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Иш: Analysis of the 3He(α,γ)7Be and 3H(α,γ)7Li astrophysical direct capture reactions in a modified potential-model approach

1. <i>Planck</i>2015 results

   P. A. R. Ade, N. Aghanim, M. Arnaud +97

   Мақола201631 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.002602

2. A compilation of charged-particle induced thermonuclear reaction rates

   C. Angulo, M. Arnould, M. Rayet +25

   Мақола199930 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.171531

3. Solar fusion cross sections. II. The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mi>p</mml:mi></mml:math>chain and CNO cycles

   E. G. Adelberger, A. Garcı́a, R. G. H. Robertson +44

   Мақола201115 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.178227

4. NACRE II: an update of the NACRE compilation of charged-particle-induced thermonuclear reaction rates for nuclei with mass number <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi>A</mml:mi><mml:mo>&lt;</mml:mo><mml:mn>16</mml:mn></mml:math>

   Y. Xu, K. Takahashi, S. Goriely +3

   Мақола201314 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.197450

5. Primordial<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mi>d</mml:mi><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mspace width="0.16em"/><mml:mi>γ</mml:mi></mml:mrow></mml:math>reaction and second lithium puzzle

   A. M. Mukhamedzhanov, R. Chatterjee Shubhchintak, C. A. Bertulani

   Мақола201612 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.191678

6. Theoretical study of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mi>d</mml:mi><mml:mo>→</mml:mo><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">Li</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>6</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow><mml:mo>+</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>astrophysical capture process in a three-body model

   E. M. Tursunov, A. S. Kadyrov, S. A. Turakulov +1

   МақолаNuclear physics research studiesPhysical review. C201612 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.191680

7. Isospin-forbidden electric dipole capture and the <i>α</i> ( <i>d</i> , <i>γ</i> ) ⁶ Li reaction

   D Baye, E M Tursunov

   МақолаNuclear physics research studiesJournal of Physics G Nuclear and Particle Physics201811 иқтибос

   ABIABI:AkademIndex/openalex/2018.article.000068

8. Compilation and R-matrix analysis of Big Bang nuclear reaction rates

   Pierre Descouvemont, Abderrahim Adahchour, Carmen Angulo +2

   Мақола200411 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.171526

9. Theoretical study of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mi>d</mml:mi><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts></mml:mrow><mml:mo>+</mml:mo><mml:mi>γ</mml:mi></mml:math> astrophysical capture process in a three-body model. II. Reaction rates and primordial abundance

   E. M. Tursunov, S. A. Turakulov, A. S. Kadyrov +1

   МақолаNuclear physics research studiesPhysical review. C20189 иқтибос

   ABIABI:AkademIndex/openalex/2018.article.000137

10. Review of Particle Physics

    Masaharu Tanabashi, Katsuro Hagiwara, Ken‐ichi Hikasa +97

    Мақола20189 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.027550

11. Theoretical analysis of the astrophysical S-factor for the capture reaction α + d → 6Li + γ in the two-body model

    E. M. Tursunov, S. A. Turakulov, P. Descouvemont

    МақолаNuclear physics research studiesPhysics of Atomic Nuclei20159 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.191672

12. First Direct Measurement of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mrow><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">H</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mrow><mml:mi>Li</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>6</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:mrow></mml:math>Cross Section at Big Bang Energies and the Primordial Lithium Problem

    M. Anders, D. Trezzi, R. Menegazzo +26

    Мақола20149 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.191674

13. Lithium Isotopic Abundances in Metal‐poor Halo Stars

    Martin Asplund, David L. Lambert, Poul Erik Nissen +2

    Мақола20069 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.192824

14. Сарлавҳасиз

    Бошқа9 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.356330

15. Microscopic Calculation of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="bold">H</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math>Capture Cross Sections Using Realistic Interactions

    Thomas Neff

    Мақола20118 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.178230

16. Astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>S</mml:mi></mml:math>factor of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow/><mml:mn>3</mml:mn></mml:msup></mml:math>He<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow><mml:mo>(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mn>7</mml:mn></mml:msup></mml:math>Be

    A. Kontos, E. Uberseder, R. J. deBoer +5

    Мақола20138 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.178246

17. Radiative alpha-capture rates leading to A - 7 nuclei - Applications to the solar neutrino problem and Big Bang nucleosynthesis

    Toshitaka Kajino, Sam M. Austin, H. Toki

    Мақола19877 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.154211

18. Radiative<i>α</i>-capture cross sections from realistic nucleon-nucleon interactions and variational Monte Carlo wave functions

    Kenneth M. Nollett

    Мақола20017 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.171509

19. Stellar and Primordial Nucleosynthesis of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math>: Measurement of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math>

    A. Di Leva, L. Gialanella, R. Kunz +16

    Мақола20097 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.178219

20. Lithium isotopic abundances in metal-poor halo stars

    Asplund, M, Lambert, D L, Nissen, P E +2

    Мақола20057 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.356331

21. Compilation and R-matrix analysis of Big Bang nuclear reaction rates

    Descouvemont, Pierre, Adahchour, Abderrahim, Angulo, Carmen +2

    Мақола20046 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.171556

22. Activation measurement of the reaction cross section at high energies

    C. Bordeanu, Gy. Gyürky, Z. Halász +6

    Мақола20136 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.178218

23. 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 of the<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>reaction measured at low energy via detection of prompt and delayed γ rays

    F. Confortola, D. Bemmerer, H. Costantini +28

    Мақола20076 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.178220

24. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">He</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">Be</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:mmultiscripts></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif" overflow="scroll"><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">H</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">Li</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:mmultiscripts></mml:math> astrophysical S factors from the no-core shell model with continuum

    Jérémy Dohet-Eraly, P. Navrátil, Sofia Quaglioni +3

    Мақола20166 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.178224

25. Cross section of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> around the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math> proton separation threshold

    T. Szücs, G. Kiss, Gy. Gyürky +3

    Мақола20196 иқтибос

    ABIABI:AkademIndex/openalex/2026.other.178253