Probing Dark Energy via Neutrino & Supernova Observatories

Simple item page
dc.creatorHall, Lawrence J.
dc.creatorMurayama, Hitoshi
dc.creatorPapucci, Michele
dc.creatorPerez, Gilad
dc.date2006-07-10
dc.date.accessioned2026-07-07T07:16:43Z
dc.date.available2026-07-07T07:16:43Z
dc.descriptionA novel method for extracting cosmological evolution parameters is proposed, using a probe other than light: future observations of the diffuse anti-neutrino flux emitted from core-collapse supernovae (SNe), combined with the SN rate extracted from future SN surveys. The relic SN neutrino differential flux can be extracted by using future neutrino detectors such as Gadolinium-enriched, megaton, water detectors or 100-kiloton detectors of liquid Argon or liquid scintillator. The core-collapse SN rate can be reconstructed from direct observation of SN explosions using future precision observatories. Our method, by itself, cannot compete with the accuracy of the optical-based measurements but may serve as an important consistency check as well as a source of complementary information. The proposal does not require construction of a dedicated experiment, but rather relies on future experiments proposed for other purposes.
dc.description30 pages, 7 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0607109
dc.identifierhttp://arxiv.org/abs/hep-ph/0607109
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/113688
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.titleProbing Dark Energy via Neutrino & Supernova Observatories
dc.typetext

Files

Collections

arXiv