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Violations of the Weak Energy Condition in Inflating Spacetimes
General Relativity and Quantum Cosmology · Submitted 10 Feb 1997
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We argue that many future-eternal inflating spacetimes are likely to violate the weak energy condition.
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The abstract, sentence by sentence
We argue that many future-eternal inflating spacetimes are likely to violate the weak energy condition. It is possible that such spacetimes may not enforce any of the known averaged conditions either. If this is indeed the case, it may open the door to constructing non-singular, past-eternal inflating cosmologies. Simple non-singular models are, however, unsatisfactory, and it is not clear if satisfactory models can be built that solve the problem of the initial singularity.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We argue that many future-eternal inflating spacetimes are likely to violate the weak energy condition. | result 0.70 | 0.72 | 0.81 | hedged possibility 1.00 |
| s1 | It is possible that such spacetimes may not enforce any of the known averaged conditions either. | interpretation 0.52 | 0.15 | 0.10 | hedged possibility 1.00 |
| s2 | If this is indeed the case, it may open the door to constructing non-singular, past-eternal inflating cosmologies. | interpretation 1.00 | 0.08 | 0.10 | hedged possibility 0.98 |
| s3 | Simple non-singular models are, however, unsatisfactory, and it is not clear if satisfactory models can be built that solve the problem of the initial singularity. | limitation 0.89 | 0.24 | 0.06 | asserted 0.67 |
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Original abstract
We argue that many future-eternal inflating spacetimes are likely to violate the weak energy condition. It is possible that such spacetimes may not enforce any of the known averaged conditions either. If this is indeed the case, it may open the door to constructing non-singular, past-eternal inflating cosmologies. Simple non-singular models are, however, unsatisfactory, and it is not clear if satisfactory models can be built that solve the problem of the initial singularity.
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