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Physical review. C

ISSN:
2469-9985
6
h-indeks
117
Iqtiboslar
68
Asarlar

Ishonch signallari

1 dan 3 signal mavjud

Mustaqil ijobiy signallar — yagona “predator/qonuniy” hukmi emas, balki yaqinlashuvchi tasvir.

  • DOAJ
    Maʼlumot yoʻq
    doaj.org
  • OAK roʻyxati
    Maʼlumot yoʻq
    OAK
  • Yaroqli ISSN
    Mavjud
    ISSN

Bu axborot yorligʻi, rasmiy qaror emas. Signal yoʻqligi jazo emas — masalan, mintaqaviy jurnal DOAJ'da boʻlmasligi mumkin.

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Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
051015200613192520172018201920202021202220232024202520262017: Nashrlar 3, Iqtiboslar 22018: Nashrlar 8, Iqtiboslar 152019: Nashrlar 1, Iqtiboslar 92020: Nashrlar 0, Iqtiboslar 82021: Nashrlar 5, Iqtiboslar 62022: Nashrlar 1, Iqtiboslar 72023: Nashrlar 4, Iqtiboslar 152024: Nashrlar 10, Iqtiboslar 222025: Nashrlar 20, Iqtiboslar 182026: Nashrlar 5, Iqtiboslar 15

Iqtibos tarixi

0613192520172018201920202021202220232024202520262017: Iqtiboslar 22018: Iqtiboslar 152019: Iqtiboslar 92020: Iqtiboslar 82021: Iqtiboslar 62022: Iqtiboslar 72023: Iqtiboslar 152024: Iqtiboslar 222025: Iqtiboslar 182026: Iqtiboslar 15

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 32018: Nashrlar 82019: Nashrlar 12020: Nashrlar 02021: Nashrlar 52022: Nashrlar 12023: Nashrlar 42024: Nashrlar 102025: Nashrlar 202026: Nashrlar 5

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 12018: h-indeks 32019: h-indeks 32020: h-indeks 32021: h-indeks 42022: h-indeks 42023: h-indeks 52024: h-indeks 52025: h-indeks 52026: h-indeks 6

Eng koʻp iqtibos qilingan asarlar

  1. Analysis of the fusion mechanism in the synthesis of superheavy element 119 via the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Cr</mml:mi><mml:mprescripts/><mml:none/><mml:mn>54</mml:mn></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mspace width="4pt"/><mml:mmultiscripts><mml:mi>Am</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>243</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math> reaction202212 iqtibos
  2. Theoretical study of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mi>d</mml:mi><mml:mo>→</mml:mo><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">Li</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>6</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow><mml:mo>+</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>astrophysical capture process in a three-body model201612 iqtibos
  3. Theoretical study of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mi>d</mml:mi><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts></mml:mrow><mml:mo>+</mml:mo><mml:mi>γ</mml:mi></mml:math> astrophysical capture process in a three-body model. II. Reaction rates and primordial abundance20189 iqtibos
  4. 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
  5. Asymptotic normalization coefficients for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mspace width="0.16em"/><mml:mo>+</mml:mo><mml:mspace width="0.16em"/><mml:mi>p</mml:mi><mml:mo>→</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> from the peripheral <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">B</mml:mi><mml:mprescripts/><mml:none/><mml:mn>8</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> reaction and their astrophysical application20168 iqtibos
  6. Optimal colliding energy for the synthesis of a superheavy element with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>Z</mml:mi><mml:mo>=</mml:mo><mml:mn>119</mml:mn></mml:mrow></mml:math>20246 iqtibos
  7. Detailed study of the astrophysical direct capture reaction <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>6</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><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> in a potential model approach20235 iqtibos
  8. Astrophysical <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</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>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mmultiscripts><mml:mi mathvariant="normal">H</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</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>Li</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> direct capture reactions in a potential-model approach20185 iqtibos
  9. 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
  10. Algorithm for calculations of asymptotic nuclear coefficients using phase-shift data for charged-particle scattering20174 iqtibos
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