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AkademScholar

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Identifikatsiya

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Ekotizim

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Sicilian Center of Nuclear Physics and Physics of Matter

Nom variantlari: Centro Siciliano di Fisica Nucleare e di Struttura della Materia · INFN Centro Siciliano di Fisica Nucleare e di Struttura della Materia · INFN-CSFNSM

Davlat:
IT
ROR:
https://ror.org/02wdzfm91
5
h-indeks
66
Iqtiboslar
21
Asarlar
22
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0120510152020172018201920202021202220232024202520262017: Nashrlar 0, Iqtiboslar 42018: Nashrlar 1, Iqtiboslar 132019: Nashrlar 1, Iqtiboslar 52020: Nashrlar 1, Iqtiboslar 12021: Nashrlar 1, Iqtiboslar 22022: Nashrlar 0, Iqtiboslar 42023: Nashrlar 2, Iqtiboslar 132024: Nashrlar 1, Iqtiboslar 32025: Nashrlar 0, Iqtiboslar 52026: Nashrlar 1, Iqtiboslar 2

Iqtibos tarixi

0510152020172018201920202021202220232024202520262017: Iqtiboslar 42018: Iqtiboslar 132019: Iqtiboslar 52020: Iqtiboslar 12021: Iqtiboslar 22022: Iqtiboslar 42023: Iqtiboslar 132024: Iqtiboslar 32025: Iqtiboslar 52026: Iqtiboslar 2

Nashr tarixi

01220172018201920202021202220232024202520262017: Nashrlar 02018: Nashrlar 12019: Nashrlar 12020: Nashrlar 12021: Nashrlar 12022: Nashrlar 02023: Nashrlar 22024: Nashrlar 12025: Nashrlar 02026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520172018201920202021202220232024202520262017: h-indeks 32018: h-indeks 32019: h-indeks 32020: h-indeks 32021: h-indeks 32022: h-indeks 32023: h-indeks 42024: h-indeks 42025: h-indeks 52026: h-indeks 5

Eng koʻp iqtibos qilingan asarlar

  1. Investigation of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow/><mml:mn>48</mml:mn></mml:msup></mml:math>Ca + <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow/><mml:mrow><mml:mn>249</mml:mn><mml:mo>–</mml:mo><mml:mn>252</mml:mn></mml:mrow></mml:msup></mml:math>Cf reactions synthesizing isotopes of the superheavy element 118201220 iqtibos
  2. Main restrictions in the synthesis of new superheavy elements: Quasifission and/or fusion fission201312 iqtibos
  3. 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
  4. Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method20205 iqtibos
  5. Processes in massive nuclei reactions and the way to complete fusion of reactants. What perspectives for the synthesis of heavier superheavy elements?20122 iqtibos
  6. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  7. Basic distinctions between cold- and hot-fusion reactions in the synthesis of superheavy elements20141 iqtibos
  8. What perspectives for the synthesis of heavier superheavy nuclei? Results and comparison with models20130 iqtibos
  9. Reaction mechanisms in massive nuclei collisions and perspectives for synthesis of heavier superheavy elements20130 iqtibos
  10. Difference in evaporation residue yields in the cold and hot fusion reactions20140 iqtibos