Dynamic wormholes, antitrapped surfaces, and energy conditions
Open accessAbstract
It is by now apparent that topology is too crude a tool to accurately characterize a generic traversable wormhole. In two earlier papers we developed a complete characterization of generic but static traversable wormholes, and in the present paper extend the discussion to arbitrary time-dependent (dynamical) wormholes. A local definition of a wormhole throat, free from assumptions about asymptotic flatness, symmetries, future and past null infinities, embedding diagrams, topology, and even time dependence is developed that accurately captures the essence of what a wormhole throat is, and where it is located. Adapting and extending a suggestion due to Page, we define a wormhole throat to be a marginally anti-trapped surface, that is, a closed two-dimensional spatial hypersurface such that one of the two future-directed null geodesic congruences orthogonal to it is just beginning to diverge. Typically a dynamic wormhole will possess two such throats, corresponding to the two orthogonal null geodesic congruences, and these two throats will not coincide (though they do coalesce into a single throat in the static limit). The divergence property of the null geodesics at the marginally anti-trapped surface generalizes the ``flare-out'' condition for an arbitrary wormhole. We derive theorems regarding violations of the null energy condition (NEC) at and near these throats and find that, even for wormholes with arbitrary time dependence, the violation of the NEC is a generic property of wormhole throats. We also discuss wormhole throats in the presence of fully antisymmetric torsion and find that the energy condition violations cannot be dumped into the torsion degrees of freedom. Finally by means of a concrete example we demonstrate that even temporary suspension of energy-condition violations is incompatible with the flare-out property of dynamic throats.
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Multiple (at least two) dynamical wormhole throats form.
“Accordingly, multiple (at least two) dynamical wormhole throats form (Hochberg & Visser 1998).”
From UNIVERSE IN A BLACK HOLE IN EINSTEIN–CARTAN GRAVITY (2016) · cites this paper as Hochberg & Visser 1998
The Abstract (p. 1) says a dynamic wormhole typically has two throats, and the Discussion (p. 29) explains how outgoing and ingoing throats are defined. The unqualified claim that at least two throats form overstates the paper’s qualified statement. (LLM, conf=0.84)
Experimental — accuracy not yet measuredWhen a trapped null surface forms in a black hole, the region within this surface is causally connected and mathematically equivalent to a new, closed universe.
“When a trapped null surface forms in a black hole (Hochberg & Visser 1998), the region within this surface is causally connected and mathematically equivalent to a new, closed universe (Berger et al. 1998;Garfinkle 2004;Popławski 2010cPopławski , 2011a).”
From UNIVERSE IN A BLACK HOLE IN EINSTEIN–CARTAN GRAVITY (2016) · cites this paper as Hochberg & Visser 1998
Section 4.1.1 (p. 14) associates trapped surfaces with gravitational collapse and black-hole physics, supporting the general connection in the clause cited to Hochberg and Visser. It does not state that a trapped null surface forms in a black hole. The sentence cites other works for the separate claim about a new, closed universe. (LLM, conf=0.78)
Experimental — accuracy not yet measuredIn general relativity, the singularity forms before the collapse has completed.
“In general relativity, the singularity forms before the collapse has completed (Landau & Lifshitz 1975;Hochberg & Visser 1998).”
From UNIVERSE IN A BLACK HOLE IN EINSTEIN–CARTAN GRAVITY (2016) · cites this paper as Hochberg & Visser 1998
Section 6.1.1 (p. 24) discusses a collapsing background in a dynamic wormhole model, but does not say when a singularity forms. Section 4.1.1 (p. 14) mentions gravitational collapse and singularity theorems while explicitly distinguishing its wormhole analysis from claims about singularities. Searches for singularity formation and the timing of gravitational collapse found no passage addressing the cited claim. (LLM, conf=0.76)
Experimental — accuracy not yet measuredDuring collapse, multiple trapped null surfaces with a very complicated structure can form in the interior and fold in on themselves.
“During the collapse, multiple trapped null surfaces with a very complicated structure can form in the interior and fold in on themselves (Hochberg & Visser 1998).”
From UNIVERSE IN A BLACK HOLE IN EINSTEIN–CARTAN GRAVITY (2016) · cites this paper as Hochberg & Visser 1998
Section 4.1.6 (p. 17) describes two distinct throats in generic time-dependent wormholes, not multiple trapped surfaces forming inside a collapse. Section 4.1.1 (p. 14) mentions gravitational collapse only as a context for trapped-surface terminology. Our copy does not address surfaces folding in on themselves; searches for collapse, interior trapped surfaces, and folding found no supporting passage. (LLM, conf=0.77)
Experimental — accuracy not yet measured
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Cites
Wald, R. M. (1984) · doi:10.7208/chicago/9780226870373.001.0001 · Cited by 7,188 · see citing works
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Research works printed but not linked: 5
- [10][10] F. De Felice and C.J.S. Clarke, Relativity on curved manifolds , (Cambridge University Press, England, 1990). -
- [12][12] J.A. Schouten, Ricci Calculus (Springer, Berlin, 1954). -
- [13][13] M.B. Green, J.H. Schwarz, and E. Witten, Superstring theory (Vol 2: Loop amplitudes, anomalies, and phenomenology) , (Cambridge University Press, England, 1987). -
- [17][17] B. Carter, 'The general theory of the mechanical, electromagnetic and thermodynamic properties of black holes', in General Relativity: an Einstein Centenary Survey , ed. S.W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1979). -
- [18][18] S.W. Hawking and G.F.R. Ellis, The Large Scale Structure of Space-Time (Cambridge University Press, Cambridge, England, 1973). -
Cited by
Sorted by citations
UNIVERSE IN A BLACK HOLE IN EINSTEIN–CARTAN GRAVITY
Popławski, N. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/832/2/96 · Cited by 91 · see citing works
Generic warp drives violate the null energy condition
Santiago, J., Schuster, S., & Visser, M. (2022) · Physical Review D · doi:10.1103/physrevd.105.064038 · Cited by 42 · see citing works
Self-citation
- Authors
- Hochberg, D., & Visser, M.
- Affiliations
- Washington University in St. Louis (US)
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1998-07-28
- Volume
- 58
- Issue
- 4
- ISSN
- 0556-2821 (ISSN-L)
- 1089-4918
- OpenAlex
- W2164003752
- Cited by
- 334
- References
- 1
- Citations by year
- 2026: 22 · 2025: 34 · 2024: 23 · 2023: 26 · 2022: 18 · 2021: 26 · 2020: 16 · 2019: 5 · 2018: 14 · 2017: 17 · 2016: 14 · 2015: 11 · 2014: 8 · 2013: 7 · 2012: 5
- FWCI
- 3.54
- 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)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Topics
- 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
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
- Keywords
- traversable wormholes, wormhole throat, null energy condition violation, flare-out condition, null geodesic congruences, energy conditions, static wormholes
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