Tham khảo Số_phận_sau_cùng_của_vũ_trụ

  1. ↑ Wollack, Edward J. (ngày 10 tháng 12 năm 2010). “Cosmology: The Study of the Universe”. Universe 101: Big Bang Theory. NASA. Truy cập ngày 27 tháng 4 năm 2011. 
  2. 1 2 3 Will the Universe expand forever?
  3. ↑ What is the Ultimate Fate of the Universe?
  4. ↑ Lemaître, Georges (1927). “Un univers homogène de masse constante et de rayon croissant rendant compte de la vitesse radiale des nébuleuses extra-galactiques”. Annales de la Société Scientifique de Bruxelles A47: 49–56. Bibcode:1927ASSB...47...49LBản mẫu:Inconsistent citations  translated by A. S. Eddington: Lemaître, Georges (1931). “Expansion of the universe, A homogeneous universe of constant mass and increasing radius accounting for the radial velocity of extra-galactic nebulæ”. Monthly Notices of the Royal Astronomical Society 91: 483–490. Bibcode:1931MNRAS..91..483L. doi:10.1093/mnras/91.5.483Bản mẫu:Inconsistent citations 
  5. ↑ Hoyle Burbidge & Narlikar "A Different Approach to Cosmology" Cambridge University Press.
  6. ↑ “Dark Energy, Dark Matter - Science Mission Directorate”. science.nasa.gov. 
  7. ↑ Ryden, Barbara. Introduction to Cosmology. The Ohio State University. tr. 56. 
  8. ↑ WMAP - Fate of the Universe, WMAP's Universe, NASA. Truy cập 17 tháng 7 năm 2008.
  9. ↑ Lehners, Jean-Luc; Steinhardt, Paul J.; Turok, Neil (2009). “The Return of the PHOENIX Universe”. International Journal of Modern Physics D 18 (14): 2231–2235. Bibcode:2009IJMPD..18.2231L. arXiv:0910.0834. doi:10.1142/S0218271809015977. 
  10. ↑ Glanz, James (1998). “Breakthrough of the year 1998. Astronomy: Cosmic Motion Revealed”. Science 282 (5397): 2156–2157. Bibcode:1998Sci...282.2156G. doi:10.1126/science.282.5397.2156a. 
  11. ↑ Wang, Yun; Kratochvil, Jan Michael; Linde, Andrei; Shmakova, Marina (2004). “Current observational constraints on cosmic doomsday”. Journal of Cosmology and Astro-Particle Physics 2004 (12): 006. Bibcode:2004JCAP...12..006W. arXiv:astro-ph/0409264. doi:10.1088/1475-7516/2004/12/006. 
  12. ↑ Adams, Fred C.; Laughlin, Gregory (1997). “A dying universe: the long-term fate and evolution of astrophysical objects”. Reviews of Modern Physics 69 (2): 337–372. Bibcode:1997RvMP...69..337A. arXiv:astro-ph/9701131. doi:10.1103/RevModPhys.69.337. 
  13. ↑ Tegmark, M (tháng 5 năm 2003). “Parallel Universes”. Scientific American 288 (5): 40–51. Bibcode:2003SciAm.288e..40T. PMID 12701329. arXiv:astro-ph/0302131. doi:10.1038/scientificamerican0503-40. 
  14. ↑ Werlang, T.; Ribeiro, G. A. P.; Rigolin, Gustavo (2013). “Interplay Between Quantum Phase Transitions and the Behavior of Quantum Correlations at Finite Temperatures”. International Journal of Modern Physics B 27: 1345032. Bibcode:2013IJMPB..2745032W. arXiv:1205.1046. doi:10.1142/S021797921345032X. 
  15. ↑ Xing, Xiu-San; Steinhardt, Paul J.; Turok, Neil (2007). "Spontaneous entropy decrease and its statistical formula". arΧiv:0710.4624 [cond-mat.stat-mech]. 
  16. ↑ Linde, Andrei (2007). “Sinks in the landscape, Boltzmann brains and the cosmological constant problem”. Journal of Cosmology and Astroparticle Physics 2007 (1): 022. Bibcode:2007JCAP...01..022L. arXiv:hep-th/0611043. doi:10.1088/1475-7516/2007/01/022.  Đã bỏ qua tham số không rõ |citeseerx= (trợ giúp)
  17. ↑ Yurov, A. V.; Astashenok, A. V.; González-Díaz, P. F. (2008). “Astronomical bounds on a future Big Freeze singularity”. Gravitation and Cosmology 14 (3): 205–212. Bibcode:2008GrCo...14..205Y. arXiv:0705.4108. doi:10.1134/S0202289308030018. 
  18. ↑
  19. ↑ S. W. Hawking & I. G. Moss (1982). “Supercooled phase transitions in the very early universe”. Phys. Lett. B110 (1): 35–8. Bibcode:1982PhLB..110...35H. doi:10.1016/0370-2693(82)90946-7. 
  20. ↑ How Advanced Can a Civilization Become? by FRASER CAIN on APRIL 26, 2004 lưu trữ 1/6/2004

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