| | <blockquote>Astrophysical black holes almost certainly exist, but [[Stephen Hawking|Hawking]]<ref name="Hawking1976" group="q">[[Stephen Hawking|S. W. Hawking]], [http://www.physics.princeton.edu/~mcdonald/examples/QM/hawking_prd_14_2460_76.pdf "Breakdown of predictability in gravitational collapse"], ''Physical Review D'', Vol. 14, Issue 10 (November 1976), pp. 2460-2473, {{doi|10.1103/PhysRevD.14.2460}}, {{bibcode|1976PhRvD..14.2460H}}. [http://www.webcitation.org/5o9PpPxNW Mirror link].</ref> and Wald<ref name="Wald1994" group="q">Robert M. Wald, ''Quantum Field Theory in Curved Spacetime and Black Hole Thermodynamics'' (Chicago: University of Chicago Press, 1994), ISBN 0226870251, {{lccn|94011065}}, Section 7.3, pp. 182-185.</ref> have shown that if black holes are allowed to exist for unlimited proper time, then they will completely evaporate, and unitarity will be violated. Thus, unitarity requires that the universe must cease to exist after finite proper time, which implies that the universe has spatial topology ''S''<sup>3</sup>.<ref name="Barrow1986" group="q">John D. Barrow, Gregory J. Galloway and Frank J. Tipler, [http://adsabs.harvard.edu/abs/1986MNRAS.223..835B "The closed-universe recollapse conjecture"], ''Monthly Notices of the Royal Astronomical Society'', Vol. 223, No. 4 (December 1986), pp. 835-844, {{bibcode|1986MNRAS.223..835B}}, CAT.INIST No. [http://cat.inist.fr/?aModele=afficheN&cpsidt=8251334 8251334]. On p. 926 of the same 2005 ''Reports on Progress in Physics'' paper, Tipler writes that "A dynamical proof for ''S''<sup>3</sup> can be found in Barrow (1986)", with "Barrow (1986)" being this reference.</ref> The [[Second law of thermodynamics|Second Law of Thermodynamics]] says the amount of entropy in the universe cannot decrease, but Ellis and Coule<ref name="EllisCoule1994" group="q">G. F. R. Ellis and D. H. Coule, [http://www.springerlink.com/content/xh785g1534074045/ "Life at the end of the universe?"], ''General Relativity and Gravitation'', Vol. 26, No. 7 (July 1994), pp. 731-739, {{doi|10.1007/BF02116959}}, {{bibcode|1994GReGr..26..731E}}.</ref> and I<ref name="Tipler1994" group="q">Frank J. Tipler, ''The Physics of Immortality: Modern Cosmology, God and the Resurrection of the Dead'' (New York: Doubleday, 1994), ISBN 0385467982, {{lccn|93045046}}, {{bibcode|1994pimc.book.....T}}, Appendix C: "The Bekenstein Bound", p. 410. Said Appendix is reproduced in Frank J. Tipler, [http://arxiv.org/abs/astro-ph/0111520 "Genesis: How the Universe Began According to Standard Model Particle Physics"], {{arxiv|astro-ph/0111520}}, November 28, 2001, Section 2: "Apparent Inconsistences in the Physical Laws in the Early Universe", Subsection a: "Bekenstein Bound Inconsistent with Second Law of Thermodynamics".</ref> have shown that the amount of entropy already in the CMBR will eventually contradict the Bekenstein Bound near the final singularity unless there are no [[event horizon]]s, since in the presence of horizons the Bekenstein Bound implies the universal entropy ''S'' ≤ constant × ''R''<sup>2</sup>, where ''R'' is the radius of the universe, and [[general relativity]] requires ''R'' → 0 at the final singularity. If there are no horizons then the (shear) energy density can grow as ''R''<sup>−6</sup> which means that the total available energy grows as (''R''<sup>−6</sup> ) ''R''<sup>3</sup> ~ ''R''<sup>−3</sup>, and so the Bekenstein Bound yields ''E R'' ~ (''R''<sup>−3</sup>)''R'' ~ ''R''<sup>−2</sup> which diverges as ''R''<sup>−2</sup> as ''R'' → 0 at the final singularity.<ref name="Tipler2003" group="q">Frank J. Tipler, [http://theophysics.freevar.com/pdf/tipler-intelligent-life-in-cosmology.pdf "Intelligent life in cosmology"], ''International Journal of Astrobiology'', Vol. 2, Issue 2 (April 2003), pp. 141-148, {{doi|10.1017/S1473550403001526}}, {{bibcode|2003IJAsB...2..141T}}. Mirror links [http://www.webcitation.org/5o9QHKGuW here] and [http://theophysics.host56.com/pdf/tipler-intelligent-life-in-cosmology.pdf here]; also available [http://math.tulane.edu/~tipler/intelligentlife.pdf here]. Also at {{arxiv|0704.0058}}, March 31, 2007.</ref><ref name="Tipler1994" group="q"/> The absence of event horizons by definition means that the universe's future c-boundary is a single point,<ref name="HawkingEllis1973" group="q">[[Stephen Hawking|S. W. Hawking]] and G. F. R. Ellis, ''The Large Scale Structure of Space-Time'' (London: [[Cambridge University Press]], 1973), ISBN 0521200164, {{lccn|72093671}}, {{bibcode|1973lsss.book.....H}}, pp. 217-221.</ref> call it the ''Omega Point''. MacCallum<ref name="MacCallum1971" group="q">Malcolm A. H. MacCallum, "Mixmaster universe problem", ''Nature—Physical Science'', Vol. 230 (March 1971), pp. 112-113, {{bibcode|1971Natur.230..112M}}, {{OSTI|4048469}}. See also [http://www.maths.qmul.ac.uk/~mm/papers.html here].</ref> has shown that an ''S''<sup>3</sup> closed universe with a single point future c-boundary is of measure zero in initial data space. Barrow,<ref name="Barrow 1982" group="q">John D. Barrow, "Chaotic behaviour in general relativity", ''Physics Reports'', Vol. 85, Issue 1 (May 1982), pp. 1-49, {{doi|10.1016/0370-1573(82)90171-5}}, {{bibcode|1982PhR....85....1B}}.</ref><ref name="Barrow1998" group="q">John D. Barrow and Janna Levin, [http://link.aps.org/doi/10.1103/PhysRevLett.80.656 "Chaos in the Einstein-Yang-Mills Equations"], ''Physical Review Letters'', Vol. 80, Issue 4 (January 1998), pp. 656-659, {{doi|10.1103/PhysRevLett.80.656}}, {{bibcode|1998PhRvL..80..656B}}. Also at {{arxiv|gr-qc/9706065}}, June 20, 1997.</ref> Cornish and Levin<ref name="CornishLevin1997" group="q">Neil J. Cornish and Janna J. Levin, [http://link.aps.org/doi/10.1103/PhysRevD.55.7489 "Mixmaster universe: A chaotic Farey tale"], ''Physical Review D'', Vol. 55, Issue 12 (June 1997), pp. 7489-7510, {{doi|10.1103/PhysRevD.55.7489}}, {{bibcode|1997PhRvD..55.7489C}}. Also at {{arxiv|gr-qc/9612066}}, December 30, 1996.</ref> and Motter<ref name="Motter2003" group="q">Adilson E. Motter, [http://llacolen.ciencias.uchile.cl/~vmunoz/download/papers/m03a.pdf "Relativistic Chaos is Coordinate Invariant"], ''Physical Review Letters'', Vol. 91, Issue 23 (December 2003), Art. No. 231101, 4 pages, {{doi|10.1103/PhysRevLett.91.231101}}, {{bibcode|2003PhRvL..91w1101M}}. [http://www.webcitation.org/5o9Pa8B4M Mirror link]. Also at {{arxiv|gr-qc/0305020}}, May 5, 2003.</ref> have shown that the evolution of an ''S''<sup>3</sup> closed universe into its final singularity is chaotic. Yorke ''et al.''<ref name="Yorke1990" group="q">Troy Shinbrot, Edward Ott, Celso Grebogi and James A. Yorke, [http://link.aps.org/doi/10.1103/PhysRevLett.65.3215 "Using chaos to direct trajectories to targets"], ''Physical Review Letters'', Vol. 65, Issue 26 (December 1990), pp. 3215-3218, {{doi|10.1103/PhysRevLett.65.3215}}, {{bibcode|1990PhRvL..65.3215S}}.</ref><ref name="Yorke1992" group="q">Troy Shinbrot, William Ditto, Celso Grebogi, Edward Ott, Mark Spano and James A. Yorke, [http://link.aps.org/doi/10.1103/PhysRevLett.68.2863 "Using the sensitive dependence of chaos (the 'butterfly effect') to direct trajectories in an experimental chaotic system"], ''Physical Review Letters'', Vol. 68, Issue 19 (May 1992), pp. 2863-2866, {{doi|10.1103/PhysRevLett.68.2863}}, {{bibcode|1992PhRvL..68.2863S}}.</ref> have shown that a chaotic physical system is likely to evolve into a measure zero state if and only if its control parameters are intelligently manipulated. Thus life (≡intelligent computers) almost certainly must be present ''arbitrarily close'' to the final singularity in order for the known laws of physics to be mutually consistent at all times. Misner<ref name="Misner1968" group="q">Charles W. Misner, [http://adsabs.harvard.edu/abs/1968ApJ...151..431M "The Isotropy of the Universe"], ''Astrophysical Journal'', Vol. 151 (February 1968), pp. 431-457, {{doi|10.1086/149448}}, {{bibcode|1968ApJ...151..431M}}.</ref><ref name="Misner1969a" group="q">Charles W. Misner, [http://link.aps.org/doi/10.1103/PhysRev.186.1319 "Quantum Cosmology. I"], ''Physical Review'', Vol. 186, Issue 5 (October 1969), pp. 1319-1327, {{doi|10.1103/PhysRev.186.1319}}, {{bibcode|1969PhRv..186.1319M}}.</ref><ref name="Misner1969b" group="q">Charles W. Misner, [http://astrophysics.fic.uni.lodz.pl/100yrs/pdf/07/036.pdf "Mixmaster Universe"], ''Physical Review Letters'', Vol. 22, Issue 20 (May 1969), pp. 1071-1074, {{doi|10.1103/PhysRevLett.22.1071}}, {{bibcode|1969PhRvL..22.1071M}}. [http://www.webcitation.org/5oFUpabxe Mirror link]. Also available as [http://www.gravityresearchfoundation.org/pdf/awarded/1969/minner.pdf an entry] in the Gravity Research Foundation's 1969 essay competition. [http://www.webcitation.org/5oFmSHFDm Mirror link].</ref> has shown in effect that event horizon elimination requires an infinite number of distinct manipulations, so an infinite amount of information must be processed between now and the final singularity. The amount of information stored at any time diverges to infinity as the Omega Point is approached, since ''S'' → +∞ there, implying divergence of the complexity of the system that must be understood to be controlled.</blockquote> | | <blockquote>Astrophysical black holes almost certainly exist, but [[Stephen Hawking|Hawking]]<ref name="Hawking1976" group="q">[[Stephen Hawking|S. W. Hawking]], [http://www.physics.princeton.edu/~mcdonald/examples/QM/hawking_prd_14_2460_76.pdf "Breakdown of predictability in gravitational collapse"], ''Physical Review D'', Vol. 14, Issue 10 (November 1976), pp. 2460-2473, {{doi|10.1103/PhysRevD.14.2460}}, {{bibcode|1976PhRvD..14.2460H}}. [http://www.webcitation.org/5o9PpPxNW Mirror link].</ref> and Wald<ref name="Wald1994" group="q">Robert M. Wald, ''Quantum Field Theory in Curved Spacetime and Black Hole Thermodynamics'' (Chicago: University of Chicago Press, 1994), ISBN 0226870251, {{lccn|94011065}}, Section 7.3, pp. 182-185.</ref> have shown that if black holes are allowed to exist for unlimited proper time, then they will completely evaporate, and unitarity will be violated. Thus, unitarity requires that the universe must cease to exist after finite proper time, which implies that the universe has spatial topology ''S''<sup>3</sup>.<ref name="Barrow1986" group="q">John D. Barrow, Gregory J. Galloway and Frank J. Tipler, [http://adsabs.harvard.edu/abs/1986MNRAS.223..835B "The closed-universe recollapse conjecture"], ''Monthly Notices of the Royal Astronomical Society'', Vol. 223, No. 4 (December 1986), pp. 835-844, {{bibcode|1986MNRAS.223..835B}}, CAT.INIST No. [http://cat.inist.fr/?aModele=afficheN&cpsidt=8251334 8251334]. On p. 926 of the same 2005 ''Reports on Progress in Physics'' paper, Tipler writes that "A dynamical proof for ''S''<sup>3</sup> can be found in Barrow (1986)", with "Barrow (1986)" being this reference.</ref> The [[Second law of thermodynamics|Second Law of Thermodynamics]] says the amount of entropy in the universe cannot decrease, but Ellis and Coule<ref name="EllisCoule1994" group="q">G. F. R. Ellis and D. H. Coule, [http://www.springerlink.com/content/xh785g1534074045/ "Life at the end of the universe?"], ''General Relativity and Gravitation'', Vol. 26, No. 7 (July 1994), pp. 731-739, {{doi|10.1007/BF02116959}}, {{bibcode|1994GReGr..26..731E}}.</ref> and I<ref name="Tipler1994" group="q">Frank J. Tipler, ''The Physics of Immortality: Modern Cosmology, God and the Resurrection of the Dead'' (New York: Doubleday, 1994), ISBN 0385467982, {{lccn|93045046}}, {{bibcode|1994pimc.book.....T}}, Appendix C: "The Bekenstein Bound", p. 410. Said Appendix is reproduced in Frank J. Tipler, [http://arxiv.org/abs/astro-ph/0111520 "Genesis: How the Universe Began According to Standard Model Particle Physics"], {{arxiv|astro-ph/0111520}}, November 28, 2001, Section 2: "Apparent Inconsistences in the Physical Laws in the Early Universe", Subsection a: "Bekenstein Bound Inconsistent with Second Law of Thermodynamics".</ref> have shown that the amount of entropy already in the CMBR will eventually contradict the Bekenstein Bound near the final singularity unless there are no [[event horizon]]s, since in the presence of horizons the Bekenstein Bound implies the universal entropy ''S'' ≤ constant × ''R''<sup>2</sup>, where ''R'' is the radius of the universe, and [[general relativity]] requires ''R'' → 0 at the final singularity. If there are no horizons then the (shear) energy density can grow as ''R''<sup>−6</sup> which means that the total available energy grows as (''R''<sup>−6</sup> ) ''R''<sup>3</sup> ~ ''R''<sup>−3</sup>, and so the Bekenstein Bound yields ''E R'' ~ (''R''<sup>−3</sup>)''R'' ~ ''R''<sup>−2</sup> which diverges as ''R''<sup>−2</sup> as ''R'' → 0 at the final singularity.<ref name="Tipler2003" group="q">Frank J. Tipler, [http://theophysics.freevar.com/pdf/tipler-intelligent-life-in-cosmology.pdf "Intelligent life in cosmology"], ''International Journal of Astrobiology'', Vol. 2, Issue 2 (April 2003), pp. 141-148, {{doi|10.1017/S1473550403001526}}, {{bibcode|2003IJAsB...2..141T}}. Mirror links [http://www.webcitation.org/5o9QHKGuW here] and [http://theophysics.host56.com/pdf/tipler-intelligent-life-in-cosmology.pdf here]; also available [http://math.tulane.edu/~tipler/intelligentlife.pdf here]. Also at {{arxiv|0704.0058}}, March 31, 2007.</ref><ref name="Tipler1994" group="q"/> The absence of event horizons by definition means that the universe's future c-boundary is a single point,<ref name="HawkingEllis1973" group="q">[[Stephen Hawking|S. W. Hawking]] and G. F. R. Ellis, ''The Large Scale Structure of Space-Time'' (London: [[Cambridge University Press]], 1973), ISBN 0521200164, {{lccn|72093671}}, {{bibcode|1973lsss.book.....H}}, pp. 217-221.</ref> call it the ''Omega Point''. MacCallum<ref name="MacCallum1971" group="q">Malcolm A. H. MacCallum, "Mixmaster universe problem", ''Nature—Physical Science'', Vol. 230 (March 1971), pp. 112-113, {{bibcode|1971Natur.230..112M}}, {{OSTI|4048469}}. See also [http://www.maths.qmul.ac.uk/~mm/papers.html here].</ref> has shown that an ''S''<sup>3</sup> closed universe with a single point future c-boundary is of measure zero in initial data space. Barrow,<ref name="Barrow 1982" group="q">John D. Barrow, "Chaotic behaviour in general relativity", ''Physics Reports'', Vol. 85, Issue 1 (May 1982), pp. 1-49, {{doi|10.1016/0370-1573(82)90171-5}}, {{bibcode|1982PhR....85....1B}}.</ref><ref name="Barrow1998" group="q">John D. Barrow and Janna Levin, [http://link.aps.org/doi/10.1103/PhysRevLett.80.656 "Chaos in the Einstein-Yang-Mills Equations"], ''Physical Review Letters'', Vol. 80, Issue 4 (January 1998), pp. 656-659, {{doi|10.1103/PhysRevLett.80.656}}, {{bibcode|1998PhRvL..80..656B}}. Also at {{arxiv|gr-qc/9706065}}, June 20, 1997.</ref> Cornish and Levin<ref name="CornishLevin1997" group="q">Neil J. Cornish and Janna J. Levin, [http://link.aps.org/doi/10.1103/PhysRevD.55.7489 "Mixmaster universe: A chaotic Farey tale"], ''Physical Review D'', Vol. 55, Issue 12 (June 1997), pp. 7489-7510, {{doi|10.1103/PhysRevD.55.7489}}, {{bibcode|1997PhRvD..55.7489C}}. Also at {{arxiv|gr-qc/9612066}}, December 30, 1996.</ref> and Motter<ref name="Motter2003" group="q">Adilson E. Motter, [http://llacolen.ciencias.uchile.cl/~vmunoz/download/papers/m03a.pdf "Relativistic Chaos is Coordinate Invariant"], ''Physical Review Letters'', Vol. 91, Issue 23 (December 2003), Art. No. 231101, 4 pages, {{doi|10.1103/PhysRevLett.91.231101}}, {{bibcode|2003PhRvL..91w1101M}}. [http://www.webcitation.org/5o9Pa8B4M Mirror link]. Also at {{arxiv|gr-qc/0305020}}, May 5, 2003.</ref> have shown that the evolution of an ''S''<sup>3</sup> closed universe into its final singularity is chaotic. Yorke ''et al.''<ref name="Yorke1990" group="q">Troy Shinbrot, Edward Ott, Celso Grebogi and James A. Yorke, [http://link.aps.org/doi/10.1103/PhysRevLett.65.3215 "Using chaos to direct trajectories to targets"], ''Physical Review Letters'', Vol. 65, Issue 26 (December 1990), pp. 3215-3218, {{doi|10.1103/PhysRevLett.65.3215}}, {{bibcode|1990PhRvL..65.3215S}}.</ref><ref name="Yorke1992" group="q">Troy Shinbrot, William Ditto, Celso Grebogi, Edward Ott, Mark Spano and James A. Yorke, [http://link.aps.org/doi/10.1103/PhysRevLett.68.2863 "Using the sensitive dependence of chaos (the 'butterfly effect') to direct trajectories in an experimental chaotic system"], ''Physical Review Letters'', Vol. 68, Issue 19 (May 1992), pp. 2863-2866, {{doi|10.1103/PhysRevLett.68.2863}}, {{bibcode|1992PhRvL..68.2863S}}.</ref> have shown that a chaotic physical system is likely to evolve into a measure zero state if and only if its control parameters are intelligently manipulated. Thus life (≡intelligent computers) almost certainly must be present ''arbitrarily close'' to the final singularity in order for the known laws of physics to be mutually consistent at all times. Misner<ref name="Misner1968" group="q">Charles W. Misner, [http://adsabs.harvard.edu/abs/1968ApJ...151..431M "The Isotropy of the Universe"], ''Astrophysical Journal'', Vol. 151 (February 1968), pp. 431-457, {{doi|10.1086/149448}}, {{bibcode|1968ApJ...151..431M}}.</ref><ref name="Misner1969a" group="q">Charles W. Misner, [http://link.aps.org/doi/10.1103/PhysRev.186.1319 "Quantum Cosmology. I"], ''Physical Review'', Vol. 186, Issue 5 (October 1969), pp. 1319-1327, {{doi|10.1103/PhysRev.186.1319}}, {{bibcode|1969PhRv..186.1319M}}.</ref><ref name="Misner1969b" group="q">Charles W. Misner, [http://astrophysics.fic.uni.lodz.pl/100yrs/pdf/07/036.pdf "Mixmaster Universe"], ''Physical Review Letters'', Vol. 22, Issue 20 (May 1969), pp. 1071-1074, {{doi|10.1103/PhysRevLett.22.1071}}, {{bibcode|1969PhRvL..22.1071M}}. [http://www.webcitation.org/5oFUpabxe Mirror link]. Also available as [http://www.gravityresearchfoundation.org/pdf/awarded/1969/minner.pdf an entry] in the Gravity Research Foundation's 1969 essay competition. [http://www.webcitation.org/5oFmSHFDm Mirror link].</ref> has shown in effect that event horizon elimination requires an infinite number of distinct manipulations, so an infinite amount of information must be processed between now and the final singularity. The amount of information stored at any time diverges to infinity as the Omega Point is approached, since ''S'' → +∞ there, implying divergence of the complexity of the system that must be understood to be controlled.</blockquote> |