NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = A.M.Mukhamedzhanov Found 178 matches. Showing 1 to 100. [Next]2023BL01 Eur.Phys.J. A 59, 162 (2023) L.D.Blokhintsev, A.S.Kadyrov, A.M.Mukhamedzhanov, D.A.Savin Determination of asymptotic normalization coefficients for the channel 16O → α+12C. II. Excited states 16O(3-, 2+, 1- RADIOACTIVITY 16O(α); analyzed available data; deduced asymptotic normalization coefficients (ANC) for a virtual decay, the overall normalization of σ of peripheral radiative capture reactions.
doi: 10.1140/epja/s10050-023-01079-4
2023MU08 Eur.Phys.J. A 59, 43 (2023) Resonances in low-energy nuclear processes and nuclear astrophysics and asymptotic normalization coefficients: a review
doi: 10.1140/epja/s10050-023-00918-8
2023MU18 Phys.Rev. C 108, 054603 (2023) Proton 0.01 MeV resonance width and low-energy S factor of p + 10B
doi: 10.1103/PhysRevC.108.054603
2022BL07 Eur.Phys.J. A 58, 257 (2022) L.D.Blokhintsev, A.S.Kadyrov, A.M.Mukhamedzhanov, D.A.Savin Determination of asymptotic normalization coefficients for the channel 16O → α+12C: excited state 16O(0+; 6.05. MeV RADIOACTIVITY 16O(α); calculated asymptotic normalization coefficients (ANC) for for the virtual decay by approximating scattering data by the sum of polynomials in energy in the physical region and then extrapolated to the pole, and by solving the Schrodinger equation for the two-body α12 C potential, the parameters of which are selected from the requirement of the best description of the phase-shift analysis data at a fixed experimental binding energy.
doi: 10.1140/epja/s10050-022-00909-1
2022MU07 Eur.Phys.J. A 58, 29 (2022) A.M.Mukhamedzhanov, L.D.Blokhintsev Asymptotic normalization coefficients in nuclear reactions and nuclear astrophysics NUCLEAR REACTIONS 14C, 58Ni(d, p), E<60 MeV; 12,15N(p, γ), E(cm)<2 MeV; 2H(α, γ), E<1 MeV; analyzed available data; deduced asymptotic normalization coefficient (ANC), S-factors, astrophysical reaction rates.
doi: 10.1140/epja/s10050-021-00651-0
2022MU13 Eur.Phys.J. A 58, 71 (2022) Status of deep subbarrier 12C+12C fusion and advancing the Trojan horse method NUCLEAR REACTIONS 12C(12C, X), E not given; analyzed available data; deduced update of the current status of deep subbarrier fusion, the Trojan horse method.
doi: 10.1140/epja/s10050-022-00718-6
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
2021SP02 Eur.Phys.J. A 57, 20 (2021) C.Spitaleri, S.Typel, C.A.Bertulani, A.M.Mukhamedzhanov, T.Kajino, M.Lattuada, A.Cvetinovic, S.Messina, G.L.Guardo, N.Soic, M.Milin, S.S.Perrotta, C.Li, P.Colovic, G.D'Agata, D.Dell'Aquila, C.G.Fatuzzo, M.Gulino, S.Q.Hou, M.La Cognata, D.Lattuada, D.Nurkic, R.Popocovski, N.Skukan, S.Szilner, O.Trippella, M.Uroic, N.Vukman The 3He + 5He → α+α reaction below the Coulomb barrier via the Trojan Horse Method NUCLEAR REACTIONS 9Be(3He, 2α), E=4 MeV; 3He(5He, α), E(cm)<1 Mev; measured reaction products, Eα, Iα; deduced two α-particles σ(θ, E), σ(θ). Comparison with theoretical calculations, Trojan Horse Method (THM).
doi: 10.1140/epja/s10050-020-00324-4
2020BE07 Eur.Phys.J. A 56, 87 (2020) C.Beck, A.M.Mukhamedzhanov, X.Tang Status on 12C + 12C fusion at deep subbarrier energies: impact of resonances on astrophysical S* factors
doi: 10.1140/epja/s10050-020-00075-2
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
2020MU14 Eur.Phys.J. A 56, 233 (2020) A.M.Mukhamedzhanov, A.S.Kadyrov, D.Y.Pang Trojan horse method as an indirect approach to study resonant reactions in nuclear astrophysics
doi: 10.1140/epja/s10050-020-00214-9
2019BL07 Phys.Rev. C 100, 024627 (2019) L.D.Blokhintsev, A.S.Kadyrov, A.M.Mukhamedzhanov, D.A.Savin New method of analytic continuation of elastic-scattering data to the negative-energy region, and asymptotic normalization coefficients for 17O and 13C NUCLEAR REACTIONS 12C(n, n), E=0.050, 0.100, 0.157, 0.207, 0.257, 0.307, 0.357, 0.407, 0.457, 0.507, 0.530, 0.630, 0.730, 0.830, 0.930, 1.040 MeV; 16O(n, n), E=0.20, 0.30, 0.40, 0.51, 0.60, 0.698, 0.73, 1.00, 1.21, 1.50, 1.75, 1.833, 2.15, 2.250, 2.353, 3.000 MeV; calculated asymptotic normalization coefficients (ANC) for excited s-states in 13C and 17O populated by elastic n-scattering using a new method based on analytic approximation of the modulus-squared of the partial-wave scattering amplitude. Comparison with theoretical results from traditional effective-range function approach.
doi: 10.1103/PhysRevC.100.024627
2019BU17 Eur.Phys.J. A 55, 114 (2019) V.Burjan, Z.Hons, V.Kroha, J.Mrazek, S.Piskor, A.M.Mukhamedzhanov, L.Trache, R.E.Tribble, M.La Cognata, L.Lamia, R.G.Pizzone, S.Romano, C.Spitaleri, A.Tumino The determination of the astrophysical S-factor of the direct 18O(p, γ)19F capture by the ANC method
doi: 10.1140/epja/i2019-12801-8
2019MU05 Phys.Rev. C 99, 024311 (2019) Connection between asymptotic normalization coefficients and resonance widths of mirror states NUCLEAR STRUCTURE 13,15C, 13N, 15,17F, 18Ne, 17,18O; calculated radial wave function of resonance states and mirror bound states in terms of the Wronskians from the radial overlap functions and regular solutions of the two-body Schrodinger equation with the short-range interaction, ratio of the resonance widths and asymptotic normalization coefficients (ANCs) of the bound mirror states using Pinkston-Satchler equation, and R-matrix wave functions.
doi: 10.1103/PhysRevC.99.024311
2019MU11 Phys.Rev. C 99, 064618 (2019) A.M.Mukhamedzhanov, D.Y.Pang, A.S.Kadyrov Astrophysical factors of 12C + 12C fusion extracted using the Trojan horse method NUCLEAR REACTIONS 12C(14N, d)24Mg*, E(cm)=13.85 MeV; calculated differential σ(θ), and bin wave functions using DWBA. 12C(12C, p)23Na*, (12C, α)20Ne*, E=0.8-2.7 MeV; calculated astrophysical S factors using Trojan horse method. Comparison with calculations using plane-wave approximation. Relevance to carbon-carbon burning in stellar environments.
doi: 10.1103/PhysRevC.99.064618
2018BL01 Phys.Rev. C 97, 024602 (2018) L.D.Blokhintsev, A.S.Kadyrov, A.M.Mukhamedzhanov, D.A.Savin Extrapolation of scattering data to the negative-energy region. II. Applicability of effective range functions within an exactly solvable model NUCLEAR REACTIONS 2H, 12C(α, α'), E not given; investigated the applicability of the effective range function (ERF) and the Δ function for scattering data to the negative-energy region in order to determine asymptotic normalization coefficients (ANCs); search for the parameters of the excited 0+ state in α+12C system using exactly solvable model.
doi: 10.1103/PhysRevC.97.024602
2018BL06 Phys.Rev. C 98, 064610 (2018) L.D.Blokhintsev, A.S.Kadyrov, A.M.Mukhamedzhanov, D.A.Savin Extrapolation of scattering data to the negative-energy region. III. Application to the p - 16O system NUCLEAR REACTIONS 16O(p, p)17F, E(cm)=0-2 MeV; calculated asymptotic normalization coefficients (ANCs) for g.s. and excited state of 17F, polynomial approximation of Κ0(E), Κ2(E), Δ0(E), and Δ2(E) functions using the effective-range function (ERF) and the Δ methods. Comparison with experimental data.
doi: 10.1103/PhysRevC.98.064610
2018HA28 Astrophys.J. 862, 62 (2018) M.Hartos, C.A.Bertulani, Shubhchintak, A.M.Mukhamedzhanov, and S.Hou Impact of the 7Be(α, γ)11C Reaction on the Primordial Abundance of 7Li NUCLEAR REACTIONS 7Be(α, γ), E(cm)<3 MeV; calculated σ, reaction rates, S-factor. Comparison with available data.
doi: 10.3847/1538-4357/aac9c1
2018MU15 Phys.Rev. C 98, 044626 (2018) Three-body Faddeev equations in two-particle Alt-Grassberger-Sandhas form with distorted-wave-Born-approximation amplitudes as effective potentials NUCLEAR REACTIONS 208Pb(d, p), E=5 MeV; calculated angular distribution of protons populating the ground state of 209Pb using three-body Faddeev equations in two-particle Alt-Grassberger-Sandhas (AGS) form with DWBA amplitudes as effective potentials for analysis of (d, p) reactions.
doi: 10.1103/PhysRevC.98.044626
2017BL04 Phys.Rev. C 95, 044618 (2017) L.D.Blokhintsev, A.S.Kadyrov, A.M.Mukhamedzhanov, D.A.Savin Extrapolation of scattering data to the negative-energy region
doi: 10.1103/PhysRevC.95.044618
2017MU06 Phys.Rev. C 95, 024616 (2017) A.M.Mukhamedzhanov, Shubhchintak, C.A.Bertulani, T.V.Nhan Hao Internal and external radiative widths in the combined R-matrix and potential-model formalism NUCLEAR REACTIONS 11,12C, 12,14,15N, 16O(p, γ), E not given; calculated radiative widths of E1 transitions and asymptotic normalization coefficients (ANC) for the following proton resonances: 2.365 MeV, 1/2+ in 13N, 2.69 MeV, 1/2+ in 13O, 3.104 MeV, 1/2- and 3.857 MeV, 5/2- in 17F, 1.191 MeV, 2- in 12N, 12.44 MeV, 1- and 13.090 MeV, 1- in 16O, and 6.79 MeV, 3/2+ in 15O using R-matrix formalism and potential model. Comparison with experimental data.
doi: 10.1103/PhysRevC.95.024616
2017MU14 Phys.Rev. C 96, 024623 (2017) A.M.Mukhamedzhanov, Shubhchintak, C.A.Bertulani Subthreshold resonances and resonances in the R-matrix method for binary reactions and in the Trojan horse method NUCLEAR REACTIONS 13C(α, n)16O, E(cm)<1.1 MeV; calculated astrophysical S factor as a function of the α-13C relative kinetic energy using the R-matrix approach for resonances and Trojan horse method (THM) for S factor. Comparison with experimental data. Relevance to neutron generation in low-mass AGB stars.
doi: 10.1103/PhysRevC.96.024623
2017MU17 Phys.Rev. C 96, 045811 (2017) A.M.Mukhamedzhanov, G.V.Rogachev Radiative capture reactions via indirect methods NUCLEAR REACTIONS 12C(6Li, dγ)16O, E=9.33 MeV; calculated angular distribution of photons (pd(θ)) proceeding through the wings of two subthreshold resonances 1- and 2+, developed a formalism of resonant indirect radiative capture reactions for triple and double differential cross sections. 12C(α, γ)16O, E=300 keV; deduced low-energy astrophysical factors for E1 and E2 transitions for radiative capture through indirect methods, and compared with experimental data.
doi: 10.1103/PhysRevC.96.045811
2016MU04 Phys.Rev. C 93, 045805 (2016) A.M.Mukhamedzhanov, Shubhchintak, C.A.Bertulani Primordial α + d → 6Li + γ reaction and second lithium puzzle NUCLEAR REACTIONS 2H(α, γ)6Li, E=0.05-2 MeV; calculated angular distribution of photons at Big Bang energies of 70, 100, 200, and 400 keV using potential model, total cross sections for E1 and E2 transitions, astrophysical S24(E) factors, 6Li/7Li ratio. Comparison with LUNA collaboration data, and other theoretical calculations.
doi: 10.1103/PhysRevC.93.045805
2016SP03 Eur.Phys.J. A 52, 77 (2016) C.Spitaleri, M.La Cognata, L.Lamia, A.M.Mukhamedzhanov, R.G.Pizzone Nuclear astrophysics and the Trojan Horse Method NUCLEAR REACTIONS 2H(d, p), (d, n), E(cm)=0.003-3 MeV;6,7Li(p, α), E(cm)=0.01-1 MeV;13C(α, n), E(cm)=0-1.2 MeV;19F(p, α0), E(cm)=0-1.0 MeV; compiled S-factor data, fitting THM (Trojan Horse Method) and calculations. 6,7Li(p, α), T=0.001-10 GK; compiled, compared THM and NACRE reaction rates.
doi: 10.1140/epja/i2016-16077-2
2015AV01 Phys.Rev.Lett. 114, 071101 (2015) M.L.Avila, G.V.Rogachev, E.Koshchiy, L.T.Baby, J.Belarge, K.W.Kemper, A.N.Kuchera, A.M.Mukhamedzhanov, D.Santiago-Gonzalez, E.Uberseder Constraining the 6.05 MeV 0+ and 6.13 MeV 3- Cascade Transitions in the 12C(α, γ)16O Reaction Using the Asymptotic Normalization Coefficients NUCLEAR REACTIONS 6Li(12C, d), E=5, 7, 9 MeV; measured reaction products; deduced σ(θ), J, π, asymptotic normalization coefficients. Comparison with available data, DWBA calculations.
doi: 10.1103/PhysRevLett.114.071101
2015GR03 Phys.Rev. C 91, 014601 (2015) J.Grineviciute, L.Lamia, A.M.Mukhamedzhanov, C.Spitaleri, M.La Cognata Low-energy R-matrix fits for the 6Li (d, α) 4He S factor NUCLEAR REACTIONS 6Li(d, α)4He, E(cm)=0.01-1.1 MeV; analyzed 2+ subthreshold resonance energy, partial width of the α+α channel, bare astrophysical S(E) factor by single-, two-, and three-level R-matrix fits to the experimental data; deduced electron screening potential. Indirect Trojan horse method.
doi: 10.1103/PhysRevC.91.014601
2015LA12 Astrophys.J. 805, 128 (2015) M.La Cognata, S.Palmerini, C.Spitaleri, I.Indelicato, A.M.Mukhamedzhanov, I.Lombardo, O.Trippella Updated THM astrophysical factor of the 19F(p, α)16O reaction and direct data at astrophysical energies NUCLEAR REACTIONS 19F(p, α)16O, E(cm)=600-800 keV; analyzed available data; deduced renormalized data, form factor. Trojan Horse Method (THM).
doi: 10.1088/0004-637X/805/2/128
2015MU08 Phys.Rev. C 92, 014625 (2015) Asymptotic normalization coefficients and radiative widths NUCLEAR REACTIONS 11C, 12,14N, 16O(p, γ), E not given; analyzed resonance radiative widths (Γγ) for two transitions in 17F and one each in 12N, 13O and 15O using asymptotic normalization coefficients (ANCs). R-matrix method.
doi: 10.1103/PhysRevC.92.014625
2015PA10 Phys.Rev. C 91, 024611 (2015) D.Y.Pang, W.M.Dean, A.M.Mukhamedzhanov Optical model potential of A=3 projectiles for 1p-shell nuclei NUCLEAR REACTIONS 9Be, 10,11B, 12,13,14C, 14,15N, 16,17,18O(t, t), (3He, 3He), E=4-118.5 MeV; 6,7Li(t, t), (3He, 3He), E=3-44 MeV; analyzed σ(θ) for 142 sets of experimental data; deduced optical model parameters.
doi: 10.1103/PhysRevC.91.024611
2014MC03 Phys.Rev. C 89, 044605 (2014) M.McCleskey, A.M.Mukhamedzhanov, L.Trache, R.E.Tribble, A.Banu, V.Eremenko, V.Z.Goldberg, Y.-W.Lui, E.McCleskey, B.T.Roeder, A.Spiridon, F.Carstoiu, V.Burjan, Z.Hons, I.J.Thompson Determination of the asymptotic normalization coefficients for 14C + n ←→ 15C, the (+14)C(n, γ)15C reaction rate, and evaluation of a new method to determine spectroscopic factors NUCLEAR REACTIONS 13C(14C, 14C), (14C, 15C)12C, E=12 MeV/nucleon; 2H(14C, p)15C, E=11.7 MeV/nucleon; 14C(d, p), E=60 MeV; measured particle spectra, σ(θ) using MDM spectrometer at Texas A-M Cyclotron Institute. 15C; deduced levels, asymptotic normalization coefficient (ANC) and spectroscopic factors for g.s. and first excited state. 13C, 17O; population of g.s. in both and excited levels in 13C. DWBA analysis with Woods-Saxon and doublefolding (DF) potentials for 13C+14C reaction. FRESCO code and adiabatic distorted wave approximation (ADWA) used for analysis of σ(θ) data in 2H+14C reactions. 15C, 15F; analyzed mirror analogy for spectroscopic factors. Deuteron stripping theory. 14C(n, γ), E=10 keV-1 MeV; deduced astrophysical direct-capture rate σ(E) to g.s. and first excited state using RADCAP code and ANCs from the present work. Comparison with previous experimental results.
doi: 10.1103/PhysRevC.89.044605
2014MU10 Phys.Rev. C 90, 034604 (2014) A.M.Mukhamedzhanov, D.Y.Pang, C.A.Bertulani, A.S.Kadyrov Surface-integral formalism of deuteron stripping NUCLEAR REACTIONS 14C(d, p), E=23.4 MeV; 16O(d, p), E=36 MeV; calculated differential σ(θ), spectroscopic factors, neutron widths for deuteron stripping reactions to bound and resonant states. Distorted-wave Born approximation (DWBA), continuum-discretized coupled channels (CDCC), and surface-integral formalism.
doi: 10.1103/PhysRevC.90.034604
2014PA49 Phys.Rev. C 90, 044611 (2014) Asymptotic normalization coefficients and spectroscopic factors from deuteron stripping reactions NUCLEAR REACTIONS 14C(d, p), E=23.4, 60 MeV; 58Ni(d, p), E=10, 56 MeV; 116Sn(d, p), E=12.2, 79.2 MeV; analyzed experimental data to determine σ(θ), asymptotic normalization coefficients (ANCs), spectroscopic factors by using three methods: distorted wave born approximation (DWBA), adiabatic distorted wave approximation (ADWA), and continuum discretized coupled-channels (CDCC) models. Discussed flaw in the treatment of the nuclear interior in nuclear reaction theory for higher energies in deuteron stripping reactions with 58Ni and 116Sn targets.
doi: 10.1103/PhysRevC.90.044611
2014PI08 Few-Body Systems 55, 1001 (2014) R.G.Pizzone, C.Spitaleri, M.L.Sergi, L.Lamia, A.Tumino, C.A.Bertulani, L.Blokhintsev, V.Burjan, V.Kroha, M.La Cognata, J.Mrazek, A.M.Mukhamedzhanov, R.Sparta Trojan Horse Particle Invariance: An Extensive Study
doi: 10.1007/s00601-014-0829-z
2014TU03 Astrophys.J. 785, 96 (2014) A.Tumino, R.Sparta, C.Spitaleri, A.M.Mukhamedzhanov, S.Typel, R.G.Pizzone, E.Tognelli, S.Degl'Innocenti, V.Burjan, V.Kroha, Z.Hons, M.La Cognata, L.Lamia, J.Mrazek, S.Piskor, P.G.Prada Moroni, G.G.Rapisarda, S.Romano, M.L.Sergi New Determination of the 2H(d, p)3H and 2H(d, n)3He Reaction Rates at Astrophysical Energies NUCLEAR REACTIONS 2H(3He, pt), E=17 MeV;2H(3He, n3He), E=18 MeV; measured reaction products, Ep, Ip; deduced σ(θ), S-factors, reaction rates, inputs for FRANEC evolutionary code. Comparison with available data.
doi: 10.1088/0004-637X/785/2/96
2013BL08 Eur.Phys.J. A 49, 108 (2013) L.D.Blokhintsev, A.M.Mukhamedzhanov, R.Yarmukhamedov Anomalous asymptotics of radial overlap functions for bound systems of three or more particles NUCLEAR STRUCTURE 9Be, 16O, 20Ne; calculated radial overlaps of bound states nuclear wave functions treated as a system of three parts.
doi: 10.1140/epja/i2013-13108-6
2013GU02 Phys.Rev. C 87, 012801 (2013) M.Gulino, C.Spitaleri, X.D.Tang, G.L.Guardo, L.Lamia, S.Cherubini, B.Bucher, V.Burjan, M.Couder, P.Davies, R.deBoer, X.Fang, V.Z.Goldberg, Z.Hons, V.Kroha, L.Lamm, M.La Cognata, C.Li, C.Ma, J.Mrazek, A.M.Mukhamedzhanov, M.Notani, S.O'Brien, R.G.Pizzone, G.G.Rapisarda, D.Roberson, M.L.Sergi, W.Tan, I.J.Thompson, M.Wiescher Suppression of the centrifugal barrier effects in the off-energy-shell neutron + 17O interaction NUCLEAR REACTIONS 2H(17O, α14C), E=41, 43.5 MeV; measured α and 14C particle spectra, (14C)α-coin, angular distributions, yields using position-sensitive silicon detectors (PSD) at LNS, Catania, and at NSL, Notre Dame. CD2 target; deduced momentum distributions, Q value. DWBA analysis. 17O(n, α)14C, E(cm)=0-350 keV; deduced yields, angular distributions, neutron from quasifree breakup of deuteron. 18O; deduced resonances, J, π, and excitation functions. Trojan Horse method (THM), and suppression of centrifugal barrier. Comparison with previous studies. Relevance to neutron-induced reactions in nuclear reactors, and nucleosynthesis in astrophysics.
doi: 10.1103/PhysRevC.87.012801
2013PI03 Phys.Rev. C 87, 025805 (2013) R.G.Pizzone, C.Spitaleri, C.A.Bertulani, A.M.Mukhamedzhanov, L.Blokhintsev, M.La Cognata, L.Lamia, A.Rinollo, R.Sparta, A.Tumino Updated evidence of the Trojan horse particle invariance for the 2H(d, p)3H reaction NUCLEAR REACTIONS 2H(6Li, pt)α, E=14 MeV; measured proton and triton spectra by energy-loss method, momentum distribution, σ(θ) at INFN-LNS facility in Catania; deduced momentum distribution width, quasifree (QF) contribution, astrophysical S(E) factor for 2H(d, p) reaction via Trojan-horse method (THM) after 6Li breakup. 2H(3He, pt), E(cm)<0.9 MeV; analyzed averaged astrophysical S(E) factor for 2H(d, p) reaction measured via THM after 3He breakup. PWIA analysis. Comparison with previous experimental studies.
doi: 10.1103/PhysRevC.87.025805
2013SO11 Phys.Rev. C 87, 054329 (2013) L.G.Sobotka, W.W.Buhro, R.J.Charity, J.M.Elson, M.F.Jager, J.Manfredi, M.H.Mahzoon, A.M.Mukhamedzhanov, V.Eremenko, M.McCleskey, R.G.Pizzone, B.T.Roeder, A.Spiridon, E.Simmons, L.Trache, M.Kurokawa, P.Navratil Proton decay of excited states in 12N and 13O and the astrophysical 11C(p, γ)12N reaction rate NUCLEAR REACTIONS 9Be(13O, X), E=30.3 MeV/nucleon, [13O secondary beam from 1H(14N, X), E=38 MeV/nucleon primary reaction]; measured particle spectra, E(p), I(p), widths using MARS spectrometer at Texas AM cyclotron facility. Invariant mass method. R-matrix analysis. 11C, 12N, 13O; deduced levels, J, π, one-proton and two-proton decay branching ratios. 11C(p, γ)12N; deduced astrophysical reaction rates and S(E) factors.
doi: 10.1103/PhysRevC.87.054329
2012LA29 Phys.Rev.Lett. 109, 232701 (2012) M.La Cognata, C.Spitaleri, O.Trippella, G.G.Kiss, G.V.Rogachev, A.M.Mukhamedzhanov, M.Avila, G.L.Guardo, E.Koshchiy, A.Kuchera, L.Lamia, S.M.R.Puglia, S.Romano, D.Santiago, R.Sparta Measurement of the -3 keV Resonance in the Reaction 13C(α, n)16O of Importance in the s-Process NUCLEAR REACTIONS 13C(6Li, X)16O, E=7.82 MeV; measured reaction products, deuterons; deduced σ(θ, E), S-factors. Comparison with available data.
doi: 10.1103/PhysRevLett.109.232701
2012MU10 Phys.Rev. C 86, 034001 (2012) A.M.Mukhamedzhanov, V.Eremenko, A.I.Sattarov Generalized Faddeev equations in the Alt-Grassberger-Sandhas form for deuteron stripping with explicit inclusion of target excitations and Coulomb interaction
doi: 10.1103/PhysRevC.86.034001
2012MU14 Phys.Rev. C 86, 044615 (2012) Coulomb renormalization and ratio of proton and neutron asymptotic normalization coefficients for mirror nuclei NUCLEAR STRUCTURE 21Na, 57Cu, 132Sn; calculated squared proton and Coulomb renormalized asymptotic normalization coefficients (ANC). 8B, 8Li, 17F, 17O, 41Sc, 41Ca; calculated ratios of the proton and neutron ANCs for isobaric analog states of the mirror nuclei. Pinkston-Satchler equation and Wronskian formalism.
doi: 10.1103/PhysRevC.86.044615
2012TU05 J.Phys.:Conf.Ser. 337, 012017 (2012) A.Tumino, C.Spitaleri, A.M.Mukhamedzhanov, S.Typel, M.Aliotta, V.Burjan, M.G.del Santo, G.G.Kiss, V.Kroha, Z.Hons, M.La Cognata, L.Lamia, J.Mrazek, R.G.Pizzone, S.Piskor, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta Bare nucleus S(E) factor of the 2H(d, p)3H and 2H(d, n)3He reactions via the Trojan Horse Method NUCLEAR REACTIONS 2H(3He, pT), (3He, n3He), E(cm)≈0.002-2 MeV; measured reaction products; deduced 2H(d, p) and 2H(d, n) S-factor using THM (Trojan horse method) with quasifree kinematics. Compared with other THM and also with direct data.
doi: 10.1088/1742-6596/337/1/012017
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
2011LA13 Astrophys.J. 739, L54 (2011) M.La Cognata, A.M.Mukhamedzhanov, C.Spitaleri, I.Indelicato, M.Aliotta, V.Burjan, S.Cherubini, A.Coc, M.Gulino, Z.Hons, G.G.Kiss, V.Kroha, L.Lamia, J.Mrazek, S.Palmerini, S.Piskor, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, A.Tumino The Fluorine Destruction in Stars: First Experimental Study of the 19F(p, α0)16O Reaction at Astrophysical Energies NUCLEAR REACTIONS 2H(19F, nα), E=50 MeV; 19F(3He, αd), E=18.2 MeV; measured reaction products, 16O recoils; deduced σ(E, θ), S-factors, reaction rates. Comparison with previous results.
doi: 10.1088/2041-8205/739/2/L54
2011MU03 Phys.Rev. C 83, 044604 (2011) A.M.Mukhamedzhanov, M.La Cognata, V.Kroha Astrophysical S factor for the 15N( p, γ )16O reaction NUCLEAR REACTIONS 15N(p, γ), E=0-1.7 MeV; analyzed Notre Dame-LUNA experimental data; deduced astrophysical S factors and resonance parameters, widths using R-matrix approach.
doi: 10.1103/PhysRevC.83.044604
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
2011MU14 Phys.Rev. C 84, 024616 (2011) A.M.Mukhamedzhanov, V.Burjan, M.Gulino, Z.Hons, V.Kroha, M.McCleskey, J.Mrazek, N.Nguyen, F.M.Nunes, S.Piskor, S.Romano, M.L.Sergi, C.Spitaleri, R.E.Tribble Asymptotic normalization coefficients from the 14C(d, p)15C reaction NUCLEAR REACTIONS 14C(d, p), E=17.06 MeV; measured ep, Ip, σ(θ). 15C; deduced levels, J, π, l-transfer, asymptotic normalization coefficients for removal of neutron from the g.s. and first exited state of 15C, FR-ADWA analysis with CH-89 potential parameters. 14C(d, d), E=17.06 MeV; measured deuteron spectra, σ(θ); deduced potential parameters. Relevance to 14C(n, γ)15C reaction at astrophysical energies.
doi: 10.1103/PhysRevC.84.024616
2011MU17 Phys.Rev. C 84, 044616 (2011) Theory of deuteron stripping: From surface integrals to a generalized R-matrix approach
doi: 10.1103/PhysRevC.84.044616
2011TU06 Phys.Lett. B 700, 111 (2011), Erratum Phys.Lett. B 705, 546 (2011) A.Tumino, C.Spitaleri, A.M.Mukhamedzhanov, S.Typel, M.Aliotta, V.Burjan, M.G.del Santo, G.G.Kiss, V.Kroha, Z.Hons, M.La Cognata, L.Lamia, J.Mrazek, R.G.Pizzone, S.Piskor, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta Low-energy d+d fusion reactions via the Trojan Horse Method NUCLEAR REACTIONS 2H(3He, X), E=18 MeV; measured reaction products, 3H-p and 3He-p coin.; deduced σ(θ), S-factors for 2H(d, p), (d, n) reactions using Trojan Horse Method. Comparison with experimental data.
doi: 10.1016/j.physletb.2011.05.001
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
2010MU11 Phys.Rev. C 82, 051601 (2010) A.M.Mukhamedzhanov, A.S.Kadyrov Unitary correlation in nuclear reaction theory: Separation of nuclear reactions and spectroscopic factors
doi: 10.1103/PhysRevC.82.051601
2010MU16 J.Phys.:Conf.Ser. 202, 012017 (2010) A.M.Mukhamedzhanov, A.Banu, P.Bem, V.Burjan, C.A.Gagliardi, V.Z.Goldberg, Z.Hons, V.Kroha, M.La Cognata, S.Piskor, R.G.Pizzone, S.Romano, E.Simeckova, C.Spitaleri, L.Trache, R.E.Tribble Asymptotic normalization coefficient and important astrophysical process 15N(p, γ)160 NUCLEAR REACTIONS 15N(p, α), E=0-1200 keV; analyzed published data; calculated S-factor using resonant and nonresonant parts of R-matrix; deduced p ANC (asymptotic normalization coefficient). 15N(p, γ), E=resonance; calculated S-factor using R-matrix and ANC.
doi: 10.1088/1742-6596/202/1/012017
2009BA09 Phys.Rev. C 79, 025805 (2009) A.Banu, T.Al-Abdullah, C.Fu, C.A.Gagliardi, M.McCleskey, A.M.Mukhamedzhanov, G.Tabacaru, L.Trache, R.E.Tribble, Y.Zhai, F.Carstoiu, V.Burjan, V.Kroha Astrophysical S factor for the radiative capture 12N(p, γ)13O determined from the 14N(12N, 13O)13C proton transfer reaction NUCLEAR REACTIONS 14N(12N, 13O), E=12 MeV/nucleon; measured particle spectra, angular distributions, DWBA analysis; 12N(p, γ); deduced asymptotic normalization coefficient, astrophysical S-factor, and reaction rates.
doi: 10.1103/PhysRevC.79.025805
2009LA13 Phys.Rev. C 80, 012801 (2009) M.La Cognata, V.Z.Goldberg, A.M.Mukhamedzhanov, C.Spitaleri, R.E.Tribble Improved determination of the astrophysical S(0) factor of the 15N(p, α)12C reaction NUCLEAR REACTIONS 15N(p, α)12C, E(cm)<0.8 MeV; analyzed experimental data; deduced astrophysical S factors and effect of finite energy resolution on S-factors using R-matrix fits to experimental and Trojan Horse data.
doi: 10.1103/PhysRevC.80.012801
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
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
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
2008ME11 Phys.Rev. C 78, 031602 (2008) K.Mercurio, R.J.Charity, R.Shane, L.G.Sobotka, J.M.Elson, M.Famiano, A.H.Wuosmaa, A.Banu, C.Fu, L.Trache, R.E.Tribble, A.M.Mukhamedzhanov Correlated two-proton decay from 10C NUCLEAR REACTIONS Be, C(10C, 10C'), E=10.7 MeV; measured proton spectra, α spectra, αp-, pp-coin from excited states. 10C; deduced levels, correlated 2p decay mode.
doi: 10.1103/PhysRevC.78.031602
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
2008MU12 Phys.Rev. C 77, 051601 (2008) A.M.Mukhamedzhanov, F.M.Nunes, P.Mohr Benchmark on neutron capture extracted from (d, p) reactions NUCLEAR REACTIONS 48Ca(d, p), E=2, 13, 19, 56 MeV; 48Ca(n, γ), E=25 MeV; analyzed angular distributions; deduced asymptotic normalization coefficients, spectroscopic factors.
doi: 10.1103/PhysRevC.77.051601
2008MU15 Phys.Rev. C 78, 015804 (2008) A.M.Mukhamedzhanov, P.Bem, V.Burjan, C.A.Gagliardi, V.Z.Goldberg, Z.Hons, M.La Cognata, V.Kroha, J.Mrazek, J.Novak, S.Piskor, R.G.Pizzone, A.Plunkett, S.Romano, E.Simeckova, C.Spitaleri, L.Trache, R.E.Tribble, F.Vesely, J.Vincour New astrophysical S factor for the 15N(p, γ)16O reaction via the asymptotic normalization coefficient (ANC) method NUCLEAR REACTIONS 15N(3He, d), E=25.74 MeV; measured deuteron spectra, asymptotic normalization coefficients, angular distributions. 15N(p, γ), (p, α); deduced astrophysical S-factors, resonance parameters.
doi: 10.1103/PhysRevC.78.015804
2008MU17 Eur.Phys.J. A 37, 185 (2008) Completeness of the Coulomb scattering wave functions
doi: 10.1140/epja/i2008-10613-1
2008RO05 J.Phys.(London) G35, 014008 (2008) S.Romano, C.Spitaleri, S.Cherubini, V.Crucilla, M.Gulino, M.La Cognata, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, M.L.Sergi, S.Tudisco, A.Tumino, R.E.Tribble, V.Z.Goldberg, A.M.Mukhamedzhanov, G.Tabacaru, L.Trache, V.Kroha, V.Burjan, Z.Hons, J.Mrazek, E.Somorjai, Z.Elekes, Z.Fulop, G.Gyurky, G.Kiss, A.Szanto de Toledo, N.Carlin, M.M.De Moura, M.G.Del Santo, M.G.Munhoz, R.Liguori Neto, F.A.Souza, A.A.P.Suaide, E.Szanto The Trojan horse method in nuclear astrophysics: recent results NUCLEAR REACTIONS 7Li(p, α)α, E(cm)=0-7 MeV; 10B(p, α)7Be, E(cm)=0-400 keV; p(p, p)p, E ≈ 0-0.6 MeV; analyzed cross section, S-factors.Trojan Horse Method.
doi: 10.1088/0954-3899/35/1/014008
2007AL28 Phys.Rev. C 75, 054003 (2007) E.O.Alt, L.D.Blokhintsev, A.M.Mukhamedzhanov, A.I.Sattarov Deuteron elastic scattering and stripping processes off 12C as a three-body problem NUCLEAR REACTIONS 12C(d, d), (d, p), E=4.66, 15, 56 MeV; calculated σ and analyzing powers within the framework of few body integral equations theory. Compared results to data.
doi: 10.1103/PhysRevC.75.054003
2007FU09 Phys.Rev. C 76, 021603 (2007) C.Fu, V.Z.Goldberg, A.M.Mukhamedzhanov, G.G.Chubarian, G.V.Rogachev, B.Skorodumov, M.McCleskey, Y.Zhai, T.Al-Abdullah, G.Tabacaru, L.Trache, R.E.Tribble Single and double proton emissions from the 14O+4He interaction NUCLEAR REACTIONS 4He(14O, X)16O, E=32.7 MeV; measured yields and excitation function.
doi: 10.1103/PhysRevC.76.021603
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
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
2007PA10 Phys.Rev. C 75, 024601 (2007) D.Y.Pang, F.M.Nunes, A.M.Mukhamedzhanov Are spectroscopic factors from transfer reactions consistent with asymptotic normalization coefficients? NUCLEAR REACTIONS 14C(d, p), E=14 MeV; 16O(d, p), E=15 MeV; 40Ca(d, p), E=11 MeV; analyzed σ(θ); deduced spectroscopic factors, asymptotic normalization coefficients.
doi: 10.1103/PhysRevC.75.024601
2006JO11 Phys.Rev.Lett. 97, 192701 (2006) E.D.Johnson, G.V.Rogachev, A.M.Mukhamedzhanov, L.T.Baby, S.Brown, W.T.Cluff, A.M.Crisp, E.Diffenderfer, V.Z.Goldberg, B.W.Green, T.Hinners, C.R.Hoffman, K.W.Kemper, O.Momotyuk, P.Peplowski, A.Pipidis, R.Reynolds, B.T.Roeder Astrophysical Reaction Rate for the Neutron-Generator Reaction 13C(α, n)16O in Asymptotic Giant Branch Stars NUCLEAR REACTIONS 6Li(13C, d), E=8.0, 8.5 MeV; measured deuteron spectra, σ(E, θ); deduced asymptotic normalization coefficient for subthreshold resonance. 13C(α, n), E ≈ 0-1 MeV; deduced astrophysical S-factor, reaction rates.
doi: 10.1103/PhysRevLett.97.192701
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
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
2006TA09 Phys.Rev. C 73, 025808 (2006) G.Tabacaru, A.Azhari, J.Brinkley, V.Burjan, F.Carstoiu, C.Fu, C.A.Gagliardi, V.Kroha, A.M.Mukhamedzhanov, X.Tang, L.Trache, R.E.Tribble, S.Zhou Scattering of 7Be and 8B and the astrophysical S17 factor NUCLEAR REACTIONS H, C, N(7Be, 7Be), E=87 MeV; C(8B, 8B), E=95 MeV; measured σ(θ); deduced asymptotic normalization coefficients. 7Be(p, γ), E=low; deduced astrophysical S-factor.
doi: 10.1103/PhysRevC.73.025808
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
2005BL23 Phys.Rev. C 72, 034606 (2005) J.C.Blackmon, F.Carstoiu, L.Trache, D.W.Bardayan, C.R.Brune, C.A.Gagliardi, U.Greife, C.J.Gross, C.C.Jewett, R.L.Kozub, T.A.Lewis, J.F.Liang, B.H.Moazen, A.M.Mukhamedzhanov, C.D.Nesaraja, F.M.Nunes, P.D.Parker, L.Sahin, J.P.Scott, D.Shapira, M.S.Smith, J.S.Thomas, R.E.Tribble Elastic scattering of the proton drip-line nucleus 17F NUCLEAR REACTIONS 12C, 14N(17F, 17F), E=10 MeV/nucleon; measured σ(θ); deduced parameters, reaction mechanism features. Double-folding procedure.
doi: 10.1103/PhysRevC.72.034606
2005MU24 Phys.Rev. C 72, 017602 (2005) Combined method to extract spectroscopic information NUCLEAR REACTIONS 208Pb(d, p), E=22 MeV; 12C(d, p), E=51 MeV; 84Se(d, p), E=4-100 MeV; analyzed data; deduced spectroscopic factors.
doi: 10.1103/PhysRevC.72.017602
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
2005NU02 Eur.Phys.J. A 25, Supplement 1, 295 (2005) F.M.Nunes, A.M.Moro, A.M.Mukhamedzhanov, N.C.Summers Progress on reactions with exotic nuclei
doi: 10.1140/epjad/i2005-06-160-7
2004BL21 Nucl.Phys. A746, 365c (2004) J.C.Blackmon, D.W.Bardayan, C.R.Brune, F.Carstoiu, A.E.Champagne, R.Crespo, T.Davinson, J.C.Fernandes, C.A.Gagliardi, U.Greife, C.J.Gross, P.A.Hausladen, C.Iliadis, C.C.Jewett, R.L.Kozub, T.A.Lewis, F.Liang, B.H.Moazen, A.M.Mukhamedzhanov, C.D.Nesaraja, F.M.Nunes, P.D.Parker, D.C.Radford, L.Sahin, J.P.Scott, D.Shapira, M.S.Smith, J.S.Thomas, L.Trache, R.E.Tribble, P.J.Woods, C.-H.Yu The 17F(p, γ)18Ne direct capture cross section NUCLEAR REACTIONS 12C, 14N(17F, 17F), E=170 MeV; 14N(17F, 18Ne), E=170 MeV; measured σ(θ).
doi: 10.1016/j.nuclphysa.2004.09.054
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
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
2004TR15 Nucl.Phys. A746, 625c (2004) L.Trache, F.Carstoiu, C.A.Gagliardi, A.M.Mukhamedzhanov, R.E.Tribble Breakup of loosely bound nuclei at intermediate energies as indirect method in nuclear astrophysics: 8B, 9C and the S17, S18 astrophysical factors NUCLEAR REACTIONS C, Al, Sn, Pb(8B, p7Be), E=28-285 MeV/nucleon; analyzed data; deduced asymptotic normalization coefficients. 7Be(p, γ), E=low; deduced astrophysical S-factors.
doi: 10.1016/j.nuclphysa.2004.09.102
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
2003BL12 Nucl.Phys. A718, 587c (2003) J.C.Blackmon, D.W.Bardayan, C.R.Brune, A.E.Champagne, R.Crespo, T.Davinson, J.C.Fernandes, C.A.Gagliardi, U.Greife, C.J.Gross, P.A.Hausladen, C.Iliadis, C.C.Jewett, R.L.Kozub, T.A.Lewis, F.Liang, B.H.Moazen, A.M.Mukhamedzhanov, C.D.Nesaraja, F.M.Nunes, P.D.Parker, D.C.Radford, L.Sahin, J.P.Scott, D.Shapira, M.S.Smith, J.S.Thomas, L.Trache, R.E.Tribble, P.J.Woods, C.-H.Yu The 17F(p, γ)18Ne Direct Capture Cross Section NUCLEAR REACTIONS 14N(17F, 18Ne), E=170 MeV; measured Eγ, Iγ, particle spectra, (particle)γ-coin, σ(θ).
doi: 10.1016/S0375-9474(03)00872-8
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
2003KR14 Nucl.Phys. A719, 119c (2003) V.Kroha, A.Azhari, P.Bem, V.Burjan, C.A.Gagliardi, A.M.Mukhamedzhanov, J.Novak, S.Piskor, E.Simeckova, X.Tang, L.Trache, R.E.Tribble, J.Vincour Asymptotic Normalization Coefficients in nuclear astrophysics NUCLEAR REACTIONS 9Be, 11,13C(p, γ), E=low; analyzed asymptotic normalization coefficients, astrophysical S-factors.
doi: 10.1016/S0375-9474(03)00979-5
2003MU12 Phys.Rev. C 67, 065804 (2003); Erratum Phys.Rev. C 68, 019901 (2003) A.M.Mukhamedzhanov, P.Bem, B.A.Brown, V.Burjan, C.A.Gagliardi, V.Kroha, J.Novak, F.M.Nunes, S.Piskor, F.Pirlepesov, E.Simeckova, R.E.Tribble, J.Vincour Asymptotic normalization coefficients for 14N + p → 15O and the astrophysical S factor for 14N(p, γ)15O NUCLEAR REACTIONS 14N(3He, d), (3He, 3He), E=26.3 MeV; measured σ(θ); deduced asymptotic normalization coefficients. 14N(p, γ), E < 600 keV; deduced astrophysical S-factors, reaction rates.
doi: 10.1103/PhysRevC.67.065804
2003MU18 Nucl.Phys. A725, 279 (2003) A.M.Mukhamedzhanov, A.Azhari, V.Burjan, C.A.Gagliardi, V.Kroha, A.Sattarov, X.Tang, L.Trache, R.E.Tribble Asymptotic normalization coefficients from proton transfer reactions and astrophysical S factors for the CNO 13C(p, γ)14N radiative capture process NUCLEAR REACTIONS 13C(14N, 13C), (3He, d), E not given; 13C(p, γ), E(cm)=100-900 keV; analyzed data; deduced asymptotic normalization coefficients. 13C(p, γ), E=0-900 keV; deduced astrophysical S-factors. R-matrix approach.
doi: 10.1016/S0375-9474(03)01618-X
2003TA02 Phys.Rev. C 67, 015804 (2003) X.Tang, A.Azhari, C.A.Gagliardi, A.M.Mukhamedzhanov, F.Pirlepesov, L.Trache, R.E.Tribble, V.Burjan, V.Kroha, F.Carstoiu Determination of the astrophysical S factor for 11C(p, γ)12N from the 12N → 11C+p asymptotic normalization coefficient NUCLEAR REACTIONS 14N(11C, 12N), E=110 MeV; measured particle spectra, σ(θ); deduced asymptotic normalization coefficient. 11C(p, γ), E(cm)=0-0.7 MeV; deduced astrophysical S-factor, reaction rate.
doi: 10.1103/PhysRevC.67.015804
2003TI13 Phys.Rev.Lett. 91, 232501 (2003) N.K.Timofeyuk, R.C.Johnson, A.M.Mukhamedzhanov Relation between Proton and Neutron Asymptotic Normalization Coefficients for Light Mirror Nuclei and its Relevance to Nuclear Astrophysics NUCLEAR STRUCTURE 6,7,8Li, 7Be, 8,11,12B, 11,12,13C, 12,13,14,15N, 15,16,17O, 17F, 22,23Ne, 22,26,27Mg, 23Al, 26Si, 27P; calculated overlap integrals, proton and neutron mirror asymptotic normalization coefficients. Astrophysical implications discussed.
doi: 10.1103/PhysRevLett.91.232501
2003TR04 Phys.Rev. C 67, 062801 (2003) L.Trache, A.Azhari, F.Carstoiu, H.L.Clark, C.A.Gagliardi, Y.-W.Lui, A.M.Mukhamedzhanov, X.Tang, N.Timofeyuk, R.E.Tribble Asymptotic normalization coefficients for 8B → 7Be + p from a study of 8Li → 7Li + n NUCLEAR REACTIONS 13C(7Li, 8Li), E=63 MeV; measured σ(θ); deduced spectroscopic factors, asymptotic normalization coefficients. 7Be(p, γ), E=low; deduced astrophysical S-factor.
doi: 10.1103/PhysRevC.67.062801
2003TR09 Nucl.Phys. A718, 147c (2003) R.E.Tribble, A.Azhari, P.Bem, V.Burjan, F.Carstoiu, C.A.Gagliardi, V.Kroha, A.M.Mukhamedzhanov, J.Novak, F.Pirlepesov, S.Piskor, A.Sattarov, E.Simeckova, X.Tang, L.Trache, J.Vincour New Results for 8B(p, γ)9C, 11C(p, γ)12N, 13C(p, γ)14N and 14N(p, γ)15O at stellar energies NUCLEAR REACTIONS 8B, 11,13C, 14N(p, γ), E=low; analyzed asymptotic normalization coefficients; deduced astrophysical reaction rates, S-factors.
doi: 10.1016/S0375-9474(03)00705-X
2003TR10 Nucl.Phys. A718, 493c (2003) L.Trache, F.Carstoiu, C.A.Gagliardi, A.M.Mukhamedzhanov, R.E.Tribble Determination of the S17 and S18 astrophysical factors from the breakup of 8B and 9C at intermediate energies NUCLEAR REACTIONS Si(8B, X), E=38 MeV/nucleon; C, Al, Sn, Pb(9C, X), E=285 MeV/nucleon; analyzed breakup data; deduced asymptotic normalization coefficients, astrophysical S-factors.
doi: 10.1016/S0375-9474(03)00867-4
2002AL18 Phys.Rev. C65, 064613 (2002) E.O.Alt, A.M.Mukhamedzhanov, M.M.Nishonov, A.I.Sattarov Proton-Deuteron Elastic Scattering from 2.5 to 22.7 MeV NUCLEAR REACTIONS 2H(p, p), E=2.5-22.7 MeV; calculated σ(θ), vector and tensor analyzing powers. Paris potential, comparison with data.
doi: 10.1103/PhysRevC.65.064613
2002GA11 Eur.Phys.J. A 13, 227 (2002) C.A.Gagliardi, A.Azhari, V.Burjan, F.Carstoiu, V.Kroha, A.M.Mukhamedzhanov, A.Sattarov, X.Tang, L.Trache, R.E.Tribble Asymptotic Normalization Coefficients and Astrophysical Direct Capture Rates NUCLEAR REACTIONS 16O(3He, d), E not given; analyzed σ(E, θ). 16O(p, γ), E=0-1.3 MeV; 9Be(p, γ), E(cm)=0-1.6 MeV; analyzed S-factors. 10B, 14N(7Be, 7Be), (7Be, 8B), E=12 MeV/nucleon; 1H, 14N(11C, 12N), (11C, 11C), E not given; measured σ(θ); deduced asymptotic normalization coefficients. 7Be(p, γ), E not given; deduced reaction rate.
doi: 10.1007/s10050-002-8747-8
2002GA44 Eur.Phys.J. A 15, 69 (2002) C.A.Gagliardi, A.Azhari, V.Burjan, F.Carstoiu, V.Kroha, A.M.Mukhamedzhanov, A.Sattarov, X.Tang, L.Trache, R.E.Tribble Asymptotic normalization coefficients in nuclear astrophysics and structure NUCLEAR REACTIONS 11C, 16O(p, γ), E ≈ 0.2-1.4 MeV; 9Be(8B, p7Be), E=41 MeV/nucleon; analyzed astrophysical S-factors, asymptotic normalization coefficients.
doi: 10.1140/epja/i2001-10228-6
2002MU14 Phys.Rev. C66, 027602 (2002) A.M.Mukhamedzhanov, A.Azhari, V.Burjan, C.A.Gagliardi, V.Kroha, A.Sattarov, X.Tang, L.Trache, R.E.Tribble Astrophysical S factor for 13C(p, γ) 14N and asymptotic normalization coefficients NUCLEAR REACTIONS 13C(p, γ), E ≈ 0-800 keV; analyzed astrophysical S-factors, asymptotic normalization coefficients.
doi: 10.1103/PhysRevC.66.027602
2002MU16 Nucl.Phys. A708, 437 (2002) Low Energy Behavior of the Astrophysical S-Factor in Radiative Captures to Loosely Bound Final States NUCLEAR REACTIONS 7Be, 14N, 16O, 20Ne(p, γ), E ≈ 0-0.15 MeV; calculated astrophysical S-factors.
doi: 10.1016/S0375-9474(02)01011-4
2002TR14 Phys.Rev. C66, 035801 (2002) L.Trache, F.Carstoiu, A.M.Mukhamedzhanov, R.E.Tribble Determination of the S18 Astrophysical Factor for 8B(p, γ)9C from the Breakup of 9C at Intermediate Energies NUCLEAR REACTIONS 12C, 27Al, 116Sn, 208Pb(9C, 8B), E=285 MeV/nucleon; analyzed data; deduced asymptotic normalization coefficients. 8B(p, γ), E(cm)=0-0.8 MeV; calculated astrophysical S-factor, reaction rates.
doi: 10.1103/PhysRevC.66.035801
2001AL16 Nucl.Phys. A684, 542c (2001) E.O.Alt, A.M.Mukhamedzhanov, A.I.Sattarov Energy-Dependence of Proton-Deuteron Scattering Observables NUCLEAR REACTIONS 2H(p, p), E=5, 18 MeV; calculated σ(θ), Ay(θ). Comparison with data.
doi: 10.1016/S0375-9474(01)00385-2
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