nikitina, Yu.V.Orlov

Nucleon-deuteron system at low energies within a two-body potential model

NUCLEAR STRUCTURE ³H, ³He; calculated binding energies, effective radius functions.

2006MU08 Phys.Rev. C 73, 035806 (2006)

A.M.Mukhamedzhanov, P.Bem, V.Burjan, C.A.Gagliardi, B.F.Irgaziev, V.Kroha, J.Novak, S.Piskor, E.Simeckova, R.E.Tribble, F.Vesely, J.Vincour

Asymptotic normalization coefficients from the ²⁰Ne(³He, d)²¹Na reaction and astrophysical factor for ²⁰Ne(p, γ)²¹Na

NUCLEAR REACTIONS ²⁰Ne(³He, d), E=25.83 MeV; measured deuteron spectra, σ(E, θ); deduced asymptotic normalization coefficients. ²⁰Ne(p, γ), E=0-1200 keV; deduced astrophysical S-factor.

doi: 10.1103/PhysRevC.73.035806
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2006MU15 Eur.Phys.J. A 27, Supplement 1, 205 (2006)

A.M.Mukhamedzhanov, L.D.Blokhintsev, B.A.Brown, V.Burjan, S.Cherubini, C.A.Gagliardi, B.F.Irgaziev, V.Kroha, F.M.Nunes, F.Pirlepesov, R.G.Pizzone, S.Romano, C.Spitaleri, X.D.Tang, L.Trache, R.E.Tribble, A.Tumino

Indirect techniques in nuclear astrophysics: Asymptotic Normalization Coefficient and Trojan Horse

NUCLEAR REACTIONS ¹⁴N(³He, d), E=26.3 MeV; measured σ(θ). ¹⁴N(p, γ), E ≈ 100-600 keV; deduced astrophysical S-factor. ¹¹C, ¹³N(p, γ), E not given; analyzed resonant and nonresonant amplitudes. Asymptotic normalization coefficient and Trojan horse techniques discussed.

doi: 10.1140/epja/i2006-08-032-7
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2005AL07 Phys.Rev. C 71, 024605 (2005)

E.O.Alt, B.F.Irgaziev, A.M.Mukhamedzhanov

Three-body Coulomb interaction effects in the final state of the ²⁰⁸Pb(⁸B, ⁷Be p)²⁰⁸Pb Coulomb breakup reaction

NUCLEAR REACTIONS ²⁰⁸Pb(⁸B, p⁷Be), E=46.5, 83 MeV/nucleon; calculated σ(E, θ), post-decay acceleration effect.

doi: 10.1103/PhysRevC.71.024605
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2005MU27 J.Phys.(London) G31, S1413 (2005)

A.M.Mukhamedzhanov, E.O.Alt, L.D.Blokhintsev, S.Cherubini, B.F.Irgaziev, A.S.Kadyrov, D.Miljanic, A.Musumarra, M.G.Pellegriti, F.Pirlepesov, C.Rolfs, S.Romano, C.Spitaleri, N.K.Timofeyuk, R.E.Tribble, A.Tumino

Few-body problems in nuclear astrophysics

doi: 10.1088/0954-3899/31/10/005
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2004NU01 Nucl.Phys. A736, 255 (2004)

F.M.Nunes, A.M.Mukhamedzhanov, C.C.Rosa, B.Irgaziev

Insight into continuum couplings

NUCLEAR REACTIONS ⁵⁸Ni(⁸B, p⁷Be), E=low; calculated continuum coupling matrix elements. Continuum discretized coupled channels method.

doi: 10.1016/j.nuclphysa.2004.03.035
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2004TA15 Phys.Rev. C 69, 055807 (2004)

X.Tang, A.Azhari, C.Fu, C.A.Gagliardi, A.M.Mukhamedzhanov, F.Pirlepesov, L.Trache, R.E.Tribble, V.Burjan, V.Kroha, F.Carstoiu, B.F.Irgaziev

Determination of the direct capture contribution for ¹³N(p, γ)¹⁴O from the ¹⁴O → ¹³N + p asymptotic normalization coefficient

NUCLEAR REACTIONS ¹⁴N(¹³N, ¹⁴O), E=11.8 MeV/nucleon; measured σ(θ); deduced asymptotic normalization coefficient. ¹²C, ¹⁴N(¹³N, ¹³N), E=11.8 MeV/nucleon; measured elastic σ(θ). ¹³N(p, γ), E=low; deduced astrophysical S-factor, reaction rates.

doi: 10.1103/PhysRevC.69.055807
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1490.

2003AL07 Phys.Rev.Lett. 90, 122701 (2003)

E.O.Alt, B.F.Irgaziev, A.M.Mukhamedzhanov

Final State Three-Body Coulomb Effects in the ²⁰⁸Pb(⁸B, ⁷Bep)²⁰⁸Pb Coulomb Breakup Reaction

NUCLEAR REACTIONS ²⁰⁸Pb(⁸B, p⁷Be), E=46.5, 83 MeV/nucleon; calculated Coulomb breakup σ(E, θ), final state three-body effects.

doi: 10.1103/PhysRevLett.90.122701
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2003IR01 Yad.Fiz. 66, 713 (2003); Phys.Atomic Nuclei 66, 684 (2003)

B.F.Irgaziev, Sh.Kalandarov, A.M.Mukhamedzhanov

Coulomb Breakup of Light Nuclei in the Field of a Heavy Ion at Relativistic Collision Energies

NUCLEAR REACTIONS ²⁰⁸Pb(⁸B, p⁷Be), E=46.5, 254 MeV/nucleon; calculated Coulomb breakup σ vs relative energy. Time-dependent perturbation theory, comparison with data.

doi: 10.1134/1.1575567
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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.

1996IR01 Yad.Fiz. 59, No 11, 1971 (1996); Phys.Atomic Nuclei 59, 1899 (1996)

B.F.Irgaziev, Kh.T.Ergashbaev

Coulomb Breakup of ⁶Li on a ²⁰⁸Pb Nucleus Through a Resonance

NUCLEAR REACTIONS ²⁰⁸Pb(⁶Li, dα), E=156 MeV; analyzed σ(θ(αd), E(αd), θ(f)). Projectile Coulomb dissociation through a resonance.

1995AL28 Yad.Fiz. 58, No 11, 1967 (1995); Phys.Atomic Nuclei 58, 1860 (1995)

E.O.Alt, B.F.Irgaziev, A.T.Muminov, A.M.Mukhamedzhanov

Effect of Three-Body Coulomb Interactions on the Breakup of Light Nuclei in the Field of a Heavy Ion: An asymptotic estimate

NUCLEAR REACTIONS ²⁰⁸Pb, ⁴⁰Ca(⁶Li, dα), (⁷Li, tα), ²⁰⁸Pb(¹⁶O, α¹²C), E=100-500 MeV; calculated differential σ ratio; deduced three-body Coulomb interactions role. Quasielastic breakup.

1993IR02 Yad.Fiz. 56, No 7, 71 (1993); Phys.Atomic Nuclei 56, 896 (1993)

B.F.Irgaziev, A.M.Mukhamedzhanov, A.T.Muminov, E.O.Alt

Coulomb Breakup of Fast Ions with Three-Body Coulomb Effects

NUCLEAR REACTIONS ²⁰⁸Pb(⁶Li, dα), E=156 MeV; calculated σ(θα, Eα, θd). Breakup reaction, Coulomb effects.

1986AV06 Yad.Fiz. 44, 942 (1986)

G.V.Avakov, B.F.Irgaziev, R.Yarmukhamedov

On Direct Mechanism of Three-Particle Photodisintegration of the ⁶Li Nucleus

NUCLEAR REACTIONS ⁶Li(γ, pd), E=60 MeV; calculated three-particle breakup σ(Ep, θp). Direct mechanism.

1983IR01 Fizika(Zagreb) 15, 147 (1983)

B.F.Irgaziev, M.M.Musakhanov, A.L.Zubarev, Z.Maric

Influence of the Energy Continuum of the NN Subsystem on the πd Elastic Scattering Length

NUCLEAR REACTIONS ²H(π, π), E=low; calculated scattering amplitude; deduced pion-deuteron scattering length.

1980BA55 Yad.Fiz. 32, 369 (1980); Sov.J.Nucl.Phys. 32, 191 (1980)

A.G.Baryshnikov, V.B.Belyaev, L.D.Blokhintsev, B.F.Irgaziev, Yu.V.Orlov

Scattering and Reactions in a 4-Nucleon System within the Framework of the K-Matrix Formalism

NUCLEAR REACTIONS ³He(p, p), E=9.75, 19.48, 30.6 MeV; ³H(p, p), E=13.6, 19.48 MeV; calculated σ(θ); deduced nucleon-nucleon interaction dependence. Multi-channel K-matrix formalism.

1972BE47 JINR-P4-6505 (1972)

V.B.Belyaev, A.L.Zubarev, B.F.Irgaziev

Factorization of the Pair Potential by the Bateman Modified Method in the Two- and Three-Body Problem

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Note: The following list of authors and aliases matches the search parameter B.Irgaziev: , B.F.IRGAZIEV