Cosmology Intertwined II: The Hubble Constant Tension

@article{Valentino2020CosmologyII,
  title={Cosmology Intertwined II: The Hubble Constant Tension},
  author={Eleonora Di Valentino and Luis A. Anchordoqui and Yacine Ali-Haimoud and Luca Amendola and Nikki Arendse and Marika Asgari and Mario Ballardini and Elia Stefano Battistelli and Micol Benetti and Simon Birrer and M arco Bruni and Erminia Calabrese and David Camarena and Salvatore Capozziello and Angela Chen and Jens Chluba and Anton Chudaykin and Eoin 'O Colg'ain and Francis-Yan Cyr-Racine and Paolo Bernardis and Jacques Delabrouille and Jo Dunkley and Agnes Fert'e and Fabio Finelli and Wendy L. Freedman and Noemi Frusciante and Elena Giusarma and Adria G'omez-Valent and Will Handley and Luke Hart and A. F. Heavens and Hendrik Hildebrandt and Daniel E. Holz and Dragan Huterer and Mikhail M. Ivanov and Shahab Joudaki and Marc Kamionkowski and Tanvi Karwal and Lloyd Knox and L. Lamagna and Julien Lesgourgues and Matteo Lucca and Valerio Marra and Silvia Masi and S. Matarrese and Alessandro Melchiorri and Olga Mena and Laura Mersini-Houghton and Vivian Miranda and David F. Mota and J. Muir and Ankan Mukherjee and Florian Niedermann and Alessio Notari and Rafael C. Nunes and Francesco Pace and Antonella Palmese and Supriya Pan and Daniela Paoletti and Valeria Pettorino and Francesco Piacentini and Vivian Poulin and M. Raveri and Adam G. Riess and Vincenzo Salzano and Emmanuel N. Saridakis and Anjan A. Sen and Arman Shafieloo and Anowar J. Shajib and Joseph I. Silk and Alessandra Silvestri and Martin S. Sloth and Tristan L. Smith and Carsten van de Bruck and Licia Verde and Luca Visinelli and Benjamin D. Wandelt and Weiqiang Yang},
  journal={arXiv: Cosmology and Nongalactic Astrophysics},
  year={2020}
}

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References

SHOWING 1-10 OF 267 REFERENCES

H0 tension or T0 tension?

We study if the discrepancy between the local and cosmological measurements of the Hubble constant $H_0$ can be reformulated as a tension in the cosmic microwave background (CMB) monopole temperature

Does the Hubble constant tension call for new physics?

The Λ Cold Dark Matter model (ΛCDM) represents the current standard model in cosmology. Within this, there is a tension between the value of the Hubble constant, H0, inferred from local distance

Alleviating the H0 and σ8 anomalies with a decaying dark matter model

The Hubble tension between the ΛCDM-model-dependent prediction of the current expansion rate H0 using Planck data and direct, model-independent measurements in the local universe from the SH0ES

A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Motivated by the current status of cosmological observations and significant tensions in the estimated values of some key parameters assuming the standard ΛCDM model, we propose a simple but radical

Can the H0 tension be resolved in extensions to ΛCDM cosmology?

We wish to investigate whether there is an extension to the base ΛCDM cosmology that can resolve the tension between the Planck observation of the cosmic microwave background anisotropies and the

Reconciling H0 tension in a six parameter space?

Consistent observations indicate that some of the important cosmological parameters measured through the local observations are in huge tension with their measurements from the global observations

Vacuum phase transition solves the H 0 tension

Taking the Planck cosmic microwave background data and the more direct Hubble constant measurement data as unaffected by systematic offsets, the values of the Hubble constant $H_0$ interpreted within

Addressing the cosmological $$H_0$$ tension by the Heisenberg uncertainty

The uncertainty on measurements, given by the Heisenberg principle, is a quantum concept usually not taken into account in General Relativity. From a cosmological point of view, several authors
...