Ushbu ishga iqtibos qilgan ishlar

8 ta ish

Ish: 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

1. 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

   MaqolaNuclear physics research studiesPhysical review. C20189 iqtibos

   ABIABI:AkademIndex/openalex/2018.article.000137

2. 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

   Q. I. Tursunmahatov, R. Yarmukhamedov

   MaqolaNuclear physics research studiesPhysical Review C20129 iqtibos

   ABIABI:AkademIndex/openalex/2026.other.178223

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

   G. Kiss, M. La Cognata, C. Spitaleri +38

   MaqolaNuclear physics research studiesPhysics Letters B20205 iqtibos

   ABIABI:AkademIndex/openalex/2020.article.000135

4. Astrophysical <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> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">H</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>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> direct capture reactions in a potential-model approach

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

   MaqolaNuclear physics research studiesPhysical review. C20185 iqtibos

   ABIABI:AkademIndex/openalex/2026.other.356326

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

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

   MaqolaNuclear physics research studiesNuclear Physics A20204 iqtibos

   ABIABI:AkademIndex/openalex/2020.article.000385

6. Indirect Methods and ANCs for Nuclear Astrophysics

   R. Yarmukhamedov, O. R. Tojiboev, S. V. Artemov

   MaqolaNuclear physics research studiesProceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)20170 iqtibos

   ABIABI:AkademIndex/openalex/2017.article.000562

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

   M. La Cognata, G. Kiss, R. Yarmukhamedov +38

   MaqolaNuclear physics research studiesEPJ Web of Conferences20230 iqtibos

   ABIABI:AkademIndex/openalex/2023.article.005771

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

   M. La Cognata, G. Kiss, R. Yarmukhamedov +38

   MaqolaNuclear physics research studiesJournal of Physics Conference Series20230 iqtibos

   ABIABI:AkademIndex/openalex/2023.article.010700