Gamma-Ray Bursts and Dark Energy - Dark Matter interaction

Abstract

In this work Gamma Ray Burst (GRB) data is used to place constraints on a putative coupling between dark energy and dark matter. Type Ia supernovae (SNe Ia) constraints from the Sloan Digital Sky Survey II (SDSS-II) first-year results, the cosmic microwave background radiation (CMBR) shift parameter from WMAP seven year results and the baryon acoustic oscillation (BAO) peak from the Sloan Digital Sky Survey (SDSS) are also discussed. The prospects for the field are assessed, as more GRB events become available.

7 pages, 3 figures. Version to match the one published in Mon. Not. R. Ast. Soc

References in corpus (7)

• First-year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Hubble Diagram and Cosmological Parameters
• Thick gas discs in faint dwarf galaxies
• Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
• Signature of the interaction between dark energy and dark matter in galaxy clusters
• High energy gamma-ray emission from Gamma-Ray Bursts -- before GLAST
• WMAP5 constraints on the unified model of dark energy and dark matter
• A minimal set of invariants as a systematic approach to higher order gravity models: Physical and Cosmological Constraints

Cited by in corpus (6)

• Irreversible thermodynamic description of interacting dark energy - dark matter cosmological models
• Dark Matter-Dark Energy Interaction and the Shape of Cosmic Voids
• Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models
• Testing the interaction of dark energy to dark matter through the analysis of virial relaxation of clusters Abell Clusters A586 and A1689 using realistic density profiles
• Coupled Quintessence scalar field model in light of observational datasets
• Interacting dark energy collapse with matter components separation