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

Fecha
2024
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EUROPEAN PHYSICAL JOURNAL C
Resumen
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