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MODIFIED HOLOGRAPHIC RICCI INTERACTING DARK ENERGY MODELS: DYNAMICAL SYSTEM ANALYSIS AND BAYESIAN COMPARISON

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2024
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EUROPEAN PHYSICAL JOURNAL C
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WE PERFORM A DYNAMICAL SYSTEM ANALYSIS AND A BAYESIAN MODEL SELECTION FOR A NEW SET OF INTERACTING SCE- NARIOS IN THE FRAMEWORK OF MODIFIED HOLOGRAPHIC RICCI DARK ENERGY (MHR-IDE) MODELS. THE DYNAMICAL ANALYSIS SHOWS A MODIFIED RADIATION EPOCH AND A LATE-TIME ATTRACTOR CORRE- SPONDING TO AN ACCELERATED PHASE OF HOLOGRAPHIC DARK ENERGY. IN THE BAYESIAN COMPARISON, WE USE A COMBINATION OF BACK- GROUND DATA INCLUDING TYPE IA SUPERNOVAE, COSMIC CHRONOME- TERS, THE LOCAL VALUE OF THE HUBBLE CONSTANT, BARYON ACOUS- TIC OSCILLATIONS, AND COSMIC MICROWAVE BACKGROUND DATA. WE FIND EVIDENCE AGAINST ALL THE MHR-IDE SCENARIOS STUDIED IN COMPARISON WITH THE ?CDM WHEN THE FULL JOINT ANALYSIS IS CONSIDERED.
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INFRARED CUTOFF, ENTROPY BOUNDS, BLACK-HOLES
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