Current GRB and SNe Ia data with full covariance do not provide evidence for interacting dark energy over Lambda CDM.
25 [67] [68] [69] [70] [71] [75] [76] [77] Guo-Jian Wang, Hai Yu, Zheng-Xiang Li, Jun-Qing Xia, and Zong-Hong Zhu
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Forecasts show that ~66 optical GRBs can achieve σ_w ≈ 0.47 in wCDM using Dainotti relations, matching Planck precision and enabling independent high-redshift tests of dark energy.
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Interacting dark energy constraints from Fermi GRBs and Pantheon+ SNe Ia with full GRB covariance
Current GRB and SNe Ia data with full covariance do not provide evidence for interacting dark energy over Lambda CDM.
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Gamma-Ray Bursts as an Independent High-Redshift Probe of Dark Energy
Forecasts show that ~66 optical GRBs can achieve σ_w ≈ 0.47 in wCDM using Dainotti relations, matching Planck precision and enabling independent high-redshift tests of dark energy.