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AkademScholar

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Czech Academy of Sciences, Nuclear Physics Institute

Nom variantlari: Czech Acad Sci, Nucl Phys Inst · Nuclear Physics Institute CAS · Nuclear Physics Institute of the Czech Academy of Sciences · ÚJF AV ČR · Ústav jaderné fyziky AV ČR · Ústav jaderné fyziky AV ČR, v. v. i. · Ústav jaderné fyziky AV ČR, veřejná výzkumná instituce

Davlat:
CZ
ROR:
https://ror.org/04jymbd90
10
h-indeks
847
Iqtiboslar
407
Asarlar
418
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
05101520025507510020172018201920202021202220232024202520262017: Nashrlar 9, Iqtiboslar 272018: Nashrlar 9, Iqtiboslar 342019: Nashrlar 12, Iqtiboslar 262020: Nashrlar 17, Iqtiboslar 282021: Nashrlar 20, Iqtiboslar 582022: Nashrlar 9, Iqtiboslar 602023: Nashrlar 10, Iqtiboslar 582024: Nashrlar 16, Iqtiboslar 932025: Nashrlar 4, Iqtiboslar 342026: Nashrlar 6, Iqtiboslar 26

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 272018: Iqtiboslar 342019: Iqtiboslar 262020: Iqtiboslar 282021: Iqtiboslar 582022: Iqtiboslar 602023: Iqtiboslar 582024: Iqtiboslar 932025: Iqtiboslar 342026: Iqtiboslar 26

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 92018: Nashrlar 92019: Nashrlar 122020: Nashrlar 172021: Nashrlar 202022: Nashrlar 92023: Nashrlar 102024: Nashrlar 162025: Nashrlar 42026: Nashrlar 6

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 62018: h-indeks 72019: h-indeks 72020: h-indeks 72021: h-indeks 82022: h-indeks 82023: h-indeks 92024: h-indeks 92025: h-indeks 102026: h-indeks 10

Eng koʻp iqtibos qilingan asarlar

  1. Experimental electron binding energies for thulium in different matrices20159 iqtibos
  2. Indirect determination of the astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor for the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><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> reaction using the asymptotic normalization coefficient method20218 iqtibos
  3. Influence of host matrices on krypton electron binding energies and KLL Auger transition energies20147 iqtibos
  4. Search for environmental effects on the KLL Auger spectrum of rubidium generated in radioactive decay20156 iqtibos
  5. Three-Hilbert-Space Formulation of Quantum Mechanics20096 iqtibos
  6. Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method20205 iqtibos
  7. Theoretical analysis of experimental data on 160Dy that were obtained in studying beta decay20105 iqtibos
  8. A Hardy Inequality in Twisted Waveguides20084 iqtibos
  9. Improved characteristics of the 22.5 keV (M1 + E2) nuclear transition in 149Sm20114 iqtibos
  10. The first observation of all the basic components of the KLL Auger spectrum of Sm generated in the radioactive decay of 147,148,149Eu atoms in a solid state source20114 iqtibos