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AkademIndex

Xizmatlar

Yongbin Feng

6 ta ish

Sun Yat-sen University

AkademScholarda batafsil koʻrsatkichlar

  1. Energy dependence of intermittency for charged hadrons in Au+Au collisions at RHIC

    M. I. Abdulhamid, B. E. Aboona, J. Adam +97

    Maqola20232 iqtibos
    ABI

  2. Evidence of Mass Ordering of Charm and Bottom Quark Energy Loss in Au+Au Collisions at RHIC

    M. S. Abdallah, B. E. Aboona, J. Adam +95

    MaqolaOchiq kirishHigh-Energy Particle Collisions ResearchThe European Physical Journal C20220 iqtibos
    ABI

  3. Strangeness production in $$ \sqrt{s_{\textrm{NN}}} $$ = 3 GeV Au+Au collisions at RHIC

    M. I. Abdulhamid, B. E. Aboona, J. Adam +95

    MaqolaOchiq kirishHigh-Energy Particle Collisions ResearchJournal of High Energy Physics20240 iqtibos
    ABI

  4. Correlations of event activity with hard and soft processes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>p</mml:mi><mml:mo>+</mml:mo><mml:mtext>Au</mml:mtext></mml:mrow></mml:math> collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><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>=</mml:mo><mml:mn>200</mml:mn></mml:mrow></mml:math> GeV at the RHIC STAR experiment

    M. I. Abdulhamid, B. E. Aboona, J. Adam +96

    MaqolaOchiq kirishHigh-Energy Particle Collisions ResearchPhysical review. C20240 iqtibos
    ABI

  5. Breaking the Efficiency‐Stability‐Sustainability Trilemma in all‐perovskite Tandem Solar Modules via Oxidative Blockchain Molecular Engineering

    Guo Yang, Jinglin Sun, Xueqing Chang +20

    MaqolaPerovskite Materials and ApplicationsAdvanced Materials20250 iqtibos
    ABI

  6. Measurement of directed flow in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>Au</mml:mi><mml:mo>+</mml:mo><mml:mi>Au</mml:mi></mml:mrow></mml:math> collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><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>=</mml:mo><mml:mn>19.6</mml:mn></mml:mrow></mml:math> and 27 GeV with the STAR event plane detector

    M. I. Abdulhamid, B. E. Aboona, J. Adam +94

    MaqolaOchiq kirishHigh-Energy Particle Collisions ResearchPhysical review. C20250 iqtibos
    ABI