Asosiy kontentga oʻtish
AkademScholar
Muassasalar

Joint Institute for Nuclear Astrophysics

Nom variantlari: JINA-CEE · Joint Institute for Nuclear Astrophysics Center for the Evolution of Elements

Davlat:
US
ROR:
https://ror.org/04kq4yy23
5
h-indeks
165
Iqtiboslar
54
Asarlar
83
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
01345025507510020172018201920202021202220232024202520262017: Nashrlar 2, Iqtiboslar 82018: Nashrlar 2, Iqtiboslar 62019: Nashrlar 1, Iqtiboslar 62020: Nashrlar 3, Iqtiboslar 92021: Nashrlar 3, Iqtiboslar 92022: Nashrlar 0, Iqtiboslar 32023: Nashrlar 3, Iqtiboslar 122024: Nashrlar 2, Iqtiboslar 82025: Nashrlar 2, Iqtiboslar 192026: Nashrlar 3, Iqtiboslar 51

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 82018: Iqtiboslar 62019: Iqtiboslar 62020: Iqtiboslar 92021: Iqtiboslar 92022: Iqtiboslar 32023: Iqtiboslar 122024: Iqtiboslar 82025: Iqtiboslar 192026: Iqtiboslar 51

Nashr tarixi

0134520172018201920202021202220232024202520262017: Nashrlar 22018: Nashrlar 22019: Nashrlar 12020: Nashrlar 32021: Nashrlar 32022: Nashrlar 02023: Nashrlar 32024: Nashrlar 22025: Nashrlar 22026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520172018201920202021202220232024202520262017: h-indeks 32018: h-indeks 32019: h-indeks 32020: h-indeks 42021: h-indeks 42022: h-indeks 42023: h-indeks 42024: h-indeks 42025: h-indeks 42026: h-indeks 5

Eng koʻp iqtibos qilingan asarlar

  1. Pair correlations in the neutrinoless double-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>β</mml:mi></mml:mrow></mml:math>decay candidate<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Te</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>130</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>20101 iqtibos
  2. A comparison of the cosmic-ray energy scales of Tunka-133 and KASCADE-Grande via their radio extensions Tunka-Rex and LOPES20161 iqtibos
  3. Long-range parity-nonconserving interaction19920 iqtibos
  4. β decay of neutron-rich Ca53-5620080 iqtibos
  5. A Monte Carlo study of the spectra from inhomogeneous accretion flow20170 iqtibos
  6. Asymptotic normalization coefficients for $α+ {}^{12}{\rm C}$ synthesis and the $S$-factor for ${}^{12}{\rm C}(α, \,γ){}^{16}{\rm O}$ radiative capture20230 iqtibos
  7. Asymptotic normalization coefficients for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>12</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> synthesis and the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>S</mml:mi></mml:math> factor for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>12</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><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:mrow></mml:math> radiative capture20240 iqtibos
  8. Enriched volatiles and refractories but deficient titanium on the day-side atmosphere of WASP-121b revealed by JWST/NIRISS20250 iqtibos
  9. Time-resolved protoplanetary disk physics in DQ Tau with JWST20250 iqtibos
  10. An Earth-sized planet on a 5.4 h orbit around a nearby K dwarf20260 iqtibos