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S. A. Turakulov

Soʻnggi maʼlum muassasa:
Tashkent State Agrarian University
ORCID:
0000-0002-9067-7618
5
h-indeks
1
i10-indeksi
53
Iqtiboslar
13
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

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0134503581020152016201820192020202120222023202420252015: Nashrlar 1, Iqtiboslar 02016: Nashrlar 1, Iqtiboslar 12018: Nashrlar 2, Iqtiboslar 72019: Nashrlar 1, Iqtiboslar 82020: Nashrlar 3, Iqtiboslar 102021: Nashrlar 1, Iqtiboslar 62022: Nashrlar 0, Iqtiboslar 42023: Nashrlar 2, Iqtiboslar 62024: Nashrlar 1, Iqtiboslar 42025: Nashrlar 1, Iqtiboslar 7

Iqtibos tarixi

03581020152016201820192020202120222023202420252015: Iqtiboslar 02016: Iqtiboslar 12018: Iqtiboslar 72019: Iqtiboslar 82020: Iqtiboslar 102021: Iqtiboslar 62022: Iqtiboslar 42023: Iqtiboslar 62024: Iqtiboslar 42025: Iqtiboslar 7

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0134520152016201820192020202120222023202420252015: Nashrlar 12016: Nashrlar 12018: Nashrlar 22019: Nashrlar 12020: Nashrlar 32021: Nashrlar 12022: Nashrlar 02023: Nashrlar 22024: Nashrlar 12025: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520152016201820192020202120222023202420252015: h-indeks 02016: h-indeks 12018: h-indeks 22019: h-indeks 32020: h-indeks 32021: h-indeks 42022: h-indeks 42023: h-indeks 42024: h-indeks 42025: h-indeks 5

Eng koʻp iqtibos qilingan asarlar

  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: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 model201612 iqtibos
  2. 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 abundance20189 iqtibos
  3. Theoretical analysis of the astrophysical S-factor for the capture reaction α + d → 6Li + γ in the two-body model20159 iqtibos
  4. Detailed study of the astrophysical direct capture reaction <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>p</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> in a potential model approach20235 iqtibos
  5. 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 approach20185 iqtibos
  6. Analysis of the 3He(α,γ)7Be and 3H(α,γ)7Li astrophysical direct capture reactions in a modified potential-model approach20204 iqtibos
  7. Astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor and rate of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> direct capture reaction in a potential model20213 iqtibos
  8. Comparative study of the direct <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"><mml:mi>α</mml:mi><mml:mo linebreak="goodbreak" linebreakstyle="after">+</mml:mo><mml:mi>d</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:msup><mml:mrow/><mml:mrow><mml:mn>6</mml:mn></mml:mrow></mml:msup><mml:mtext>Li</mml:mtext><mml:mo linebreak="goodbreak" linebreakstyle="after">+</mml:mo><mml:mi>γ</mml:mi></mml:math> astrophysical capture reaction in few-body models20203 iqtibos
  9. Analysis of the 12C(3He, d)13N Proton Stripping Reaction to the Resonant State20231 iqtibos
  10. Study of the direct 16O(p,γ)17F astrophysical capture reaction within a potential model approach20241 iqtibos
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