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Dark Energy Versus Modified Gravity
Open accessAbstract
Understanding the reason for the observed accelerated expansion of the Universe represents one of the fundamental open questions in physics. In cosmology, a classification has emerged among physical models for this acceleration, distinguishing between dark energy and modified gravity. In this review, we provide a brief overview of models in both categories as well as their phenomenology and characteristic observable signatures in cosmology. We also introduce a rigorous distinction between dark energy and modified gravity based on the strong and weak equivalence principles.
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“They state that using the SEP to make this distinction can be motivated further by the conjecture that GR is the only metric theory that satisfy the SEP, see Will (2014).”
From Testing general relativity in cosmology (2019) · cites this paper as Joyce et al. (2016)
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“Joyce et al. (2016) and possibly others, propose to use the strong equivalence principle (SEP) (see Sect. 2.1) to draw a distinction between GR dark energy models versus MG models. They suggest to call any model that satisfies the SEP as a dark energy model and any model that violates SEP to be an MG model.”
From Testing general relativity in cosmology (2019) · cites this paper as Joyce et al. (2016)
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“They state that, heuristically, the SEP forbids the presence of a fifth force which motivates the use of such a discriminant.”
From Testing general relativity in cosmology (2019) · cites this paper as Joyce et al. (2016)
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Cites
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, A. G., Filippenko, A. V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P. M., Gilliland, R. L., Hogan, C. J., Jha, S., Kirshner, R. P., et al. (1998) · The Astronomical Journal · doi:10.1086/300499 · Cited by 19,704
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
Observation of Gravitational Waves from a Binary Black Hole Merger
Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., et al. (2016) · Physical Review Letters · doi:10.1103/physrevlett.116.061102 · Cited by 14,251
A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917
The cosmological constant problem
Weinberg, S. (1989) · Reviews of Modern Physics · doi:10.1103/revmodphys.61.1 · Cited by 7,341
A Universal Density Profile from Hierarchical ClusteringPreprint
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · Cited by 6,275
Mach's Principle and a Relativistic Theory of Gravitation
Brans, C., & Dicke, R. H. (1961) · Physical Review · doi:10.1103/physrev.124.925 · Cited by 5,621
Modified gravity and cosmology
Clifton, T., Ferreira, P. G., Padilla, A., & Skordis, C. (2012) · Physics Reports · doi:10.1016/j.physrep.2012.01.001 · Cited by 4,630
Felice, A. D., & Tsujikawa, S. (2010) · Living Reviews in Relativity · doi:10.12942/lrr-2010-3 · Cited by 4,327
Cosmological consequences of a rolling homogeneous scalar field
Ratra, B., & Peebles, P. J. E. (1988) · Physical Review D · doi:10.1103/physrevd.37.3406 · Cited by 4,310
Research works printed but not linked: 6
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Items 301–400 of 458
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Cosmic growth signatures of modified gravitational strength
Denissenya, M., & Linder, E. V. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/06/030 · Cited by 6
“, [16] for a review, and references therein).”
BackgroundNavigating Permanent Underdetermination in Dark Energy and Inflationary Cosmology
Wolf, W. J., & Read, J. A. M. (2026) · Philosophy of Physics · doi:10.31389/pop.269 · Cited by 5
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Pizzuti, L., Fantoccoli, F., Broccolato, V., Biviano, A., & Diaferio, A. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202452739 · Cited by 5
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Ghedini, P., Hajjar, R., & Mena, O. (2026) · Physics of the Dark Universe · doi:10.1016/j.dark.2026.102237 · Cited by 5
Dynamical Analysis in Chameleon Dark Energy
Paliathanasis, A. (2023) · Fortschritte der Physik · doi:10.1002/prop.202300088 · Cited by 5
Stealth black holes in Aether Scalar Tensor theory
Skordis, C., & Vokrouhlický, D. M. J. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/03/035 · Cited by 7
“Another possibility which has been in vogue in the last twenty years or so, is to extend GR with new gravitational degrees of freedom playing the role of dark energy, in an attempt to alleviate some of the issues associated with the cosmological constant [6, 10, 11].”
Generalized frameworks: Structuring searches for new physics
Koberinski, A. (2023) · European Journal for Philosophy of Science · doi:10.1007/s13194-022-00504-7 · Cited by 5
“where H is the Hubble parameter, a the scale factor, and m the fraction of energy density in the universe due to matter (Joyce et al., 2016).”
BackgroundInfluentialArmijo, J., Baugh, C. M., Norberg, P., & Padilla, N. D. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae449 · Cited by 5
García-Farieta, J. E., Balaguera-Antolínez, A., & Kitaura, F.-S. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202450755 · Cited by 5
Non-linear density–velocity dynamics in f(R) gravity from spherical collapse
Nadkarni-Ghosh, S., & Chowdhury, S. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac133 · Cited by 5
Constraining Brans–Dicke Cosmology with the CSST Galaxy Clustering Spectroscopic Survey
Chen, A., Gong, Y., Wu, F., Wang, Y., & Chen, X. (2022) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/ac6418 · Cited by 5
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Schmidt, F. (2017) · Physics · doi:10.1103/physics.10.134 · Cited by 5
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BackgroundSelf-citationCosmological Reconstructions with Artificial Neural NetworksPreprint
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“In order to make sense of the plethora of currently available cosmological models and observations [9, 10], it is necessary to develop valuable statistical tools.”
BackgroundMimetic-f(Q) gravity: Cosmic reconstruction and energy conditions
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Goswami, K. B., Bhattacharjee, D., Chattopadhyay, P. K., & Saha, A. (2024) · Physics of the Dark Universe · doi:10.1016/j.dark.2024.101752 · Cited by 4
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Vedder, C., Belgacem, E., Chisari, N. E., & Prokopec, T. (2023) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2023/03/016 · Cited by 4
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Xiao, L., & Zheng, Y. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad2282 · Cited by 4
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Sunny, A., Xavier, S., & Shankaranarayanan, S. (2024) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ad4c4b · Cited by 4
Kofinas, G., & Lima, N. A. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.084016 · Cited by 4
Chakrabarti, S., & Chattopadhyay, S. (2018) · Zeitschrift für Naturforschung A · doi:10.1515/zna-2017-0444 · Cited by 4
Progress in Fine Particle Plasmas
Mieno, T., Hayashi, Y., & Xue, K. (2019) · IntechOpen eBooks · doi:10.5772/intechopen.83211 · Cited by 4
Blinnikov, S. I., & Dolgov, A. D. (2018) · Physics-Uspekhi · doi:10.3367/ufnr.2018.10.038469 · Cited by 26
“[316] Joyce, A.”
Damping of cosmological tensor modes in Horndeski theories after GW170817Preprint
Scomparin, M., & Vazzoler, S. (2019) · arXiv (Cornell University) · doi:10.48550/arxiv.1903.01502 · Cited by 4
Revisiting cosmological diffusion models in Unimodular Gravity and the $H_0$ tensionPreprint
Cedeño, F. X. L., & Nucamendi, U. (2020) · arXiv (Cornell University) · doi:10.48550/arxiv.2009.10268 · Cited by 4
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Garcion, C., Gill, S. S., Misslisch, M., Heidt, A., Papadakis, I., Piest, B., Schkolnik, V., Wendrich, T., Prat, A., Bleeke, K., et al. (2025) · EPJ Quantum Technology · doi:10.1140/epjqt/s40507-025-00371-0 · Cited by 3
“It has been proposed, in the frame of theories of modified gravity [5], to explain the cosmological constant by the existence of a scalar field that couples to all particles.”
Effective field theories for neutron stars physics
Alarcón, J. M., Lope-Oter, E., & Cano, Y. (2025) · The European Physical Journal Special Topics · doi:10.1140/epjs/s11734-025-02026-8 · Cited by 3
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Zaregonbadi, R., Saba, N., & Farhoudi, M. (2023) · The European Physical Journal C · doi:10.1140/epjc/s10052-023-12138-x · Cited by 3
Stability aspects of an LRS Bianchi type-I cosmological model in f(Q) gravity
Rathore, S., & Singh, S. S. (2024) · General Relativity and Gravitation · doi:10.1007/s10714-024-03215-x · Cited by 3
Toniato, J. D., & Richarte, M. G. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.109.104068 · Cited by 3
Dark energy and dark matter as a kinematic-electromagnetic Abelian gauge effect
Garat, A. (2024) · International Journal of Geometric Methods in Modern Physics · doi:10.1142/s0219887824501731 · Cited by 3
The accelerated expansion in F(G,TμνTμν) gravity
Marciu, M., & Ioan, D. M. (2024) · Modern Physics Letters A · doi:10.1142/s0217732324500275 · Cited by 3
“This phenomenon has been discovered almost two decades ago [2, 3], triggering various developments in science and technology.”
Background$$f\left( R,\square R\right) $$-gravity and equivalency with the modified GUP Scalar field models
Paliathanasis, A. (2024) · The European Physical Journal C · doi:10.1140/epjc/s10052-024-12797-4 · Cited by 3
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Montano, F., & Camera, S. (2024) · Physics of the Dark Universe · doi:10.1016/j.dark.2024.101570 · Cited by 3
“In this context, a measurement of an effect due to GR coming from cosmology would represent another amazing success of Einsteinian gravity, whereas departures from GR would be a window into the intriguing ‘modified gravity’ scenario (Clifton et al. , 2012; Joyce et al. , 2016).”
BackgroundRobertson, A., Huff, E., Markovic, K., & Li, B. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae1980 · Cited by 3
Experimental evaluation of complete safe coordination of astrobots for Sloan Digital Sky Survey V
Macktoobian, M., Araújo, R., Grossen, L., Kronig, L., Bouri, M., Gillet, D., & Kneib, J. (2020) · Experimental Astronomy · doi:10.1007/s10686-020-09687-4 · Cited by 3
Constraining gravity with hadron physics: neutron stars, modified gravity and gravitational waves
Llanes–Estrada, F. J. (2017) · Springer Link (Chiba Institute of Technology) · doi:10.1051/epjconf/201713701013/pdf · Cited by 3
Cosmic acceleration and stars in an asymptotically Ricci flat universe
Jaime, L. G., & Salgado, M. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.084045 · Cited by 3
Ali, A. (2026) · Zenodo (CERN European Organization for Nuclear Research) · doi:10.5281/zenodo.20633582 · Cited by 3
Unified description of dark energy and dark matter candidates with the dark energy interiors
Dymnikova, I. (2024) · Physics of the Dark Universe · doi:10.1016/j.dark.2024.101738 · Cited by 2
Probing Time-dependent Dark Energy with the Flux Power Spectrum of the Lyα Forest
Coughlin, J. W., Mathews, G. J., Phillips, L. A., Snedden, A., & Suh, I. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab04f9 · Cited by 2
“See, however, Joyce et al. (2016) for an excellent discussion of dark energy as compared with modified gravity.”
BackgroundFast approximate methods for modified gravity cosmological simulations
Vrastil, M., & Habib, S. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa333 · Cited by 2
Impact of PSF misestimation and galaxy population bias on precision shear measurement using a CNN
Voigt, L. M. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae038 · Cited by 2
Galactic dynamics in the presence of scalaron: a perspective from f(R) gravity
Mohan, G., & Goswami, U. D. (2024) · Physica Scripta · doi:10.1088/1402-4896/ad6d0d · Cited by 2
Koskas, R., & Alimi, J. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202451898 · Cited by 2
Generation of effective massive Spin-2 fields through spontaneous symmetry breaking of scalar field
Mandal, S., & Shankaranarayanan, S. (2025) · General Relativity and Gravitation · doi:10.1007/s10714-025-03367-4 · Cited by 2
Bounce cosmologies in generalized coupling theories
Troisi, A., & Carloni, S. (2025) · Physics Letters B · doi:10.1016/j.physletb.2025.139426 · Cited by 2
“One often considered solution for these questions involves modifications of General Relativity (see [3, 4, 5, 6] and references therein).”
Burrage, C. (2022) · SciPost Physics Lecture Notes · doi:10.21468/scipostphyslectnotes.41 · Cited by 2
“3There are modifications of gravity that cannot be mapped to novel matter and vice versa, but there are also many theories which could be put into either category depending on how the theory is formulated [13].”
BackgroundModified gravity and large scale flows, a review
Mould, J. R. (2017) · Astrophysics and Space Science · doi:10.1007/s10509-017-3005-3 · Cited by 2
“In the context of General Relativity there is almost unlimited scope for modified gravity theories (Joyce et al 2016).”
BackgroundVarying alpha generalized Dirac-Born-Infeld models
Tavares, V. C., & Martins, C. J. A. P. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.103.023525 · Cited by 2
Cosmological Constant from Boundary Condition and Its Implications beyond the Standard Model
Stenflo, J. O. (2023) · Universe · doi:10.3390/universe9020103 · Cited by 2
Analytical models of hyperbolical gravitational sources
Yousaf, Z., Bhatti, M. Z. U. H., & Asad, H. (2023) · International Journal of Modern Physics D · doi:10.1142/s021827182350089x · Cited by 2
Developments of the Relativistic Bohm-Poisson Equation and Dark Energy
Perelman, C. C. (2018) · Theoretical Physics · doi:10.22606/tp.2019.41003 · Cited by 2
“The real scalar field φ = φ(t) is assumed to behave as a perfect fluid whose density and pressure are [4]”
BackgroundInfluentialOks, E. (2021) · Open Journal of Microphysics · doi:10.4236/ojm.2021.111001 · Cited by 2
Amended FRW Metric and Rényi Dark Energy Model
Ali, S., Iqbal, S., Khan, K. A., & Moradi, H. R. (2021) · Advances in High Energy Physics · doi:10.1155/2021/9704909 · Cited by 2
“This is called dark energy (DE) [4, 5], and it is considered one of the existing theoretical possibilities, including modifications of gravity theories [6].”
Background4G: Pure fourth-order gravityPreprint
Tian, S. (2018) · arXiv (Cornell University) · doi:10.48550/arxiv.1807.06432 · Cited by 2
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Mancarella, M., Kennedy, J., Bose, B., & Lombriser, L. (2020) · arXiv (Cornell University) · Cited by 2
Self-citationDark energy with oscillatory tracking potential: observational constraints and perturbative effects
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Dodelson, S., & Schmidt, F. (2020) · Elsevier eBooks · doi:10.1016/b978-0-12-815948-4.00008-5 · Cited by 1
Self-citationMeasuring Cosmological Parameters with Gravitational Waves
Mastrogiovanni, S., & Steer, D. A. (2021) · Springer eBooks · doi:10.1007/978-981-15-4702-7_48-1 · Cited by 1
Accelerated expansion is a built-in property of the Boltzmann universe
Michel, D. (2025) · Physica A Statistical Mechanics and its Applications · doi:10.1016/j.physa.2025.130448 · Cited by 1
Ying, X., & Jia, J. (2024) · Chinese Physics C · doi:10.1088/1674-1137/ada34a · Cited by 1
Cluster optical depth and pairwise velocity estimation using machine learning
Gong, Y., & Bean, R. (2025) · Physical review. D/Physical review. D. · doi:10.1103/d6tz-tdb8 · Cited by 1
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Yousaf, Z., Bhatti, M. Z. U. H., Shrahili, M., Manan, A., & Malik, A. (2025) · Modern Physics Letters A · doi:10.1142/s0217732325501573 · Cited by 1
From matter density to deflection angle and gravitational lensing using a perturbative method
Liu, P., Zhang, X., & Jia, J. (2025) · Physics of the Dark Universe · doi:10.1016/j.dark.2025.102095 · Cited by 1
Shaikh, A. Y., & Jenekar, A. P. (2025) · New Astronomy · doi:10.1016/j.newast.2025.102497 · Cited by 1
Vogt, S. M. L., Bocquet, S., Davies, C. T., Mohr, J. J., Schmidt, F., Ruan, C.-Z., Li, B., Hernández‐Aguayo, C., Grandis, S., Bleem, L. E., et al. (2026) · Physical review. D/Physical review. D. · doi:10.1103/t189-srtj · Cited by 1
Self-citationPatki, R., Battaglia, N., & Bean, R. (2025) · Physical review. D/Physical review. D. · doi:10.1103/5d6p-4bys · Cited by 1
Li, S., & Zheng, Y. (2026) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ae31f7 · Cited by 1
“Breaking this degeneracy requires simultaneously measuring the cosmic expansion and structure growth histories (Weinberg et al. 2013; Joyce et al. 2016; Koyama 2016).”
Luminosity-temperature relation as a probe for modified gravity
Popolo, A. D., Fakhry, S., & Mota, D. F. (2026) · Physical review. D/Physical review. D. · doi:10.1103/fq33-yts8 · Cited by 1
Goh, L. W. K., Nouri-Zonoz, A., Pamuk, S., Ballardini, M., Bose, B., Cañas-Herrera, G., Casas, S., Abellán, G. F., Ilić, S., Keil, F., et al. (2026) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202556859 · Cited by 1
Scalar-field reconstruction of Ricci–Gauss–Bonnet dark energy in Hořava–Lifshitz cosmology
Chattopadhyay, S. (2026) · Physics Letters A · doi:10.1016/j.physleta.2026.131799 · Cited by 1
Trouble with Hubble? A brief philosophical assessment of the $$H_0$$ tension
Wolf, W. J. (2026) · European Journal for Philosophy of Science · doi:10.1007/s13194-026-00761-w · Cited by 1
DE-DM Unification Based on Space-Time Symmetry
Dymnikova, I. (2018) · Gravitation and Cosmology · doi:10.1134/s020228931802007x · Cited by 1
An Accelerating Universe with No Dark Energy
Friedmann, D. E. (2018) · OALib · doi:10.4236/oalib.1104740 · Cited by 1
Speeding up N-Body Simulations of Modified Gravity: Chameleon Screening Models
Bose, S. (2018) · Springer theses · doi:10.1007/978-3-319-96761-5_6 · Cited by 1
Deflection in higher dimensional spacetime and asymptotically non-flat spacetimes
He, J., Wang, Q., Hu, Q., Li, F., & Jia, J. (2023) · Classical and Quantum Gravity · doi:10.1088/1361-6382/acbade · Cited by 1
Late Accelerated Expansion of the Universe in Diffusive Scenarios
Piratova-Moreno, E. F., & García, L. Á. (2023) · Revista Mexicana de Astronomía y Astrofísica · doi:10.22201/ia.01851101p.2023.59.02.15 · Cited by 1
Spatial dependence of the growth factor in scalar-tensor cosmology
Caruana, M., Farrugia, G., Said, J., & Sultana, J. (2024) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2024/06/053 · Cited by 1
“Scalar-tensor theories [23–25] have featured in all these possible avenues for confronting the cosmic tensions problem.”
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Raveri, M. (2024) · Springer Series in Astrophysics and Cosmology · doi:10.1007/978-981-99-0177-7_27 · Cited by 1
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Mandal, S., & Shankaranarayanan, S. (2025) · The European Physical Journal Plus · doi:10.1140/epjp/s13360-025-06037-1 · Cited by 3
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Ildes, M., Arık, M., & Sheftel, M. B. (2018) · International Journal of Modern Physics D · doi:10.1142/s0218271819500664 · Cited by 2
Thermodynamic instability of dark energy equation of state
Roupas, Z. (2023) · Physics of the Dark Universe · doi:10.1016/j.dark.2023.101181 · Cited by 1
Inflation: a quantum laboratory on cosmological scalesPreprint
Pattison, C. A. (2021) · arXiv (Cornell University) · doi:10.48550/arxiv.2102.01030 · Cited by 1
Exploring the self-tuning of the cosmological constant from Planck mass variationPreprint
Blanco, D. S., & Lombriser, L. (2020) · arXiv (Cornell University) · doi:10.48550/arxiv.2012.01838 · Cited by 1
“But it also motivates the conjecture of a yet undetermined mechanism [5–13] preventing vacuum energy from gravitating to full extent with cosmic acceleration attributed to a different origin such as a dark energy field permeating the Cosmos or a breakdown of General Relativity at large scales [14–16].”
BackgroundSelf-citationNeural Network Reconstructions for the Hubble Parameter, Growth Rate and Distance ModulusPreprint
Gómez-Vargas, I., Esquivel, R. M., García‐Salcedo, R., & Vazquez, J. A. (2021) · SSRN Electronic Journal · doi:10.2139/ssrn.3990646 · Cited by 1
Farooq, O. (2026) · SSRN Electronic Journal · doi:10.2139/ssrn.6864448 · Cited by 1
Carrilho, P., Carrion, K., Bose, B., Pourtsidou, A., Hidalgo, J. C., Lombriser, L., & Baldi, M. (2021) · arXiv (Cornell University) · doi:10.1093/mnras/stac641 · Cited by 27
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Wenzl, L., Doux, C., Heinrich, C., Bean, R., Jain, B., Dor\'e, O., Eifler, T., & Fang, X. (2021) · arXiv (Cornell University) · doi:10.1093/mnras/stac790 · Cited by 21
Cosmology in the mimetic higher-curvature $$f(R,R_{\mu \nu }R^{\mu \nu })$$ gravity
Kaczmarek, A. Z., & Szczęśniak, D. (2021) · Scientific Reports · doi:10.1038/s41598-021-97907-y
Singularities and Soft-Big Bang in a viscous $\Lambda$CDM modelPreprint
Cruz, N., González, E., & Jovel, J. (2021) · arXiv (Cornell University) · doi:10.1103/physrevd.105.024047
“[12] Fabian Schmidt Austin Joyce, Lucas Lombriser.”
Probing beyond-Horndeski gravity on ultra-large scales
Moloi, T. A., Duniya, D. G. A., & Clarkson, C. (2020) · UWC Research Repository (University of the Western Cape) · doi:10.1088/1475-7516/2020/01/033 · Cited by 9
A Shift of Nucleon Mass Could Substitute the Idea of an Accelerated Expansion
Köhler, J. M. (2017) · International Journal of High Energy Physics · doi:10.11648/j.ijhep.20170402.11
The Joint Institute for Nuclear Research in Experimental Physics of Elementary Particles
Bednyakov, V. A., & Rusakovich, N. A. (2018) · Physics of Particles and Nuclei · doi:10.1134/s1063779618030024
Metadata
- Authors
- Joyce, A., Lombriser, L., & Schmidt, F.
- Affiliations
- University of Chicago (US)
- Royal Observatory (GB)
- Max Planck Institute for Astrophysics (DE)
- Corresponding author
- Schmidt, Fabian
- Venue
- Annual Review of Nuclear and Particle Science
- Publisher
- Annual Reviews
- Published
- 2016-10-19
- Volume
- 66
- Issue
- 1
- Pages
- 95-122
- ISSN
- 0163-8998 (ISSN-L)
- 1545-4134
- OpenAlex
- W2253235198
- Cited by
- 463
- References
- 158
- Citations by year
- 2026: 30 · 2025: 56 · 2024: 57 · 2023: 46 · 2022: 37 · 2021: 42 · 2020: 52 · 2019: 46 · 2018: 43 · 2017: 46 · 2016: 8
- FWCI
- 3.45
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Annual Review of Nuclear and Particle Science (publishedVersion)
- arXiv (Cornell University) (publishedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Keywords
- dark energy, modified gravity, cosmic acceleration, equivalence principle, strong equivalence principle, weak equivalence principle, cosmological models, observational signatures
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