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Mualliflar

S. A. Turakulov

Soʻnggi maʼlum muassasa:
Oʻzbekiston Respublikasi Fanlar Akademiyasi
ORCID:
0000-0002-9067-7618
5
h-indeks
1
i10-indeksi
53
Iqtiboslar
19
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0134503581020162018201920202021202220232024202520262016: Nashrlar 1, Iqtiboslar 12018: Nashrlar 2, Iqtiboslar 72019: Nashrlar 1, Iqtiboslar 82020: Nashrlar 3, Iqtiboslar 102021: Nashrlar 1, Iqtiboslar 62022: Nashrlar 1, Iqtiboslar 42023: Nashrlar 3, Iqtiboslar 62024: Nashrlar 2, Iqtiboslar 42025: Nashrlar 2, Iqtiboslar 72026: Nashrlar 1, Iqtiboslar 0

Iqtibos tarixi

03581020162018201920202021202220232024202520262016: Iqtiboslar 12018: Iqtiboslar 72019: Iqtiboslar 82020: Iqtiboslar 102021: Iqtiboslar 62022: Iqtiboslar 42023: Iqtiboslar 62024: Iqtiboslar 42025: Iqtiboslar 72026: Iqtiboslar 0

Nashr tarixi

0134520162018201920202021202220232024202520262016: Nashrlar 12018: Nashrlar 22019: Nashrlar 12020: Nashrlar 32021: Nashrlar 12022: Nashrlar 12023: Nashrlar 32024: Nashrlar 22025: Nashrlar 22026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520162018201920202021202220232024202520262016: 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 52026: 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

Hammualliflar

  1. E. M. Tursunov16 ta umumiy asar2015–2026
  2. A. S. Kadyrov8 ta umumiy asar2016–2025
  3. K. I. Tursunmakhatov2 ta umumiy asar2023
  4. I. Bray2 ta umumiy asar2016–2018
  5. D. S. Toshova1 ta umumiy asar2026
  6. E.M. Tursunov1 ta umumiy asar2024
  7. Tursunmakhatov, K. I.1 ta umumiy asar2024
  8. R. Yarmukhamedov1 ta umumiy asar2023
  9. S. V. Artemov1 ta umumiy asar2023
  10. L. D. Blokhintsev1 ta umumiy asar2021

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