Asosiy kontentga oʻtish
AkademScholar

Kashfiyot

Xizmatlar

Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud

Nom variantlari: INFN Laboratori Nazionali del Sud · LNS · Laboratori Nazionali del Sud · National Institute for Nuclear Physics, Laboratori Nazionali del Sud

Davlat:
IT
ROR:
https://ror.org/02k1zhm92
8
h-indeks
330
Iqtiboslar
92
Asarlar
199
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0134501325385020172018201920202021202220232024202520262017: Nashrlar 5, Iqtiboslar 112018: Nashrlar 5, Iqtiboslar 422019: Nashrlar 1, Iqtiboslar 172020: Nashrlar 4, Iqtiboslar 102021: Nashrlar 2, Iqtiboslar 212022: Nashrlar 3, Iqtiboslar 222023: Nashrlar 5, Iqtiboslar 432024: Nashrlar 0, Iqtiboslar 272025: Nashrlar 1, Iqtiboslar 262026: Nashrlar 1, Iqtiboslar 25

Iqtibos tarixi

01325385020172018201920202021202220232024202520262017: Iqtiboslar 112018: Iqtiboslar 422019: Iqtiboslar 172020: Iqtiboslar 102021: Iqtiboslar 212022: Iqtiboslar 222023: Iqtiboslar 432024: Iqtiboslar 272025: Iqtiboslar 262026: Iqtiboslar 25

Nashr tarixi

0134520172018201920202021202220232024202520262017: Nashrlar 52018: Nashrlar 52019: Nashrlar 12020: Nashrlar 42021: Nashrlar 22022: Nashrlar 32023: Nashrlar 52024: Nashrlar 02025: Nashrlar 12026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 52018: h-indeks 52019: h-indeks 52020: h-indeks 52021: h-indeks 62022: h-indeks 72023: h-indeks 72024: h-indeks 72025: h-indeks 72026: h-indeks 8

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 method20218 iqtibos
  2. GRANDMA observations of ZTF/<i>Fink</i> transients during summer 202120227 iqtibos
  3. GRANDMA and HXMT Observations of GRB 221009A: The Standard Luminosity Afterglow of a Hyperluminous Gamma-Ray Burst—In Gedenken an David Alexander Kann20236 iqtibos
  4. Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method20205 iqtibos
  5. Comprehensive analysis of high-lying states in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>18</mml:mn></mml:mmultiscripts></mml:math> populated with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mo>(</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>18</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></mml:mmultiscripts><mml:mo>)</mml:mo></mml:mrow></mml:math> reactions20174 iqtibos
  6. Two-neutron transfer analysis of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>18</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></mml:mmultiscripts><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>18</mml:mn></mml:mmultiscripts></mml:mrow></mml:math>reaction20163 iqtibos
  7. RBS analysis of ions implanted in light substrates exposed to hot plasmas laser-generated at PALS20050 iqtibos
  8. Few-body problems in nuclear astrophysics20050 iqtibos
  9. Indirect techniques in nuclear astrophysics20060 iqtibos
  10. STUDIES OF EXOTIC SYSTEMS USING TRANSFER REACTIONS AT GANIL20080 iqtibos