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S. V. Artemov

Ism variantlari: S V Artemov

Soʻnggi maʼlum muassasa:
Academy of Sciences Republic of Uzbekistan
ORCID:
0000-0001-8181-9672
4
h-indeks
0
i10-indeksi
60
Iqtiboslar
45
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

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  • Iqtiboslar
0134503581020172018201920202021202220232024202520262017: Nashrlar 2, Iqtiboslar 12018: Nashrlar 0, Iqtiboslar 32019: Nashrlar 1, Iqtiboslar 12020: Nashrlar 2, Iqtiboslar 22021: Nashrlar 0, Iqtiboslar 32022: Nashrlar 1, Iqtiboslar 52023: Nashrlar 1, Iqtiboslar 22024: Nashrlar 4, Iqtiboslar 102025: Nashrlar 1, Iqtiboslar 82026: Nashrlar 1, Iqtiboslar 6

Iqtibos tarixi

03581020172018201920202021202220232024202520262017: Iqtiboslar 12018: Iqtiboslar 32019: Iqtiboslar 12020: Iqtiboslar 22021: Iqtiboslar 32022: Iqtiboslar 52023: Iqtiboslar 22024: Iqtiboslar 102025: Iqtiboslar 82026: Iqtiboslar 6

Nashr tarixi

0134520172018201920202021202220232024202520262017: Nashrlar 22018: Nashrlar 02019: Nashrlar 12020: Nashrlar 22021: Nashrlar 02022: Nashrlar 12023: Nashrlar 12024: Nashrlar 42025: Nashrlar 12026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520172018201920202021202220232024202520262017: h-indeks 22018: h-indeks 22019: h-indeks 22020: h-indeks 22021: h-indeks 32022: h-indeks 32023: h-indeks 32024: h-indeks 42025: h-indeks 42026: h-indeks 4

Eng koʻp iqtibos qilingan asarlar

  1. Nuclear asymptotic normalization coefficients for 14N → 13C + p configurations and astrophysical S factor for radiative proton capture20089 iqtibos
  2. Determination of nuclear vertex constants (asymptotic normalization coefficients) for the virtual decays 3He → d + p and 17F → 16O + p and their use for extrapolating astrophysical S-factors of the radiative proton capture by the deuteron and the 16O nucleus at very low energies20098 iqtibos
  3. Asymptotic normalization coefficients for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mspace width="0.16em"/><mml:mo>+</mml:mo><mml:mspace width="0.16em"/><mml:mi>p</mml:mi><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> from the peripheral <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction and their astrophysical application20168 iqtibos
  4. Effects of t- and α-transfer on the spectroscopic information from the reaction20135 iqtibos
  5. Extrapolation of astrophysical S factors for the reaction 14N((p, γ) 15O to near-zero energies20124 iqtibos
  6. Asymptotic normalization coefficient for $${{}^{12}\mathrm{C}}+p\rightarrow {{}^{13}\mathrm{N}}$$ from the $${}^{12}{\mathrm{C}}({}^{10}\mathrm{B},{}^{9}{\mathrm{Be}}){}^{13}\mathrm{N}$$ reaction and the $${}^{12}\mathrm{C}(p,\gamma ){}^{13}\mathrm{N}$$ astrophysical S factor20224 iqtibos
  7. Deuteron scattering on 6Li at an energy of 25 MeV20103 iqtibos
  8. Proton-separation vertex constants for sd-shell nuclei from an analysis of peripheral transfer reactions20003 iqtibos
  9. Role of channel coupling and deuteron-exchange mechanisms in anomalous alpha-particle scattering on 6Li20092 iqtibos
  10. ESTIMATES OF THE ASTROPHYSICAL <font>S</font>-FACTORS FOR PROTON RADIATIVE CAPTURE BY <sup>10</sup><font>B</font> AND <sup>24</sup><font>Mg</font> NUCLEI USING THE ANCs FROM PROTON TRANSFER REACTIONS20102 iqtibos