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A. Gibson

3 та иш

Valparaiso University

  1. Production of protons and light nuclei in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>Au</mml:mi><mml:mo>+</mml:mo><mml:mi>Au</mml:mi></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:mspace width="0.16em"/><mml:mo>=</mml:mo><mml:mspace width="0.16em"/><mml:mn>3</mml:mn></mml:mrow></mml:math> GeV with the STAR detector

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

    МақолаHigh-Energy Particle Collisions ResearchPhysical review. C20240 иқтибос
    ABI

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

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

    МақолаHigh-Energy Particle Collisions ResearchJournal of High Energy Physics20240 иқтибос
    ABI

  3. 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

    МақолаHigh-Energy Particle Collisions ResearchPhysical review. C20250 иқтибос
    ABI