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Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 2016-07, Vol.825, p.17-23

2016

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Determination of the 3 He( α , γ ) 7 Be and 6 Li( p , γ ) 7 Be astrophysical factors down to zero energy using the asymptotic normalization coefficients

EPJ Web of conferences, 2023, Vol.279, p.11001

2023

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Asymptotic normalization coefficients (nuclear vertex constants) for p + {sup 7}Be {yields} {sup 8}B and the direct {sup 7}Be(p, {gamma}){sup 8}B astrophysical S factors at solar energies

Physics of atomic nuclei, 2008-10, Vol.71 (10)

2008

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Extrapolation of astrophysical S factors for the reaction [sup.14]N[sup.15]O to near-zero energies

Physics of atomic nuclei, 2012-03, Vol.75 (3), p.291

2012

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

Physics of atomic nuclei, 2008-10, Vol.71 (10), p.1740-1755

2008

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

Physics of atomic nuclei, 2012-03, Vol.75 (3), p.291-309

2012

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

Physics of atomic nuclei, 2007-10, Vol.70 (10), p.1694-1705

2007

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Nuclear asymptotic normalization coefficients for {sup 14}N {sup {yields} 13}C + p configurations and astrophysical S factor for radiative proton capture

Physics of atomic nuclei, 2008-06, Vol.71 (6)

2008

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

Physics of atomic nuclei, 2008-06, Vol.71 (6), p.998-1011

2008

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Determination of nuclear vertex constants (asymptotic normalization coefficients) for the virtual decays ^sup 3^He [rarr] d + p and ^sup 17^F [rarr] ^sup 16^O + p and their use for extrapolating astrophysical S-factors of the radiative proton capture by the deuteron and the ^sup 16^O nucleus at very low energies

Bulletin of the Russian Academy of Sciences. Physics, 2009-02, Vol.73 (2), p.165

2009

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Determination of nuclear vertex constants (asymptotic normalization coefficients) for the virtual decays 3He → d + p and 17F → 16O + p and their use for extrapolating astrophysical S-factors of the radiative proton capture by the deuteron and the 16O nucleus at very low energies

Bulletin of the Russian Academy of Sciences. Physics, 2009-02, Vol.73 (2), p.165-170

2009

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Modificated activation method for measurement of the yield of the astrophysical reactions

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

Asymptotic normalization coefficient for 12C+p→13N from the 12C(10B,9Be)13N reaction and the 12C(p,γ)13N astrophysical S factor

Dispersion (asymptotic) theory of charged-particle transfer reactions and nuclear astrophysics

Determination of the astrophysical factor of the 3He(α,γ)7Be down to zero energy using the asymptotic normalization coefficient method

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

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

Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method

Erratum to “Modified two-body potential approach to the peripheral direct capture astrophysical a + A → B + γ reaction and asymptotic normalization coefficients” [Nucl. Phys. A 781 (2007) 247]

Asymptotic normalization coefficient for α+d →6Li from the peripheral direct capture d(α,γ)6 reaction and the astrophysical S factor at Big Bang energies

Asymptotic normalization coefficient for $${{}^{12}\mathrm{C}}+p\rightarrow {{}^{13}\mathrm{N}}$$ from the $^{12}{\mathrm{C}}({}^{10}\mathrm{B},{}^{9}{\mathrm{Be}}){}^{13}\mathrm{N}$$ reaction and the $^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$ astrophysical S factor

Determination of the astrophysical factor of the 3 He(α,γ) 7 Be down to zero energy using the asymptotic normalization coefficient method

Effects of t- and α-transfer on the spectroscopic information from the Li6(He3,d)Be7 reaction

A Modified activation method for reaction total cross section and yield measurements at low astrophysically relevant energies

Determination of the 3 He( α , γ ) 7 Be and 6 Li( p , γ ) 7 Be astrophysical factors down to zero energy using the asymptotic normalization coefficients

Asymptotic normalization coefficients (nuclear vertex constants) for p + {sup 7}Be {yields} {sup 8}B and the direct {sup 7}Be(p, {gamma}){sup 8}B astrophysical S factors at solar energies

Extrapolation of astrophysical S factors for the reaction [sup.14]N[sup.15]O to near-zero energies

Determination of the 3He(α, γ)7Be and 6Li(p, γ)7Be astrophysical factors down to zero energy using the asymptotic normalization coefficients

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

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

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

Nuclear asymptotic normalization coefficients for {sup 14}N {sup {yields} 13}C + p configurations and astrophysical S factor for radiative proton capture

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

Determination of nuclear vertex constants (asymptotic normalization coefficients) for the virtual decays 3He → d + p and 17F → 16O + p and their use for extrapolating astrophysical S-factors of the radiative proton capture by the deuteron and the 16O nucleus at very low energies

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