首页 | 本学科首页   官方微博 | 高级检索  
     检索      


Coupling between cold dark matter and dark energy from neutrino mass experiments
Authors:JR Kristiansen  G La Vacca  LPL Colombo  R Mainini  SA Bonometto
Institution:1. Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029, 0315 Oslo, Norway;2. Physics Dept. G. Occhialini, Milano–Bicocca University, Piazza della Scienza 3, 20126 Milano, Italy;3. I.N.F.N., Sez. Milano–Bicocca, Piazza della Scienza 3, 20126 Milano, Italy;4. Physics Dept., University of Southern California, Los Angeles, CA 90089-0484, USA;5. I.N.A.F., Roma Observatory, Via Frascati 33, 00040 Monteporzio Catone, Italy
Abstract:We consider cosmological models with dynamical dark energy (dDE) coupled to cold dark matter (CDM), while simultaneously allowing neutrinos to be massive. Using a MCMC approach, we compare these models with a wide range of cosmological data sets. We find a strong correlation between this coupling strength and the neutrino mass. This correlation persists when BAO data are included in the analysis. We add then priors on ν mass from particle experiments. The claimed detection of ν mass from the Heidelberg–Moscow neutrinoless double-β decay experiment would imply a 7–8σ detection of CDM–DE coupling. Similarly, the detection of ν mass from coming KATRIN tritium β decay experiment will imply a safe detection of a coupling in the dark sector. Previous attempts to accommodate cosmic phenomenology with such possible ν mass data made recourse to a w<-1 eoS. We compare such an option with the coupling option and find that the latter allows a drastic improvement.
Keywords:
本文献已被 ScienceDirect 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号