Relaxing cosmological constraints on current neutrino masses: Acknowledgment, Appendix & References by@cosmological
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Relaxing cosmological constraints on current neutrino masses: Acknowledgment, Appendix & References
by Cosmological thinking: time, space and universal causation May 24th, 2024
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In this paper, researchers present a mass-varying neutrino model driven by scalar field dark energy, relaxing the upper bound on current neutrino mass.
This paper is available on arxiv under CC 4.0 license.
Authors:
(1) Vitor da Fonseca, Instituto de Astrof´ısica e Ciˆencias do Espa¸co, Faculdade de Ciˆencias da Universidade de Lisboa;
(2) Tiago Barreiro, Instituto de Astrof´ısica e Ciˆencias do Espa¸co, Faculdade de Ciˆencias da Universidade de Lisboa and 2ECEO, Universidade Lus´ofona;
(3) Nelson J. Nunes, Instituto de Astrof´ısica e Ciˆencias do Espa¸co, Faculdade de Ciˆencias da Universidade de Lisboa.
Table of Links
- Abstract and Intro
- Coupling Dark Energy to Neutrinos
- Impact of the Coupling on Perturbations and Observables
- Parameter Estimation
- Discussion
- Acknowledgment, Appendix, and References
ACKNOWLEDGMENTS
The authors would like to thank C. van de Bruck and D. F. Mota for the fruitful discussions. This work is supported by the Funda¸c˜ao para a Ciˆencia e a Tecnologia (FCT) through the research grants UIDB/04434/2020 and UIDP/04434/2020, and the BEYLA project PTDC/FIS-AST/0054/2021. V.d.F. acknowledges FCT support through fellowship 2022.14431.BD.
Appendix A: Parameter constraints for the MaVaN and the uncoupled scalar field models
In the appendix we show the triangular plots of the analysis made with the Plk18+BAO data for the MaVaN model (β free) and the uncoupled case (β = 0), i.e. no interaction between the quintessence component and the neutrino fluid.
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