【第二季】144｜【终结之问】能在孤岛化前搞清楚暗能量吗？

参考文献1. DESI Collaboration (2024). DESI 2024 VI： Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations. arXiv preprint， arXiv：2404.03002.2. DESI Collaboration (2025). DESI 2025： Three-year Baryon Acoustic Oscillation measurements and cosmological constraints. Lawrence Berkeley National Laboratory News Release， March 2025.3. Euclid Collaboration (2024). Euclid. I. Overview of the Euclid mission. Astronomy & Astrophysics， 662， A112.4. Spergel， D.， et al. (2015). Wide-Field InfraRed Survey Telescope-Astrophysics Focused Telescope Assets (WFIRST-AFTA) Final Report. arXiv preprint， arXiv：1305.5422.5. Weinberg， D. H.， et al. (2013). Observational probes of cosmic acceleration. Physics Reports， 530(2)， 87–255.6. Eisenstein， D. J.， et al. (2005). Detection of Baryon Acoustic Oscillations in the Correlation Function of a Sample of 46，748 Luminous Red Galaxies. The Astrophysical Journal， 633(2)， 560–574.7. Peebles， P. J. E.， & Ratra， B. (2003). The cosmological constant and dark energy. Reviews of Modern Physics， 75(2)， 559–606.8. Caldwell， R. R.， Dave， R.， & Steinhardt， P. J. (1998). Cosmological Imprint of an Energy Component with General Equation of State. Physical Review Letters， 80(8)， 1582.9. Berkeley Lab News Center. “New DESI Results Strengthen Hints That Dark Energy May Evolve.” March 19， 2025.10. Chevallier， M.， & Polarski， D. (2001). Accelerating universes with scaling dark matter. International Journal of Modern Physics D， 10(2)， 213–223.