Ushbu ish iqtibos qilgan ishlar
50 ta ish
Ish: Determination of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mn mathvariant="bold">3</mml:mn></mml:mrow></mml:msup><mml:mi mathvariant="normal">He</mml:mi><mml:mo>+</mml:mo><mml:mi>α</mml:mi><mml:mo>→</mml:mo><mml:msup><mml:mrow/><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>Be asymptotic normalization coefficients, the nuclear vertex constants, and their application for the extrapolation of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mn mathvariant="bold">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>He(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow><mml:mi mathvariant="bold-italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="bold">γ</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mn mathvariant="bold">7</mml:mn></mml:msup></mml:math>Be astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="bold-italic">S</mml:mi></mml:math>factors to the solar energy region
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Be</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>cross section at low energies
Gy. Gyürky, F. Confortola, H. Costantini +27
Maqola20074 iqtibosABIScattering of 3He and 4He from polarized 3He between 4 and 10 MeV
W.R. Boykin, S. Baker, D.M. Hardy
Maqola19724 iqtibosABIClusters as Subsystems in Light Nuclei
V. I. Kukulin, V. G. Neudatchin, I. T. Obukhovski +1
Bob19833 iqtibosABIScattering of 3He and 4He from polarized 3He between 7 and 18 MeV
D.M. Hardy, R. J. Spiger, S. Baker +2
Maqola19723 iqtibosABI<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>4</mml:mn></mml:mrow></mml:mmultiscripts></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mo>→</mml:mo></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Be</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>S</mml:mi></mml:mrow></mml:math>factor
T. A. D. Brown, C. Bordeanu, K. A. Snover +5
Maqola20073 iqtibosABIErratum to “Modified two-body potential approach to the peripheral direct capture astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi>a</mml:mi><mml:mo>+</mml:mo><mml:mi>A</mml:mi><mml:mo>→</mml:mo><mml:mi>B</mml:mi><mml:mo>+</mml:mo><mml:mi>γ</mml:mi></mml:math> reaction and asymptotic normalization coefficients” [Nucl. Phys. A 781 (2007) 247]
S. B. Igamov, R. Yarmukhamedov
Boshqa20093 iqtibosABIThe3He(?,?)7Be reaction and the solar neutrino problem
H. Kr�winkel, Harry Becker, L. Buchmann +11
Maqola19822 iqtibosABI