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E. M. Tursunov

Soʻnggi maʼlum muassasa:
Academy of Sciences Republic of Uzbekistan
ORCID:
0000-0003-4175-4151
5
h-indeks
2
i10-indeksi
89
Iqtiboslar
29
Asarlar
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013450510152020162018201920202021202220232024202520262016: Nashrlar 1, Iqtiboslar 52018: Nashrlar 3, Iqtiboslar 162019: Nashrlar 2, Iqtiboslar 112020: Nashrlar 3, Iqtiboslar 152021: Nashrlar 2, Iqtiboslar 82022: Nashrlar 2, Iqtiboslar 102023: Nashrlar 1, Iqtiboslar 62024: Nashrlar 0, Iqtiboslar 42025: Nashrlar 1, Iqtiboslar 52026: Nashrlar 1, Iqtiboslar 0

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0510152020162018201920202021202220232024202520262016: Iqtiboslar 52018: Iqtiboslar 162019: Iqtiboslar 112020: Iqtiboslar 152021: Iqtiboslar 82022: Iqtiboslar 102023: Iqtiboslar 62024: Iqtiboslar 42025: Iqtiboslar 52026: Iqtiboslar 0

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0134520162018201920202021202220232024202520262016: Nashrlar 12018: Nashrlar 32019: Nashrlar 22020: Nashrlar 32021: Nashrlar 22022: Nashrlar 22023: Nashrlar 12024: Nashrlar 02025: Nashrlar 12026: Nashrlar 1

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0134520162018201920202021202220232024202520262016: h-indeks 22018: h-indeks 42019: h-indeks 42020: h-indeks 52021: h-indeks 52022: h-indeks 52023: h-indeks 52024: h-indeks 52025: h-indeks 52026: h-indeks 5

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 model200614 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. Gamma-delayed deuteron emission of the halo state20075 iqtibos
  6. 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 states19985 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
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