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Mualliflar

E. M. Tursunov

Soʻnggi maʼlum muassasa:
Oʻzbekiston Respublikasi Fanlar Akademiyasi
ORCID:
0000-0003-4175-4151
6
h-indeks
2
i10-indeksi
94
Iqtiboslar
38
Asarlar
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Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

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  • Iqtiboslar
013450510152020162018201920202021202220232024202520262016: Nashrlar 1, Iqtiboslar 52018: Nashrlar 3, Iqtiboslar 162019: Nashrlar 2, Iqtiboslar 112020: Nashrlar 3, Iqtiboslar 152021: Nashrlar 2, Iqtiboslar 82022: Nashrlar 3, Iqtiboslar 102023: Nashrlar 2, Iqtiboslar 62024: Nashrlar 2, Iqtiboslar 42025: Nashrlar 2, Iqtiboslar 52026: Nashrlar 2, Iqtiboslar 1

Iqtibos tarixi

0510152020162018201920202021202220232024202520262016: Iqtiboslar 52018: Iqtiboslar 162019: Iqtiboslar 112020: Iqtiboslar 152021: Iqtiboslar 82022: Iqtiboslar 102023: Iqtiboslar 62024: Iqtiboslar 42025: Iqtiboslar 52026: Iqtiboslar 1

Nashr tarixi

0134520162018201920202021202220232024202520262016: Nashrlar 12018: Nashrlar 32019: Nashrlar 22020: Nashrlar 32021: Nashrlar 22022: Nashrlar 32023: Nashrlar 22024: Nashrlar 22025: Nashrlar 22026: Nashrlar 2

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020162018201920202021202220232024202520262016: h-indeks 22018: h-indeks 42019: h-indeks 52020: h-indeks 52021: h-indeks 62022: h-indeks 62023: h-indeks 62024: h-indeks 62025: h-indeks 62026: h-indeks 6

Eng koʻp iqtibos qilingan asarlar

  1. Analysis 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>6</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>β decay into the<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>d</mml:mi></mml:mrow></mml:math>continuum within a three-body model200615 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: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
  3. 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
  4. Theoretical analysis of the astrophysical S-factor for the capture reaction α + d → 6Li + γ in the two-body model20159 iqtibos
  5. Moscow-type<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>NN</mml:mi></mml:math>potentials and three-nucleon bound states19986 iqtibos
  6. Gamma-delayed deuteron emission of the halo state20075 iqtibos
  7. 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
  8. 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
  9. Analysis of the 3He(α,γ)7Be and 3H(α,γ)7Li astrophysical direct capture reactions in a modified potential-model approach20204 iqtibos
  10. 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

Hammualliflar

  1. S. A. Turakulov16 ta umumiy asar2015–2026
  2. D Baye10 ta umumiy asarSkelet yozuvlar: 12003–2020
  3. P. Descouvemont9 ta umumiy asarSkelet yozuvlar: 12003–2018
  4. A. S. Kadyrov9 ta umumiy asar2016–2025
  5. K. I. Tursunmakhatov2 ta umumiy asar2023
  6. I. Bray2 ta umumiy asar2016–2018
  7. S. Krewald2 ta umumiy asar2014
  8. Jurabek Khushvaktov1 ta umumiy asar2026
  9. M. Sh. Kayumova1 ta umumiy asar2026
  10. D. S. Toshova1 ta umumiy asar2026

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