Tackling non-linearities with the effective field theory of dark energy and modified gravity (Q5021829): Difference between revisions

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+<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
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+Evolution of second-order cosmological perturbations
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+Existence of Long-Range Magnetic Order in the Ground State of Two-Dimensional Spin-1/2 Heisenberg Antiferromagnets
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+Comparing two different formulations of metric cosmological perturbation theory
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+Gradient Expansion Approach to Nonlinear Superhorizon Perturbations
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+Nonlinear superhorizon curvature perturbation in generic single-field inflation
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+Large-scale structure of the universe and cosmological perturbation theory
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+Effective field theory of cosmological perturbations
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+A unifying description of dark energy
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+Effective field theory approach to modified gravity including Horndeski theory and Hořava–Lifshitz gravity
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+Starting the universe: stable violation of the null energy condition and non-standard cosmologies
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+\(3+1\) formalism in general relativity. Bases of numerical relativity.
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+Effective description of higher-order scalar-tensor theories
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+Higher derivative field theories: degeneracy conditions and classes
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+Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order
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+On the stability conditions for theories of modified gravity in the presence of matter fields
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+\(\text{xPand}\): an algorithm for perturbing homogeneous cosmologies
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