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Mualliflar

Y. Guo

Soʻnggi maʼlum muassasa:
University of Tsukuba
ORCID:
0000-0003-0299-7011
1
h-indeks
0
i10-indeksi
2
Iqtiboslar
5
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0120120142015201720182014: Nashrlar 2, Iqtiboslar 02015: Nashrlar 2, Iqtiboslar 12017: Nashrlar 0, Iqtiboslar 12018: Nashrlar 1, Iqtiboslar 0

Iqtibos tarixi

0120142015201720182014: Iqtiboslar 02015: Iqtiboslar 12017: Iqtiboslar 12018: Iqtiboslar 0

Nashr tarixi

01220142015201720182014: Nashrlar 22015: Nashrlar 22017: Nashrlar 02018: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0120142015201720182014: h-indeks 02015: h-indeks 12017: h-indeks 12018: h-indeks 1

Eng koʻp iqtibos qilingan asarlar

  1. Suppression of ϒ production in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi>d</mml:mi><mml:mo>+</mml:mo><mml:mtext>Au</mml:mtext></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif" overflow="scroll"><mml:mtext>Au</mml:mtext><mml:mo>+</mml:mo><mml:mtext>Au</mml:mtext></mml:math> collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si3.gif" overflow="scroll"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi>N</mml:mi><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>200</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext></mml:math>20141 iqtibos
  2. Energy dependence of acceptance-corrected dielectron excess mass spectrum at mid-rapidity in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mtext>Au</mml:mtext><mml:mo>+</mml:mo><mml:mtext>Au</mml:mtext></mml:math> collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si102.gif" overflow="scroll"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="italic">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>19.6</mml:mn></mml:math> and 200 GeV20151 iqtibos
  3. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi>J</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>ψ</mml:mi></mml:math> polarization in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif" overflow="scroll"><mml:mi>p</mml:mi><mml:mo>+</mml:mo><mml:mi>p</mml:mi></mml:math> collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si3.gif" overflow="scroll"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>200</mml:mn><mml:mtext> GeV</mml:mtext></mml:math> in STAR20140 iqtibos
  4. Di-hadron correlations with identified leading hadrons in 200 GeV Au + Au and d + Au collisions at STAR20150 iqtibos
  5. Transverse spin-dependent azimuthal correlations of charged pion pairs measured in p↑ + p collisions at s=500 GeV20180 iqtibos

Hammualliflar

Yana 5 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

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