1993/08/19 by Jishnu Dey, Lauro Tomio, Mira Dey
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Quantum Electrodynamics and Casimir Effect #hep-ph
paper · pdf · doi:10.1016/0370-2693(93)90144-7
published as Phys.Lett. B318 (1993) 387-390; Addendum-ibid. B320 (1994) 431 · 8 pages, 2 figures, figures on request to [email protected], IFT preprint-IFT P-050/93, Latex
arxiv created 1993/08/19 · openalex publication_date 1993/12/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Recent Deep Inelastic data leads to an up-down quark asymmetry of the nucleon sea. Explanations of the flavour asymmetry and the di-lepton production in proton-nucleus collisions call for a temperature T ≈ 100 MeV in a statistical model. This T may be conjectured as being due to the Fulling-Davies-Unruh effect. But it is not possible to fit the structure function itself.