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Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Mualliflar

V. Burjan

Ism variantlari: Vaclav Burjan

Soʻnggi maʼlum muassasa:
National Research Nuclear University MEPhI
ORCID:
0000-0001-8248-3883
5
h-indeks
2
i10-indeksi
99
Iqtiboslar
24
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0103581020172018201920202021202220232024202520262017: Nashrlar 1, Iqtiboslar 22018: Nashrlar 1, Iqtiboslar 32019: Nashrlar 0, Iqtiboslar 12020: Nashrlar 0, Iqtiboslar 42021: Nashrlar 0, Iqtiboslar 32022: Nashrlar 0, Iqtiboslar 32023: Nashrlar 0, Iqtiboslar 52024: Nashrlar 0, Iqtiboslar 52025: Nashrlar 0, Iqtiboslar 42026: Nashrlar 0, Iqtiboslar 7

Iqtibos tarixi

03581020172018201920202021202220232024202520262017: Iqtiboslar 22018: Iqtiboslar 32019: Iqtiboslar 12020: Iqtiboslar 42021: Iqtiboslar 32022: Iqtiboslar 32023: Iqtiboslar 52024: Iqtiboslar 52025: Iqtiboslar 42026: Iqtiboslar 7

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. Comparative analysis of (p, d), (d, t) and (3He, α) reactions on13C nucleus19900 iqtibos
  5. Asymptotic normalization coefficients and astrophysical radiative capture reactions19980 iqtibos
  6. Indirect techniques in nuclear astrophysics20060 iqtibos
  7. Pole approximation validation in the study of the [sup 6]Li(d,α)[sup 4]He reaction20100 iqtibos
  8. Indirect techniques in nuclear astrophysics20100 iqtibos
  9. 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
  10. New insight into the cluster structure of 9Be by reactions with deuteron beam20170 iqtibos

Hammualliflar

  1. V. Kroha8 ta umumiy asar1998–2017
  2. A. M. Mukhamedzhanov6 ta umumiy asarSkelet yozuvlar: 121990–2010
  3. L. Trache5 ta umumiy asarSkelet yozuvlar: 111997–2010
  4. C. A. Gagliardi5 ta umumiy asar1998–2010
  5. R. E. Tribble5 ta umumiy asar1998–2010
  6. B. F. Irgaziev4 ta umumiy asarSkelet yozuvlar: 12004–2010
  7. Š. Piskoř4 ta umumiy asar1998–2015
  8. Xiaodong Tang3 ta umumiy asarSkelet yozuvlar: 61999–2010
  9. C. Spitaleri3 ta umumiy asarSkelet yozuvlar: 22006–2010
  10. R. G. Pizzone3 ta umumiy asarSkelet yozuvlar: 22006–2010

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