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V. Burjan

Soʻnggi maʼlum muassasa:
Institute of Nuclear Physics
ORCID:
0000-0001-8248-3883
5
h-indeks
2
i10-indeksi
94
Iqtiboslar
23
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
010134520172018201920202021202220232024202520262017: Nashrlar 1, Iqtiboslar 22018: Nashrlar 1, Iqtiboslar 32019: Nashrlar 0, Iqtiboslar 12020: Nashrlar 0, Iqtiboslar 42021: Nashrlar 0, Iqtiboslar 32022: Nashrlar 0, Iqtiboslar 22023: Nashrlar 0, Iqtiboslar 52024: Nashrlar 0, Iqtiboslar 52025: Nashrlar 0, Iqtiboslar 42026: Nashrlar 0, Iqtiboslar 3

Iqtibos tarixi

0134520172018201920202021202220232024202520262017: Iqtiboslar 22018: Iqtiboslar 32019: Iqtiboslar 12020: Iqtiboslar 42021: Iqtiboslar 32022: Iqtiboslar 22023: Iqtiboslar 52024: Iqtiboslar 52025: Iqtiboslar 42026: Iqtiboslar 3

Nashr tarixi

0120172018201920202021202220232024202520262017: Nashrlar 12018: Nashrlar 12019: Nashrlar 02020: Nashrlar 02021: Nashrlar 02022: Nashrlar 02023: Nashrlar 02024: Nashrlar 02025: Nashrlar 02026: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520172018201920202021202220232024202520262017: h-indeks 52018: h-indeks 52019: h-indeks 52020: 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. 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
  2. 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
  3. The nuclear fluctuation width and the method of maxima in excitation curves19880 iqtibos
  4. Asymptotic normalization coefficients and astrophysical radiative capture reactions19980 iqtibos
  5. Indirect techniques in nuclear astrophysics20060 iqtibos
  6. Pole approximation validation in the study of the [sup 6]Li(d,α)[sup 4]He reaction20100 iqtibos
  7. Indirect techniques in nuclear astrophysics20100 iqtibos
  8. Some Insights into Cluster Structure of &amp;lt;sup&amp;gt;9&amp;lt;/sup&amp;gt;Be from &amp;lt;sup&amp;gt;3&amp;lt;/sup&amp;gt;He + &amp;lt;sup&amp;gt;9&amp;lt;/sup&amp;gt;Be Reaction20150 iqtibos
  9. New insight into the cluster structure of 9Be by reactions with deuteron beam20170 iqtibos
  10. REACTIONS 11B+209BI AT ENERGIES ABOVE COULOMB BARRIER20180 iqtibos
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