Asosiy kontentga oʻtish
AkademScholar
Muassasalar

Institute of Research into the Fundamental Laws of the Universe

Nom variantlari: Institut de Recherche sur les Lois Fondamentales de l'Univers · IRFU

Davlat:
FR
ROR:
https://ror.org/05k705z76
17
h-indeks
1,770
Iqtiboslar
369
Asarlar
452
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
025507510002505007501k20172018201920202021202220232024202520262017: Nashrlar 14, Iqtiboslar 272018: Nashrlar 12, Iqtiboslar 402019: Nashrlar 14, Iqtiboslar 212020: Nashrlar 28, Iqtiboslar 542021: Nashrlar 27, Iqtiboslar 582022: Nashrlar 16, Iqtiboslar 672023: Nashrlar 27, Iqtiboslar 1222024: Nashrlar 29, Iqtiboslar 2052025: Nashrlar 53, Iqtiboslar 7842026: Nashrlar 9, Iqtiboslar 281

Iqtibos tarixi

02505007501k20172018201920202021202220232024202520262017: Iqtiboslar 272018: Iqtiboslar 402019: Iqtiboslar 212020: Iqtiboslar 542021: Iqtiboslar 582022: Iqtiboslar 672023: Iqtiboslar 1222024: Iqtiboslar 2052025: Iqtiboslar 7842026: Iqtiboslar 281

Nashr tarixi

025507510020172018201920202021202220232024202520262017: Nashrlar 142018: Nashrlar 122019: Nashrlar 142020: Nashrlar 282021: Nashrlar 272022: Nashrlar 162023: Nashrlar 272024: Nashrlar 292025: Nashrlar 532026: Nashrlar 9

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0510152020172018201920202021202220232024202520262017: h-indeks 52018: h-indeks 52019: h-indeks 62020: h-indeks 72021: h-indeks 82022: h-indeks 82023: h-indeks 102024: h-indeks 112025: h-indeks 162026: h-indeks 17

Eng koʻp iqtibos qilingan asarlar

  1. DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations202536 iqtibos
  2. DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman alpha forest202524 iqtibos
  3. Decay of excited nuclei produced in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Kr</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>78</mml:mn><mml:mo>,</mml:mo><mml:mn>82</mml:mn></mml:mrow></mml:mmultiscripts></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Ca</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>40</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reactions at 5.5 MeV/nucleon201113 iqtibos
  4. DESI 2024 VII: cosmological constraints from the full-shape modeling of clustering measurements202511 iqtibos
  5. DESI 2024 II: sample definitions, characteristics, and two-point clustering statistics20259 iqtibos
  6. DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars20246 iqtibos
  7. DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars20246 iqtibos
  8. Euclid Quick Data Release (Q1)20256 iqtibos
  9. Cosmology and fundamental physics with the Euclid satellite20185 iqtibos
  10. DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data20255 iqtibos