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Possible early universe signals in proton collisions at the Large Hadron Collider

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arxiv 2201.00202 v1 pith:5IFXCUL5 submitted 2022-01-01 hep-ph hep-exhep-thnucl-exnucl-th

classification hep-phhep-exhep-thnucl-exnucl-th
keywords universecollisionsearlymattersignalscolliderdenseexperimental
verification ladder T0 review T1 audit T2 compute T3 formal

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Our universe was born about 13.8 billion years ago from an extremely hot and dense singular point, in a process known as the Big Bang. The hot and dense matter which dominated the system within a few microseconds of its birth was in the form of a soup of elementary quarks and gluons, known as the quark-gluon plasma (QGP). Signatures compatible with the formation of the QGP matter have experimentally been observed in heavy-ion (such as Au or Pb) collisions at ultra-relativistic energies. Recently, experimental data of proton-proton (pp) collisions at the CERN Large Hadron Collider (LHC) have also shown signals resembling those of the QGP formation, which made these studies quite stimulating as to how the collision of small systems features in producing the early universe signals. In this article, we report on some of the compelling experimental results and give an account of the present understanding. We review the pp physics program at the LHC and discuss future prospects in the context of exploring the nature of the primordial matter in the early universe.

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  1. Systematic analysis of the pp collisions at LHC energies with Tsallis function

    hep-ph 2024-11 conditional novelty 3.0 of 10

    A standard Tsallis fit to published LHC pp spectra yields mass- and energy-dependent effective temperature and non-extensivity parameters, confirming trends reported in earlier papers.

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