2020
DOI: 10.1007/jhep09(2020)056
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Unattainability of the trans-Planckian regime in nonlocal quantum gravity

Abstract: Based on the ultraviolet asymptotic freedom of nonlocal quantum gravity, we show that the trans-Planckian energy regime is unattainable in laboratory experiments. As physical implications, it turns out that the violation of causality, typical of nonlocal field theories, can never be detected in particle accelerators, while the asymptotic freedom of the theory provides an elegant solution to the so called trans-Planckian cosmological problem.

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Cited by 12 publications
(7 citation statements)
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“…However, the TCC also constrains models in which the period of canonical inflation is replaced by a period of k-inflation [38] or a period of superluminal sound speed [39]. The TCC also applies to holographic cosmology [40], but it is not constraining in the context of nonlocal gravity [41].…”
Section: Discussionmentioning
confidence: 99%
“…However, the TCC also constrains models in which the period of canonical inflation is replaced by a period of k-inflation [38] or a period of superluminal sound speed [39]. The TCC also applies to holographic cosmology [40], but it is not constraining in the context of nonlocal gravity [41].…”
Section: Discussionmentioning
confidence: 99%
“…A unified nonlocal theory of all fundamental interactions with the aforementioned properties of the purely gravitational theories has been recently proposed in [62,63]. In the ultraviolet regime all nonlocal gravitational theories (or local with more than ten derivatives in four dimensions) are asymptotically free [58] or finite [54,59]. Theories with a number of derivatives from six to eight are super-renormalizable but, to prove asymptotic freedom, quantitative analysis and explicit computations are needed because there are divergences also at two and/or three loops.…”
Section: Universality Of the Effective Field Theory Resultsmentioning
confidence: 99%
“…and coordinates x μ = (t, r). We assume that m M, such that we can neglect contribution of the small mass m to the potentials (57) and (58). The one-loop corrections to (61) can be obtained from (40) by the substitution T μν −→ T μν + T μν m [11], where…”
Section: The Motion Of a Test Particlementioning
confidence: 99%
“…Last but not least, we would like to stress the correctness of our result in the ultraviolet regime, regardless the linear approximation. Indeed, the asymptotic freedom of the theory [86] at short distances guarantees the stability of the potential (or the metric) under nonlinear corrections.…”
Section: Discussionmentioning
confidence: 99%