Skip to content
AkademScholar

Products

For developers

AkademBasesoonDeveloper API
Authors

V. Burjan

Last known institution:
Institute of Nuclear Physics
ORCID:
0000-0001-8248-3883
5
h-index
2
i10-index
94
Citations
23
Works
Trends over time

Performance over time

Citation overview

Publications (bars) and citations (line) by year

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

Citation history

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

Publication history

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

h-index evolution

Cumulative h-index by year

0134520172018201920202021202220232024202520262017: h-index 52018: h-index 52019: h-index 52020: h-index 52021: h-index 52022: h-index 52023: h-index 52024: h-index 52025: h-index 52026: h-index 5

Most-cited works

  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 citations
  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 citations
  3. The nuclear fluctuation width and the method of maxima in excitation curves19880 citations
  4. Asymptotic normalization coefficients and astrophysical radiative capture reactions19980 citations
  5. Indirect techniques in nuclear astrophysics20060 citations
  6. Pole approximation validation in the study of the [sup 6]Li(d,α)[sup 4]He reaction20100 citations
  7. Indirect techniques in nuclear astrophysics20100 citations
  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 citations
  9. New insight into the cluster structure of 9Be by reactions with deuteron beam20170 citations
  10. REACTIONS 11B+209BI AT ENERGIES ABOVE COULOMB BARRIER20180 citations
View in AkademIndex →