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Identifikatsiya

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Ekotizim

Mualliflar

S. Gliske

Soʻnggi maʼlum muassasa:
Argonne National Laboratory
ORCID:
0000-0002-2259-2612
3
h-indeks
0
i10-indeksi
31
Iqtiboslar
15
Asarlar
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Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0134503581020112012201320142015201720182019202220252011: Nashrlar 1, Iqtiboslar 02012: Nashrlar 3, Iqtiboslar 02013: Nashrlar 3, Iqtiboslar 12014: Nashrlar 4, Iqtiboslar 22015: Nashrlar 2, Iqtiboslar 92017: Nashrlar 0, Iqtiboslar 42018: Nashrlar 0, Iqtiboslar 42019: Nashrlar 0, Iqtiboslar 22022: Nashrlar 0, Iqtiboslar 12025: Nashrlar 0, Iqtiboslar 8

Iqtibos tarixi

03581020112012201320142015201720182019202220252011: Iqtiboslar 02012: Iqtiboslar 02013: Iqtiboslar 12014: Iqtiboslar 22015: Iqtiboslar 92017: Iqtiboslar 42018: Iqtiboslar 42019: Iqtiboslar 22022: Iqtiboslar 12025: Iqtiboslar 8

Nashr tarixi

0134520112012201320142015201720182019202220252011: Nashrlar 12012: Nashrlar 32013: Nashrlar 32014: Nashrlar 42015: Nashrlar 22017: Nashrlar 02018: Nashrlar 02019: Nashrlar 02022: Nashrlar 02025: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520112012201320142015201720182019202220252011: h-indeks 02012: h-indeks 02013: h-indeks 12014: h-indeks 12015: h-indeks 22017: h-indeks 22018: h-indeks 22019: h-indeks 32022: h-indeks 32025: h-indeks 3

Eng koʻp iqtibos qilingan asarlar

  1. Di-electron spectrum at mid-rapidity in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>+</mml:mo><mml:mi>p</mml:mi></mml:mrow></mml:math>collisions at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>200</mml:mn></mml:mrow></mml:math>GeV20122 iqtibos
  2. 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
  3. Measurement of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>J</mml:mi><mml:mo>/</mml:mo><mml:mi>ψ</mml:mi></mml:math>Azimuthal Anisotropy in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>Au</mml:mi><mml:mo mathvariant="bold">+</mml:mo><mml:mi>Au</mml:mi></mml:math>Collisions at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msqrt><mml:msub><mml:mi>s</mml:mi><mml:mrow><mml:mi>N</mml:mi><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo mathvariant="bold">=</mml:mo><mml:mn>200</mml:mn><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>GeV</mml:mi></mml:math>20130 iqtibos
  4. Single spin asymmetry <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:msub><mml:mrow><mml:mi>A</mml:mi></mml:mrow><mml:mrow><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:math> in polarized proton–proton elastic scattering at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif" overflow="scroll"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>200</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext></mml:math>20130 iqtibos
  5. <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
  6. Isolation of flow and nonflow correlations by two- and four-particle cumulant measurements of azimuthal harmonics in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</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> Au+Au collisions20150 iqtibos
  7. Corrigendum to “Suppression of ϒ production in d+ Au and Au + Au collisions at sNN=200 GeV ” [Phys. Lett. B 735 (2014) 127–137]20150 iqtibos

Hammualliflar

Yana 7 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 8 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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