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Hide and Seek with Neutralino Dark Matter WIMP

2001/02/27 by Leszek Roszkowski, Roszkowski, Leszek
Physics and Astronomy · #Astrophysics (astro-ph) #Atomic and Subatomic Physics Research #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #astro-ph #hep-ph

paper · pdf · doi:10.48550/arxiv.hep-ph/0102326

Invited talk at the 3rd International Conference on Particle Physics and the Early Universe (COSMO-99), Trieste, Italy, 27 September - 3 October, 1999

arxiv created 2001/02/27 · openalex publication_date 2001/02/27 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

As experimental sensitivity increases, one is approaching the range of WIMP-nucleon interaction strengths characteristic of neutralinos. But this continuing progress also unearths new experimental challenges and uncertainties.

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