Tham khảo Giới_hạn_Bekenstein

  1. 1 2 Bekenstein, Jacob D. (1981). “Universal upper bound on the entropy-to-energy ratio for bounded systems” (PDF). Physical Review D. 23 (2): 287–298. Bibcode:1981PhRvD..23..287B. doi:10.1103/PhysRevD.23.287.
  2. 1 2 Bekenstein, Jacob D. (2005). “How does the Entropy/Information Bound Work?”. Foundations of Physics. 35 (11): 1805–1823. arXiv:quant-ph/0404042. Bibcode:2005FoPh...35.1805B. doi:10.1007/s10701-005-7350-7.
  3. 1 2 Bekenstein, Jacob (2008). “Bekenstein bound”. Scholarpedia. 3 (10): 7374. Bibcode:2008SchpJ...3.7374B. doi:10.4249/scholarpedia.7374.
  4. ↑ Tipler, F. J. (2005). “The structure of the world from pure numbers” (PDF). Reports on Progress in Physics. 68 (4): 897–964. arXiv:0704.3276. Bibcode:2005RPPh...68..897T. doi:10.1088/0034-4885/68/4/R04.
  5. ↑ Jacobson, Ted (1995). “Thermodynamics of Spacetime: The Einstein Equation of State” (PDF). Physical Review Letters. 75 (7): 1260–1263. arXiv:gr-qc/9504004. Bibcode:1995PhRvL..75.1260J. CiteSeerX 10.1.1.54.6675. doi:10.1103/PhysRevLett.75.1260. PMID 10060248. Bản gốc (PDF) lưu trữ ngày 23 tháng 5 năm 2010. Truy cập ngày 3 tháng 6 năm 2020.
  6. ↑ Lee Smolin, Three Roads to Quantum Gravity (New York, N.Y.: Basic Books, 2002), pp. 173 and 175, ISBN 0-465-07836-2, LCCN 2007-310371.
  7. ↑ Bousso, Raphael (1999). “Holography in general space-times”. Journal of High Energy Physics. 1999 (6): 028. arXiv:hep-th/9906022. Bibcode:1999JHEP...06..028B. doi:10.1088/1126-6708/1999/06/028.
  8. ↑ Bousso, Raphael (1999). “A covariant entropy conjecture”. Journal of High Energy Physics. 1999 (7): 004. arXiv:hep-th/9905177. Bibcode:1999JHEP...07..004B. doi:10.1088/1126-6708/1999/07/004.
  9. ↑ Bousso, Raphael (2000). “The holographic principle for general backgrounds”. Classical and Quantum Gravity. 17 (5): 997–1005. arXiv:hep-th/9911002. Bibcode:2000CQGra..17..997B. doi:10.1088/0264-9381/17/5/309.
  10. ↑ Bekenstein, Jacob D. (2000). “Holographic bound from second law of thermodynamics”. Physics Letters B. 481 (2–4): 339–345. arXiv:hep-th/0003058. Bibcode:2000PhLB..481..339B. doi:10.1016/S0370-2693(00)00450-0.
  11. ↑ Bousso, Raphael (2002). “The holographic principle” (PDF). Reviews of Modern Physics. 74 (3): 825–874. arXiv:hep-th/0203101. Bibcode:2002RvMP...74..825B. doi:10.1103/RevModPhys.74.825. Bản gốc (PDF) lưu trữ ngày 23 tháng 5 năm 2010. Truy cập ngày 3 tháng 6 năm 2020.
  12. ↑ Jacob D. Bekenstein, "Information in the Holographic Universe: Theoretical results about black holes suggest that the universe could be like a gigantic hologram", Scientific American, Vol. 289, No. 2 (August 2003), pp. 58-65. Mirror link.
  13. ↑ Bousso, Raphael; Flanagan, Éanna É.; Marolf, Donald (2003). “Simple sufficient conditions for the generalized covariant entropy bound”. Physical Review D. 68 (6): 064001. arXiv:hep-th/0305149. Bibcode:2003PhRvD..68f4001B. doi:10.1103/PhysRevD.68.064001.
  14. ↑ Bekenstein, Jacob D. (2004). “Black holes and information theory”. Contemporary Physics. 45 (1): 31–43. arXiv:quant-ph/0311049. Bibcode:2004ConPh..45...31B. doi:10.1080/00107510310001632523.
  15. ↑ Tipler, F. J. (2005). “The structure of the world from pure numbers” (PDF). Reports on Progress in Physics. 68 (4): 897–964. arXiv:0704.3276. Bibcode:2005RPPh...68..897T. doi:10.1088/0034-4885/68/4/R04.. Tipler gives a number of arguments for maintaining that Bekenstein's original formulation of the bound is the correct form. See in particular the paragraph beginning with "A few points..." on p. 903 of the Rep. Prog. Phys. paper (or p. 9 of the arXiv version), and the discussions on the Bekenstein bound that follow throughout the paper.
  16. ↑ Casini, Horacio (2008). “Relative entropy and the Bekenstein bound”. Classical and Quantum Gravity. 25 (20): 205021. arXiv:0804.2182. Bibcode:2008CQGra..25t5021C. doi:10.1088/0264-9381/25/20/205021.