In type IIB/F-theory models, axion-scalar systems in finite distance limits produce trajectories of infinite length that drive asymptotic cosmic acceleration.
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Different choices of dynamical variables in cosmological systems affect the extractable information from Friedmann equations, illustrated by revisiting standard models and quintessence with exponential potentials using new variables.
Dynamical systems analysis in f(R,L_m,T) gravity identifies stable critical points that describe different evolutionary phases of the Universe.
citing papers explorer
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Axion-Scalar Dynamics: from the Distance Conjecture to Cosmic Acceleration
In type IIB/F-theory models, axion-scalar systems in finite distance limits produce trajectories of infinite length that drive asymptotic cosmic acceleration.
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The choice of variables in cosmological dynamical systems
Different choices of dynamical variables in cosmological systems affect the extractable information from Friedmann equations, illustrated by revisiting standard models and quintessence with exponential potentials using new variables.
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Evolutionary Phase of Universe in $f(R,L_m,T)$ Gravity: The Dynamical System Analysis
Dynamical systems analysis in f(R,L_m,T) gravity identifies stable critical points that describe different evolutionary phases of the Universe.