Relaxing cosmological constraints on current neutrino masses: Acknowledgment, Appendix & References

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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