Limits on Neutrino Masses from Large-Scale Structure

Simple item page
dc.creatorGawiser, Eric
dc.date2000-05-24
dc.date.accessioned2026-07-07T01:53:44Z
dc.date.available2026-07-07T01:53:44Z
dc.descriptionMassive neutrinos have a detectable effect on cosmological structure formation, in particular on the large-scale distribution of galaxies. Adding Hot Dark Matter to the now-standard Lambda CDM model leads to a worse fit to large-scale structure and CMB anisotropy data. This results in a limit on the mass of the most massive neutrino of 4 eV, assuming a power-law primordial power spectrum.
dc.descriptionProceedings of PASCOS99 Conference, Lake Tahoe, CA 1999. 6 pages, 1 color figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0005475
dc.identifierhttp://arxiv.org/abs/astro-ph/0005475
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1067
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleLimits on Neutrino Masses from Large-Scale Structure
dc.typetext

Files

Collections

arXiv