Ushbu ishga iqtibos qilgan ishlar

2 ta ish

Ish: Production of deuterons, tritons, <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts></mml:math> nuclei, and their antinuclei in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>p</mml:mi><mml:mi>p</mml:mi></mml:mrow></mml:math> collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>0.9</mml:mn></mml:mrow></mml:math>, 2.76, and 7 TeV

1. Particle species and energy dependencies of freeze-out parameters in high-energy proton–proton collisions

   Muhammad Waqas, Guang Xiong Peng, F. H. Liu +4

   MaqolaHigh-Energy Particle Collisions ResearchThe European Physical Journal Plus20220 iqtibos

   ABIABI:AkademIndex/openalex/2022.article.001147

2. 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

   MaqolaHigh-Energy Particle Collisions ResearchPhysical review. C20240 iqtibos

   ABIABI:AkademIndex/openalex/2024.article.000373