Arrow of time in a recollapsing quantum universe
Open accessAbstract
We argue that the Wheeler-DeWitt equation with a consistent boundary condition is only compatible with an arrow of time that formally reverses in a recollapsing universe. To recover a classically recollapsing universe in terms of wave packets, we impose the usual boundary condition of excluding exponentially increasing wave functions for large scale factors. Consistency of these opposite arrows is then facilitated by quantum effects in the region of the classical turning point. We also discuss in this context the meaning of the time-asymmetric expression used in the definition of ``consistent histories.'' Since gravitational time dilation diverges at horizons, one has to conclude that collapsing matter must start reexpanding ``anticausally'' (controlled by the reversed arrow) in this scenario before horizons or singularities can form. There would then also be no mass inflation nor any information loss paradox.
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Every observer in this quantum universe would only be able to see an expanding universe.
“Every observer in this quantum universe would thus only be able to see an expanding universe (Kiefer and Zeh 1995).”
From On a quantum Weyl curvature hypothesis (2022) · cites this paper as Kiefer and Zeh 1995
In a classically recollapsing universe, the quantum theory does not distinguish between the regions with a classical big bang and a classical big crunch; they correspond to the same region in configuration space with small a.
“Since the quantum theory does not distinguish between the regions with a classical big bang and a classical big crunch (they both correspond to the same region in configuration space with small a ), imposing low entropy for the 'big bang' directly leads to low entropy for the 'big crunch'.”
From On a quantum Weyl curvature hypothesis (2022) · cites this paper as Kiefer and Zeh 1995
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Cites
Consistent histories and the interpretation of quantum mechanics
Griffiths, R. B. (1984) · Journal of Statistical Physics · doi:10.1007/bf01015734 · Cited by 1,138 · see citing works
There are no quantum jumps, nor are there particles!
Zeh, H. D. (1993) · Physics Letters A · doi:10.1016/0375-9601(93)91005-p · Cited by 117 · see citing works
Self-citationWhat is the geometry of superspace?
Giulini, D. (1995) · Physical Review D · doi:10.1103/physrevd.51.5630 · Cited by 74 · see citing works
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Research works printed but not linked: 35
- [1][1] H.D. Zeh, The Physical Basis of the Direction of Time (Springer, Berlin, 1992). -
- [2][2] H. Price, in Time's Arrow Today , edited by S. Savitt (Cambridge University Press, Cambridge, 1994). -
- [3][3] H.D. Zeh, in Physical Origins of Time Asymmetry , edited by J.J. Halliwell, J.P. Perez-Mercader and W.H. Zurek (Cambridge University Press, Cambridge, 1994). -
- [5][5] R. Penrose, in Quantum Gravity 2 , edited by C.J. Isham, R. Penrose and D.W. Sciama (Clarendon Press, London, 1981). -
- [6][6] J.B. Barbour, in Quantum Concepts in Space and Time , edited by R. Penrose and C.J. Isham (Clarendon Press, London, 1986). -
- [8][8] H.D. Conradi and H.D. Zeh, Phys. Lett. A 154, 321 (1991). -
- [9][9] T. Gold, Am. J. Phys. 30, 403 (1962). -
- [11][11] S.W. Hawking, R. Laflamme and G.W. Lyons, Phys. Rev. D 47, 5342 (1993). -
- [12][12] D.N. Page, Phys. Rev. D 32, 2496 (1985). -
- [13][13] S.W. Hawking, Phys. Rev. D 32, 2489 (1985). -
- [14][14] J.B. Hartle and S.W. Hawking, Phys. Rev. D 28, 2960 (1983). -
- [15][15] H.D. Zeh, Phys. Lett. A 116, 9 (1986). -
- [16][16] H.D. Zeh, Phys. Lett. A 126, 311 (1988). -
- [17][17] H.D. Zeh, in Complexity, Entropy and the Physics of Information , edited by W.H. Zurek (Addison-Wesley, Reading, Mass., 1990). -
- [18][18] J.J. Halliwell and S.W. Hawking, Phys. Rev. D 31, 1777 (1985). -
- [20][20] A. Higuchi and R. Wald, Applications of a new proposal for solving the 'problem of time' to some simple quantum cosmological models , Preprint gr-qc/9407038 (1994). - · arXiv
- [21][21] C. Kiefer, Phys. Rev. D 38, 1761 (1988). -
- [22][22] J.J. Halliwell and M.E. Ortiz, Phys. Rev. D 48, 748 (1993). -
- [23][23] J.B. Hartle, in Quantum Physics and the Universe , edited by S. Coleman et al. (World Scientific, Singapore, 1991). -
- [24][24] J.J. Halliwell, Phys. Rev. D 38, 2468 (1988). -
- [25][25] C. Kiefer, Ann. Phys. (N.Y.) 207, 53 (1991). -
- [26][26] R. Laflamme and E.P.S. Shellard, Phys. Rev. D 35, 2315 (1987). -
- [27][27] C. Kiefer, Class. Quantum Grav. 4, 1369 (1987). -
- [28][28] J.B. Barbour, Phys. Rev. D 47, 5422 (1993). -
- [29][29] H.D. Zeh, in Stochastic Evolution of Quantum States in Open Systems and in Measurement Processes , edited by L. Di´ osi and B. Luk´ acs (World Scientific, Singapore, 1994). -
- [30][30] C. Kiefer, Phys. Rev. D 47, 5414 (1993). -
- [31][31] R. Laflamme, Class. Quantum Grav. 10, L79 (1993). -
- [33][33] P.C.W. Davies and J. Twamley, Class. Quantum Grav. 10, 931 (1993). -
- [34][34] R.B. Partridge, Nature 244, 263 (1973). -
- [35][35] H.D. Zeh, Phys. Lett. A 172, 189 (1993). -
- [36][36] E. Joos, Phys. Rev. D 29, 1626 (1984). -
- [37][37] J.P. Paz and W.H. Zurek, Phys. Rev. D 48, 2728 (1993). -
- [38][38] R. Griffiths, J. Stat. Phys. 36, 219 (1984). -
- [41][41] D.N. Page, Phys. Rev. Lett. 70, 4034 (1993). -
- [42][42] A.E. Sikkema and W. Israel, Nature 349, 45 (1991).
Cited by
Sorted by citations
Singularity avoidance in Bianchi I quantum cosmology
Kiefer, C., Kwidzinski, N., & Piontek, D. (2019) · The European Physical Journal C · doi:10.1140/epjc/s10052-019-7193-6 · Cited by 50 · see citing works
Self-citationOn a quantum Weyl curvature hypothesis
Kiefer, C. (2022) · AVS Quantum Science · doi:10.1116/5.0076811 · Cited by 10 · see citing works
“Every observer in this quantum universe would thus only be able to see an expanding universe (Kiefer and Zeh 1995).”
BackgroundInfluentialSelf-citation
- Authors
- Kiefer, C., & Zeh, H. D.
- Affiliations
- University of Freiburg (DE)
- ORCID
- Kiefer, C.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1995-04-15
- Volume
- 51
- Issue
- 8
- Pages
- 4145-4153
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W1985544149
- Cited by
- 133
- References
- 3
- Citations by year
- 2026: 1 · 2025: 18 · 2024: 2 · 2023: 17 · 2022: 5 · 2020: 1 · 2019: 5 · 2018: 5 · 2017: 4 · 2016: 7 · 2015: 1 · 2014: 7 · 2013: 4 · 2012: 4
- FWCI
- 2.92
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Keywords
- arrow of time, Wheeler-DeWitt equation, boundary conditions, wave packets, consistent histories, gravitational time dilation, horizon, mass inflation, black hole information paradox, quantum cosmology, turning points
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