参考文献1. Caldwell， R. R.， Kamionkowski， M.， & Weinberg， N. N. (2003). Phantom Energy： Dark Energy with w < −1 Causes a Cosmic Doomsday. Physical Review Letters， 91(7)， 071301.2. Caldwell， R. R. (2002). A phantom menace? Cosmological consequences of a dark energy component with super-negative equation of state. Physics Letters B， 545(1–2)， 23–29.3. Carroll， S. M.， Hoffman， M.， & Trodden， M. (2003). Can the dark energy equation-of-state parameter w be less than −1? Physical Review D， 68(2)， 023509.4. Frampton， P. H.， Ludwick， K. J.， & Scherrer， R. J. (2011). The little rip. Physical Review D， 84(6)， 063003.5. Frieman， J.， Turner， M.， & Huterer， D. (2008). Dark energy and the accelerating universe. Annual Review of Astronomy and Astrophysics， 46， 385–432.6. Barrow， J. D.， & Tipler， F. J. (1986). The Anthropic Cosmological Principle. Oxford University Press.7. Perlmutter， S.， et al. (1999). Measurements of Ω and Λ from 42 High-Redshift Supernovae. The Astrophysical Journal， 517(2)， 565–586.8. 世界科学. “WMAP将要告诉我们什么？——谈人类对宇宙演化的探索.” 检索于2026.9. Nojiri， S.， & Odintsov， S. D. (2006). The dark energy evolution from the early universe to future phantom doomsday and the Big Rip. Physics Letters B， 637(3)， 139–148.10. Weinberg， S. (1989). The cosmological constant problem. Reviews of Modern Physics， 61(1)， 1–23.

Ask this episode

“What did the council decide on item 42?” — answered with the speaker and the moment.

Transcript

Related