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Search: Author = A.Mukhamedzhanov

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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
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2023MU08      Eur.Phys.J. A 59, 43 (2023)

A.M.Mukhamedzhanov

Resonances in low-energy nuclear processes and nuclear astrophysics and asymptotic normalization coefficients: a review

doi: 10.1140/epja/s10050-023-00918-8
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2023MU18      Phys.Rev. C 108, 054603 (2023)

A.M.Mukhamedzhanov

Proton 0.01 MeV resonance width and low-energy S factor of p + 10B

doi: 10.1103/PhysRevC.108.054603
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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
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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
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2022MU13      Eur.Phys.J. A 58, 71 (2022)

A.M.Mukhamedzanov

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
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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.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD1037.


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
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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.


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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0956. Data from this article have been entered in the XUNDL database. For more information, click here.


2019MU05      Phys.Rev. C 99, 024311 (2019)

A.M.Mukhamedzhanov

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
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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
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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
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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
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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
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2018MU15      Phys.Rev. C 98, 044626 (2018)

A.M.Mukhamedzhanov

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
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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
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2017GU05      Phys.Rev. C 95, 025807 (2017)

G.L.Guardo, C.Spitaleri, L.Lamia, M.Gulino, M.La Cognata, X.Tang, R.deBoer, X.Fang, V.Goldberg, J.Mrazek, A.Mukhamedzhanov, M.Notani, R.G.Pizzone, G.G.Rapisarda, M.L.Sergi, M.Wiescher

Assessing the near threshold cross section of the 17O(n, α)14C reaction by means of the Trojan horse method

NUCLEAR REACTIONS 2H(17O, α14C), E=43.5 MeV; measured reaction products, particle spectra, (particle)(particle)-coin, angular distributions using two telescopes of ionization chambers (IC) and silicon position-sensitive detector (PSD) at LNS-Catania and NSL-Notre Dame accelerator facilities; deduced normalized reaction yields, experimental momentum distribution, quasifission (QF) cross sections and best fit from R-matrix analysis. 18O; deduced levels, resonances, J, π, and Trojan horse method (THM) analysis of Γn, Γα and total widths. 17O(n, α)14C, T9=0.01-10; deduce astrophysical reaction rates by THM method.

doi: 10.1103/PhysRevC.95.025807
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23332. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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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
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2017SP04      Phys.Rev. C 95, 035801 (2017)

C.Spitaleri, S.M.R.Puglia, M.La Cognata, L.Lamia, S.Cherubini, A.Cvetinovic, G.D'Agata, M.Gulino, G.L.Guardo, I.Indelicato, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, S.Tudisco, A.Tumino, M.Gimenez Del Santo, N.Carlin, M.G.Munhoz, F.A.Souza, A.Szanto de Toledo, A.Mukhamedzhanov, C.Broggini, A.Caciolli, R.Depalo, R.Menegazzo, V.Rigato, I.Lombardo, D.Dell'Aquila

Measurement of the 10B(p, α0)7Be cross section from 5 keV to 1.5 MeV in a single experiment using the Trojan horse method

NUCLEAR REACTIONS 2H(10B, α7Be), E=27 MeV; measured α and 7Be spectra using ΔE-E method at Pelletron-Linac laboratory of DFN-Sao Paulo; deduced Q-value spectrum, energy scatter plots, momentum distribution, astrophysical S(E) factors, Trojan horse method (THM) astrophysical factor, R-matrix fit of THM data 11C; deduced levels, resonances, center-of-mass energies, J, π, Γp, Γα0, Γα1.

doi: 10.1103/PhysRevC.95.035801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0837.


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


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
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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
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2015MU08      Phys.Rev. C 92, 014625 (2015)

A.M.Mukhamedzhanov, D.Y.Pang

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
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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
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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, Γp, Γα, Γγ 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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Data from this article have been entered in the XUNDL database. For more information, click here.


2014AL05      Phys.Rev. C 89, 025809 (2014)

T.Al-Abdullah, F.Carstoiu, X.Chen, H.L.Clark, C.A.Gagliardi, Y.-W.Lui, A.Mukhamedzhanov, G.Tabacaru, Y.Tokimoto, L.Trache, R.E.Tribble, Y.Zhai

Astrophysical reaction rate for 17F(p, γ)18Ne from the transfer reaction 13C(17O, 18O)12C

NUCLEAR REACTIONS 13C(17O, 18O), 12C(18O, 18O), E=12 MeV/nucleon; measured particle spectra using multipole dipole-multipole (MDM) magnetic spectrometer, σ(θ) at Texas A and M facility. 18O; deduced levels, J, asymptotic normalization coefficients (ANCs) of ground state, first two 2+ states and first 4+ state. 17F(p, γ)18Ne, at T9=0.1-1; deduced reaction rates, astrophysical S factor from mirror analogy of states in 18O and 18Ne. Optical model parameters and DWBA analysis. Discussed production of 18F at stellar energies in ONe novae.

doi: 10.1103/PhysRevC.89.025809
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2090. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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2014PA49      Phys.Rev. C 90, 044611 (2014)

D.Y.Pang, A.M.Mukhamedzhanov

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
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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
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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 Eα-Be and Eα-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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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
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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
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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
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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
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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
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2012LA01      J.Phys.(London) G39, 015106 (2012)

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

New measurement of the 11B(p, α0)8Be bare-nucleus S(E) factor via the Trojan horse method

NUCLEAR REACTIONS 2H(11B, α), E=27 MeV; measured reaction products, Eα, Iα. 8Be; deduced σ(θ), S-factors.

doi: 10.1088/0954-3899/39/1/015106
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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
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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
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2012MU14      Phys.Rev. C 86, 044615 (2012)

A.M.Mukhamedzhanov

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
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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
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2011AD03      Rev.Mod.Phys. 83, 195 (2011)

E.G.Adelberger, A.Garcia, R.G.H.Robertson, K.A.Snover, A.B.Balantekin, K.Heeger, M.J.Ramsey-Musolf, A.B.Balantekin, K.Heeger, M.J.Ramsey-Musolf, D.Bemmerer, A.Junghans, D.Bemmerer, A.Junghans, C.A.Bertulani, K.-W.Chen, H.Costantini, P.Prati, M.Couder, E.Uberseder, M.Wiescher, R.Cyburt, B.Davids, S.J.Freedman, M.Gai, D.Gazit, L.Gialanella, G.Imbriani, U.Greife, M.Hass, W.C.Haxton, T.Itahashi, K.Kubodera, K.Langanke, D.Leitner, M.Leitner, P.Vetter, L.Winslow, L.E.Marcucci, T.Motobayashi, A.Mukhamedzhanov, R.E.Tribble, F.M.Nunes, T.-S.Park, R.Schiavilla, E.C.Simpson, C.Spitaleri, F.Strieder, H.-P.Trautvetter, K.Suemmerer, S.Typel

Solar fusion cross sections. II. The pp chain and CNO cycles

NUCLEAR REACTIONS 2H(p, γ), 3He(3He, 2p), (α, γ), (p, e), 7Be, 12C, 14N, 15N, 17O(p, γ), 15N, 16,17,18O(p, α), E<3 MeV; analyzed and evaluated experimental data; deduced recommended values and uncertainties.

doi: 10.1103/RevModPhys.83.195
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2011CH08      Acta Phys.Pol. B42, 769 (2011)

S.Cherubini, C.Spitaleri, M.Gulino, M.La Cognata, R.G.Pizzone, L.Lamia, G.G.Rapisarda, S.Romano, L.Sergi, A.Mukhamedzhanov, L.Trache, R.E.Tribble, S.Kubono, H.Yamaguchi, A.Tumino

Recent Studies on Trojan Horse Method

doi: 10.5506/APhysPolB.42.769
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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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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
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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
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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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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
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2011MU17      Phys.Rev. C 84, 044616 (2011)

A.M.Mukhamedzhanov

Theory of deuteron stripping: From surface integrals to a generalized R-matrix approach

doi: 10.1103/PhysRevC.84.044616
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2011PI04      Phys.Rev. C 83, 045801 (2011)

R.G.Pizzone, C.Spitaleri, L.Lamia, C.Bertulani, A.Mukhamedzhanov, L.Blokhintsev, V.Burjan, S.Cherubini, Z.Hons, G.G.Kiss, V.Kroha, M.La Cognata, C.Li, J.Mrazek, S.Piskor, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, A.Tumino

Trojan horse particle invariance studied with the 6Li(d, α)4He and 7Li( p, α)4He reactions

NUCLEAR REACTIONS 6Li(3He, 2α), E=17.5 MeV; measured Eα, Iα, angular distribution; deduced momentum distribution, Q value, quasifree (QF) contribution. 6Li(d, α), E(cm)=0-5 MeV; 7Li(p, α), E(cm)=0-7 MeV; 7Li(3He, 2α), E not given; analyzed excitation functions, σ, differential σ. Trojan horse method (THM) in the framework of the plane wave approximation.

doi: 10.1103/PhysRevC.83.045801
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2011TU04      Few-Body Systems 50, 323 (2011)

A.Tumino, C.Spitaleri, A.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

Indirect Study of the 2H(d, p)3H and 2H(d, n)3He Reactions at Astrophysical Energies via the Trojan Horse Method

NUCLEAR REACTIONS 2H(d, p), (d, n), E(cm)=0.02, 0.13, 0.98, 1.25 MeV; measured reaction products, proton spectra; deduced σ(θ). Trojan horse method.

doi: 10.1007/s00601-010-0213-6
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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
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2010AL10      Phys.Rev. C 81, 035802 (2010)

T.Al-Abdullah, F.Carstoiu, X.Chen, H.L.Clark, C.Fu, C.A.Gagliardi, Y.-W.Lui, A.Mukhamedzhanov, G.Tabacaru, Y.Tokimoto, L.Trache, R.E.Tribble

Stellar reaction rate for 22Mg+p → 23Al from the asymptotic normalization coefficient in the mirror nuclear system 22Ne+n → 23Ne

NUCLEAR REACTIONS 13C(12C, 13C), (12C, 12C), E=10.6 MeV/nucleon; 12C(22Ne, 22Ne), (22Ne, 22Ne'), 13C(22Ne, 22Ne), (22Ne, 23Ne), E=12 MeV/nucleon; measured particle spectra, σ and σ(θ); deduced optical model parameters and asymptotic normalization coefficients (ANC). 22Mg(p, γ); deduced direct and resonant capture rates, and effect on the depletion of 22Na in O-Ne Novae.

doi: 10.1103/PhysRevC.81.035802
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2010GU17      J.Phys.(London) G37, 125105 (2010)

M.Gulino, C.Spitaleri, S.Cherubini, V.Crucilla, M.La Cognata, L.Lamia, R.G.Pizzone, S.Romano, M.L.Sergi, A.Tumino, C.-B.Li, Z.Elekes, E.Somorjai, V.Burjan, V.Kroha, A.Mukhamedzhanov

Study of the 6Li(n, α)3H reaction via the 2H quasi-free break-up

NUCLEAR REACTIONS 2H(6Li, tα), E=14, 17 MeV; measured reaction products; deduced σ for 6Li(n, α) reaction.

doi: 10.1088/0954-3899/37/12/125105
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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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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
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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
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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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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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2010SP04      Nucl.Phys. A834, 639c (2010)

C.Spitaleri, S.Cherubini, M.La Cognata, L.Lamia, A.Mukhamedzhanov, R.G.Pizzone, S.Romano, M.L.Sergi, A.Tumino

Trojan Horse Method: recent applications in nuclear astrophysics

doi: 10.1016/j.nuclphysa.2010.01.111
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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
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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
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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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2008LA06      J.Phys.(London) G35, 014014 (2008)

M.La Cognata, C.Spitaleri, R.E.Tribble, T.Al-Abdullah, A.Banu, S.Cherubini, V.Crucilla, C.Fu, V.Goldberg, M.Gulino, L.Lamia, A.Mukhamedzhanov, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, G.Tabacaru, L.Trache, S.Tudisco, A.Tumino, S.Typel, Y.Zhai

Indirect measurement of the 18O(p, α)15N reaction rate through the THM

NUCLEAR REACTIONS 2H(18O, α15N)n, E=54 MeV; measured charged particle spectra, angular and momentum distributions, cross sections; 18O(p, α)15N, E(cm)=0-1.5 MeV; deduced S-factor, reaction rate. Trojan Horse Method.

doi: 10.1088/0954-3899/35/1/014014
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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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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
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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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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
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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
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2008MU17      Eur.Phys.J. A 37, 185 (2008)

A.M.Mukhamedzhanov, M.Akin

Completeness of the Coulomb scattering wave functions

doi: 10.1140/epja/i2008-10613-1
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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
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2008TU07      Phys.Rev. C 78, 064001 (2008)

A.Tumino, C.Spitaleri, A.Mukhamedzhanov, G.G.Rapisarda, L.Campajola, S.Cherubini, V.Crucilla, Z.Elekes, Z.Fulop, L.Gialanella, M.Gulino, G.Gyurky, G.Kiss, M.La Cognata, L.Lamia, A.Ordine, R.G.Pizzone, S.Romano, M.L.Sergi, E.Somorjai

Off-energy-shell p-p scattering at sub-Coulomb energies via the Trojan horse method

NUCLEAR REACTIONS 2H(p, 2p), E=5 MeV; measured Ep, Ip, pp-coin, momentum distributions, two- and three-body σ. Trojan Horse Method.

doi: 10.1103/PhysRevC.78.064001
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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
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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
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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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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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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
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2007SK02      Phys.Rev. C 75, 024607 (2007)

B.B.Skorodumov, G.V.Rogachev, P.Boutachkov, A.Aprahamian, V.Z.Goldberg, A.Mukhamedzhanov, S.Almaraz, H.Amro, F.D.Becchetti, S.Brown, Y.Chen, H.Jiang, J.J.Kolata, L.O.Lamm, M.Quinn, A.Woehr

Lowest excited states of 13O

NUCLEAR REACTIONS 1H(12N, p), E(cm)=0.8-2.7 MeV; measured Ep, excitation functions for elastic scattering. 13O deduced resonance energies, J, π, widths. 12N(p, γ), E=low; calculated astrophysical reaction rates. R-matrix calculations.

doi: 10.1103/PhysRevC.75.024607
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2007TU02      Phys.Rev.Lett. 98, 252502 (2007)

A.Tumino, C.Spitaleri, A.Mukhamedzhanov, G.G.Rapisarda, S.Cherubini, V.Crucilla, Z.Elekes, Z.Fulop, M.Gulino, G.Gyurky, G.Kiss, M.La Cognata, L.Lamia, F.Mudo, R.G.Pizzone, S.Romano, M.L.Sergi, E.Somorjai

Suppression of the Coulomb Interaction in the Off-Energy-Shell p - p Scattering form the p + d → p + p + m Reaction

NUCLEAR REACTIONS 2H(p, 2p), E=5 MeV; measured cross sections. Analyzed data using the Trojan Horse Method to deduce off-energy shell effects on p-p scattering.

doi: 10.1103/PhysRevLett.98.252502
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2007TU04      Nucl.Phys. A787, 337c (2007)

A.Tumino, C.Spitaleri, G.G.Rapisarda, S.Cherubini, S.Blagus, M.Bogovac, V.Crucilla, Z.Elekes, Z.Fulop, M.Gulino, G.Gyurky, G.Kiss, M.La Cognata, L.Lamia, Dj.Miljanic, M.Milin, F.Mudo, A.Mukhamedzhanov, R.G.Pizzone, D.Rendic, S.Romano, M.L.Sergi, E.Somorjai

No signature of nuclear-Coulomb interference in the proton-proton elastic scattering via the Trojan Horse Method

NUCLEAR REACTIONS 2H(p, 2p), E=5, 6 MeV; measured Ep, Ip, σ(E, θ). Plane wave impulse approximation, Trojan horse method.

doi: 10.1016/j.nuclphysa.2006.12.053
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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
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2006LA18      Eur.Phys.J. A 27, Supplement 1, 249 (2006)

M.La Cognata, S.Romano, C.Spitaleri, R.Tribble, L.Trache, S.Cherubini, C.Fu, L.Lamia, A.Mukhamedzhanov, R.G.Pizzone, C.Rolfs, G.Tabacaru, A.Tumino

Indirect measurement of the 15N(p, α)12C reaction cross section through the Trojan-Horse Method

NUCLEAR REACTIONS 2H(15N, nα), E=60 MeV; measured particle spectra, correlations; deduced quasi-free contribution. 15N(p, α), E(cm) ≈ 0-600 keV; deduced astrophysical S-factor.

doi: 10.1140/epja/i2006-08-039-0
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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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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1495.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1367.


2005MU24      Phys.Rev. C 72, 017602 (2005)

A.M.Mukhamedzhanov, F.M.Nunes

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
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Note: The following list of authors and aliases matches the search parameter A.Mukhamedzhanov: , A.M.MUKHAMEDZANOV, A.I.MUKHAMEDZHANOV, A.M.MUKHAMEDZHANOV