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We constrain dark energy and modified gravity within the effective field theory of dark energy framework using the full-shape BOSS galaxy power spectrum, combined with Planck cosmic microwave background (CMB) data and recent baryon acoustic oscillations (BAO) measurements from DESI.
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Z. Huang, “A Cosmology Forecast Toolkit – CosmoLib,” JCAP
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G. Gubitosi, F. Piazza, and F. Vernizzi, “The Effective Field Theory of Dark Energy,” JCAP
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E. V. Linder, “Challenges in connecting modified gravity theory and observations,” Phys. Rev. D
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J. Gleyzes, “Parametrizing modified gravity for cosmological surveys,” Phys. Rev. D
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2013
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J. Bloomfield, “A Simplified Approach to General Scalar-Tensor Theories,” JCAP
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J. Gleyzes, D. Langlois, and F. Vernizzi, “A unifying description of dark energy,” Int. J. Mod. Phys
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G. Cusin, M. Lewandowski, and F. Vernizzi, “Nonlinear Effective Theory of Dark Energy,” JCAP
2018
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2018
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M. Denissenya and E. V. Linder, “Gravity’s Islands: Parametrizing Horndeski Stability,” JCAP
2018
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V. Desjacques, D. Jeong, and F. Schmidt, “Large-Scale Galaxy Bias,” Phys. Rept
2018
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