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B. F. Irgaziev

Soʻnggi maʼlum muassasa:
National University of Uzbekistan
ORCID:
0000-0002-9829-2667
4
h-indeks
0
i10-indeksi
56
Iqtiboslar
41
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

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0134503581020152016201720182019202020222023202420252015: Nashrlar 1, Iqtiboslar 62016: Nashrlar 2, Iqtiboslar 52017: Nashrlar 1, Iqtiboslar 62018: Nashrlar 2, Iqtiboslar 102019: Nashrlar 0, Iqtiboslar 22020: Nashrlar 2, Iqtiboslar 12022: Nashrlar 1, Iqtiboslar 52023: Nashrlar 0, Iqtiboslar 22024: Nashrlar 2, Iqtiboslar 42025: Nashrlar 3, Iqtiboslar 3

Iqtibos tarixi

03581020152016201720182019202020222023202420252015: Iqtiboslar 62016: Iqtiboslar 52017: Iqtiboslar 62018: Iqtiboslar 102019: Iqtiboslar 22020: Iqtiboslar 12022: Iqtiboslar 52023: Iqtiboslar 22024: Iqtiboslar 42025: Iqtiboslar 3

Nashr tarixi

0134520152016201720182019202020222023202420252015: Nashrlar 12016: Nashrlar 22017: Nashrlar 12018: Nashrlar 22019: Nashrlar 02020: Nashrlar 22022: Nashrlar 12023: Nashrlar 02024: Nashrlar 22025: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520152016201720182019202020222023202420252015: h-indeks 22016: h-indeks 32017: h-indeks 32018: h-indeks 42019: h-indeks 42020: h-indeks 42022: h-indeks 42023: h-indeks 42024: h-indeks 42025: h-indeks 4

Eng koʻp iqtibos qilingan asarlar

  1. Effect of Coulomb forces on the position of the pole in the scattering amplitude and on its residue20105 iqtibos
  2. Algorithm for calculations of asymptotic nuclear coefficients using phase-shift data for charged-particle scattering20174 iqtibos
  3. Resonance-state properties from a phase shift analysis with the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math>-matrix pole method and the effective-range method20154 iqtibos
  4. Asymptotic normalization coefficients of resonant and bound states from the phase shifts for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mi>α</mml:mi></mml:mrow></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>12</mml:mn></mml:mmultiscripts></mml:mrow></mml:math>scattering20164 iqtibos
  5. Asymptotic normalization coefficients from the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<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>3</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>,<i>d</i>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Na</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>21</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction and astrophysical factor for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Na</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>21</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>20063 iqtibos
  6. Final State Three-Body Coulomb Effects in the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">P</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mn>208</mml:mn></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">B</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mi>p</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">P</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mn>208</mml:mn></mml:mmultiscripts></mml:math>Coulomb Breakup Reaction20033 iqtibos
  7. Determination of the direct capture contribution for<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">N</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>13</mml:mn></mml:mrow></mml:mmultiscripts><mml:mrow><mml:mo>(</mml:mo><mml:mrow><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow><mml:mo>)</mml:mo></mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>14</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math>from the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>14</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">N</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>13</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mi>p</mml:mi></mml:mrow></mml:math>asymptotic normalization coefficient20042 iqtibos
  8. Extracting the complex energy of broad resonances by the S-matrix pole method20111 iqtibos
  9. The resonance pole and the residue of the scattering amplitude while the Coulomb forces gradually decrease20091 iqtibos
  10. On the Direct Mechanism of Photodisintegration of the <sup>6</sup> Li Nucleus19890 iqtibos