Skip to main content Accessibility help
×
Hostname: page-component-848d4c4894-4rdrl Total loading time: 0 Render date: 2024-06-27T16:39:13.804Z Has data issue: false hasContentIssue false

17 - The Big Bang, quantum gravity and black-hole information loss

Published online by Cambridge University Press:  05 August 2012

Roger Penrose
Affiliation:
The Mathematical Institute
Jeff Murugan
Affiliation:
University of Cape Town
Amanda Weltman
Affiliation:
University of Cape Town
George F. R. Ellis
Affiliation:
University of Cape Town
Get access

Summary

I argue that the common idea of applying standard quantization procedures to the space-time geometry at the Big Bang to obtain a Planck-scale chaotic geometry is likely to be wrong, whilst such a quantum-geometric structure could indeed have relevance at black-hole singularities, these appearing to lead to a necessity of information loss. These issues are addressed by re-examining the basic rules of quantum theory in a gravitational context and by viewing things from the perspective of conformal cyclic cosmology, which is dependent upon the idea of conformal space-time geometry. This kind of geometry is also central to twistor theory, a subject in which significant advances have been made in recent years.

General remarks

What follows is essentially an extended summary of my actual talk, which I hope adequately conveys the gist of what I did report at the Stellenbosch meeting. I hope, also, that it can serve as a small token of the great respect that I have for George Ellis – in the honouring of his 70th birthday – both as a person and for the enormous contributions that he has made to science and to the cause of humanity.

I briefly discuss three different topics, all of which have relevance to the nature of quantum space-time geometry. The first has to do with the very framework of quantum theory in relation to Einstein's foundational principle of equivalence, and provides a reason for anticipating a change in the rules of quantum mechanics when superpositions of significant displacements of mass are involved.

Type
Chapter
Information
Foundations of Space and Time
Reflections on Quantum Gravity
, pp. 410 - 418
Publisher: Cambridge University Press
Print publication year: 2012

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

[1] Colella, R., Overhauser, A. W. and Werner, S. A. (1975) Phys. Rev. Lett. 34, 1472.
[2] Bonse, U. and Wroblewski, T. (1983) Phys. Rev. Lett. 51, 1401.
[3] Penrose, R. (2004) The Road to Reality: A Complete Guide to the Laws of the Universe (Jonathan Cape, London).
[4] Penrose, R. (2009) Black holes, quantum theory and cosmology. J. Phys.: Conf. Ser. 174, 012001 (15pp) http://www.iop.org/EJ/toc/1742-6596/174/1.Google Scholar
[5] Disi, L. (1984) Gravitation and quantum mechanical localization of macro-objects. Phys. Lett. 105A, 199–202.Google Scholar
[6] Disi, L. (1987) Phys. Lett. 120A, 377.
[7] Disi, L. (1989) Models for universal reduction of macroscopic quantum fluctuations. Phys. Rev. A40, 1165–74.Google Scholar
[8] Penrose, R. (1993) Gravity and quantum mechanics. In General Relativity and Gravitation 13, Cordoba, Argentina. Part 1: Plenary Lectures 1992. (Eds R. J., Gleiser, C. N., Kozameh and O. M., Moreschi, Institute of Physics Publishing, Bristol & Philadelphia), pp. 179–89.
[9] Penrose, R. (1996) On gravity's role in quantum state reduction. Gen. Rel. Grav. 28, 581–600.Google Scholar
[10] Penrose, R. (2000a) Wavefunction collapse as a real gravitational effect. In Mathematical Physics 2000, eds A., Fokas, T. W. B., Kibble, A., Grigouriou and B., Zegarlinski (Imperial College Press, London), pp. 266–82.
[11] Tod, K. P. (2003) Isotropic cosmological singularities: other matter models. Class. Quant. Grav. 20, 521–34. doi:10.1088/0264-9381/20/3/309.Google Scholar
[12] Rugh, S. E. and Zinkernagel, H. (2007) Cosmology and the meaning of time (Symposium, The Socrates Spirit Section for Philosophy and the Foundations of Physics, Hellabaekgade 27, Copenhagen N, Denmark).
[13] Penrose, R. (2006) Before the big bang: an outrageous new perspective and its implications for particle physics. In EPAC 2006 Proceedings, Edinburgh, Scotland, pp. 2759–62, ed. C. R., Prior (European Physical Society Accelerator Group, EPS-AG). http://accelconf.web.cern.ch/AccelConf/e06/PAPERS/THESPA01.PDF.
[14] Penrose, R. (2008) Causality, quantum theory and cosmology. In On Space and Time, ed. S., Majid (Cambridge University Press, Cambridge), pp. 141–95.
[15] Ellis, G. F. R. (2009) Dark energy and inhomogeneity (paper for NEB XIII conference, Thessaloniki, 2008).
[16] Braunstein, S. L. and Pati, A. K. (2007) Quantum information cannot be completely hidden in correlations: implications for the black-hole information paradox. Phys. Rev. Lett. 98, 080502.Google Scholar
[17] Unruh, W. G. (1976) Notes on black hole evaporation. Phys. Rev. D14, 870.Google Scholar
[18] Penrose, R. and Rindler, W. (1986) Spinors and Space-Time, Vol. 2: Spinor and Twistor Methods in Space-Time Geometry (Cambridge University Press, Cambridge).
[19] Penrose, R. (2005) The twistor approach to space-time structures. In 100 Years of Relativity; Space-time Structure: Einstein and Beyond, ed. A., Ashtekar (World Scientific, Singapore).
[20] Penrose, R. and MacCallum, M. A. H. (1972) Twistor theory: an approach to the quantization of fields and space-time. Phys. Repts. 6C, 241–315.Google Scholar
[21] Hodges, A. P. (1982) Twistor diagrams. Physica 114A, 157–75.Google Scholar
[22] Hodges, A. P. (1985) A twistor approach to the regularization of divergences. Proc. Roy. Soc. London A397, 341–74.Google Scholar
Mass eigenstates in twistor theory, Proc. Roy. Soc. London A397, 375–96.
[23] Hodges, A. P. (1998) The twistor diagram programme. In The Geometric Universe; Science, Geometry, and the Work of Roger Penrose, eds S. A., Huggett, L. J., Mason, K. P., Tod, S. T., Tsou, and N. M. J., Woodhouse (Oxford University Press, Oxford).
[24] Witten, E. (2004) Perturbative gauge theory as a string theory in twistor space. Commun. Math. Phys. 252, 189–258. arXiv:hep-th/0312171v2.Google Scholar
[25] Parke, S. and Taylor, T. (1986) An amplitude for N gluon scatterings. Phys. Rev. Lett. 56, 2459.Google Scholar
[26] Nair, V. (1988) A current algebra for some gauge theory amplitudes. Phys. Lett. B214, 215.Google Scholar
[27] Mason, L. J. and Skinner, D. (2009) Scattering amplitudes and BCFW recursion in twistor space. arXiv:0903.2083v3.
[28] Arkani-Hamed, N., Cachazo, F., Cheung, C., and Kaplan, J. (2009) The s-matrix in twistor space. arXiv:0903.2110v2 [hep-th].
[29] Penrose, R. (2000a) On extracting the googly information. Twistor Newsletter 45, 1–24.Google Scholar
[30] Hodges, A. P. (2006a) Twistor diagrams for all tree amplitudes in gauge theory: a helicity-independent formalism. arXiv:hep-th/0512336v2.
[31] Hodges, A. P. (2006b) Scattering amplitudes for eight gauge fields. arXiv:hep-th/0603101v1.

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×