2002/10/09 by Manuel Drees, Drees, Manuel
Physics and Astronomy · #Astrophysics (astro-ph) #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #Particle physics theoretical and experimental studies #astro-ph #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0210142
LaTeX with equation.sty and axodraw.sty (included), 21 p., 5 figures; invited plenary talk at LCWS2002, Jeju Island, Republic of Korea. v.2: Replaced one reference
openalex publication_date 2002/10/09 · arxiv created 2002/10/16 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
In this talk I discuss the interplay between collider physics and four topics of astro-particle physics: neutrino oscillations, electroweak baryogenesis, LSP Dark Matter, and ultra-high energy cosmic rays (UHECR). Some astrophysical scenarios can (only) be tested decisively at colliders. In other cases input from collider experiments is required to sharpen predictions for future astro--particle physics experiments, e.g. for the LSP detection rate or the UHECR spectrum in top--down models.