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S. Vagnozzi, New physics in light of the H 0 H_{0} tension: An alternative view
Original
1907
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, O. Mena, and S. Vagnozzi, Interacting dark energy in the early 2020s: A promising solution to the H 0 H_{0} and cosmic shear tensions
Original
1908
Earlier work this paper cites.
A. Heinesen, C. Blake, and D. L. Wiltshire, Quantifying the accuracy of the Alcock-Paczy&nacute;ski scaling of baryon acoustic oscillation measurements
Original
1908
Earlier work this paper cites.
C. García-García, E. Bellini, P. G. Ferreira, D. Traykova, and M. Zumalacárregui, Theoretical priors in scalar-tensor cosmologies: Thawing quintessence
Original
1911
Earlier work this paper cites.
Z. Zhai, C.-G. Park, Y. Wang, and B. Ratra, CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters
Original
1912
Earlier work this paper cites.
S. Tsujikawa, Quintessence: A Review
Original
1961
Earlier work this paper cites.
C. Williams and C. Rasmussen, Gaussian processes for regression
1995
Earlier work this paper cites.
W. Hu and N. Sugiyama, Small scale cosmological perturbations: An Analytic approach
1996
Earlier work this paper cites.
R. R. Caldwell, R. Dave, and P. J. Steinhardt, Cosmological imprint of an energy component with general equation of state
1998
Earlier work this paper cites.
Supernova Search Team
1998
Earlier work this paper cites.
I. Zlatev, L.-M. Wang, and P. J. Steinhardt, Quintessence, cosmic coincidence, and the cosmological constant
1999
Earlier work this paper cites.
Y. Wang, Flux-averaging analysis of type ia supernova data
2000
Earlier work this paper cites.
M. Chevallier and D. Polarski, Accelerating universes with scaling dark matter
2001
Earlier work this paper cites.
E. V. Linder, Exploring the expansion history of the universe
2003
Earlier work this paper cites.
L. Amendola, C. Quercellini, D. Tocchini-Valentini, and A. Pasqui, Constraints on the interaction and selfinteraction of dark energy from cosmic microwave background
2003
Earlier work this paper cites.
J. L. Bernal, T. L. Smith, K. K. Boddy, and M. Kamionkowski, Robustness of baryon acoustic oscillation constraints for early-Universe modifications of Λ \Lambda CDM cosmology
Original
2004
Earlier work this paper cites.
MIT Press, 2006
C. Rasmussen and C. Williams, Gaussian Processes for Machine Learning · 2006
Earlier work this paper cites.
G. Ellis, R. Maartens, and M. A. H. MacCallum, Causality and the speed of sound
2007
Earlier work this paper cites.
P. Mukherjee and N. Banerjee, Non-parametric reconstruction of the cosmological j e r k jerk parameter
Original
2007
Earlier work this paper cites.
S. Tsujikawa, Modified gravity models of dark energy
Original
2010
Earlier work this paper cites.
T. Clemson, K. Koyama, G.-B. Zhao, R. Maartens, and J. Valiviita, Interacting Dark Energy – constraints and degeneracies
Original
2012
Earlier work this paper cites.
T. Clifton, P. G. Ferreira, A. Padilla, and C. Skordis, Modified Gravity and Cosmology
Original
2012
Earlier work this paper cites.
A. Shafieloo, A. G. Kim, and E. V. Linder, Gaussian Process Cosmography
Original
2012
Earlier work this paper cites.
M. Seikel, C. Clarkson, and M. Smith, Reconstruction of dark energy and expansion dynamics using Gaussian processes
Original
2012
Earlier work this paper cites.
A. Pourtsidou, C. Skordis, and E. J. Copeland, Models of dark matter coupled to dark energy
Original
2013
Earlier work this paper cites.
R. Murgia, S. Gariazzo, and N. Fornengo, Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
Original
2016
Earlier work this paper cites.
K. Koyama, Cosmological Tests of Modified Gravity
Original
2016
Earlier work this paper cites.
B. R. Dinda and A. A. Sen, Imprint of thawing scalar fields on the large scale galaxy overdensity
Original
2018
Earlier work this paper cites.

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2024

Model-agnostic assessment of dark energy after DESI DR1 BAO

Dinda, Bikash R., Maartens, Roy

Understand

Baryon acoustic oscillation measurements by the Dark Energy Spectroscopic Instrument (Data Release 1) have revealed exciting results that show evidence for dynamical dark energy at $\sim3\sigma$ when combined with cosmic microwave background and type Ia supernova observations.

These measurements are based on the $w_0w_a$CDM model of dark energy.
The evidence is less in other dark energy models such as the $w$CDM model.
In order to avoid imposing a dark energy model, we reconstruct the distance measures and the equation of the state of dark energy independent of any dark energy model and driven only by observational data.