Asosiy kontentga oʻtish
AkademScholar

Mahsulotlar

Ishlab chiquvchilar uchun

AkademBasetez oradaDasturchilar API
Mualliflar

C. Spitaleri

Soʻnggi maʼlum muassasa:
Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud
ORCID:
0000-0001-6256-9727
5
h-indeks
1
i10-indeksi
53
Iqtiboslar
22
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0120510152020172018201920202021202220232024202520262017: Nashrlar 2, Iqtiboslar 22018: Nashrlar 0, Iqtiboslar 42019: Nashrlar 0, Iqtiboslar 22020: Nashrlar 2, Iqtiboslar 42021: Nashrlar 1, Iqtiboslar 42022: Nashrlar 0, Iqtiboslar 22023: Nashrlar 2, Iqtiboslar 112024: Nashrlar 0, Iqtiboslar 22025: Nashrlar 0, Iqtiboslar 42026: Nashrlar 0, Iqtiboslar 3

Iqtibos tarixi

0510152020172018201920202021202220232024202520262017: Iqtiboslar 22018: Iqtiboslar 42019: Iqtiboslar 22020: Iqtiboslar 42021: Iqtiboslar 42022: Iqtiboslar 22023: Iqtiboslar 112024: Iqtiboslar 22025: Iqtiboslar 42026: Iqtiboslar 3

Nashr tarixi

01220172018201920202021202220232024202520262017: Nashrlar 22018: Nashrlar 02019: Nashrlar 02020: Nashrlar 22021: Nashrlar 12022: Nashrlar 02023: Nashrlar 22024: Nashrlar 02025: Nashrlar 02026: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520172018201920202021202220232024202520262017: h-indeks 22018: h-indeks 22019: h-indeks 22020: 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. 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 method20217 iqtibos
  2. Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method20205 iqtibos
  3. Complex analysis of scattering 1p-shell nuclei in the framework of coupled channel method20161 iqtibos
  4. Few-body problems in nuclear astrophysics20050 iqtibos
  5. Indirect techniques in nuclear astrophysics20060 iqtibos
  6. Pole approximation validation in the study of the [sup 6]Li(d,α)[sup 4]He reaction20100 iqtibos
  7. Indirect techniques in nuclear astrophysics20100 iqtibos
  8. Indirect Study of the<sup>16</sup>O+<sup>16</sup>O Fusion Reaction Toward Stellar Energies by the Trojan Horse Method20160 iqtibos
  9. Scattering of 13C ions by 12C nuclei at energies close to the Coulomb barrier20160 iqtibos
  10. Measurements of the Elastic and Inelastic Scattering Cross Sections of <sup>13</sup>C Ions on <sup>12</sup>C Nuclei at the Near Coulomb Barrier Energy20170 iqtibos