The weak-gravity bound and the need for spin in asymptotically safe matter-gravity models
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Abstract We discover a weak-gravity bound in scalar-gravity systems in the asymptotic-safety paradigm. The weak-gravity bound arises in these systems under the approximations we make, when gravitational fluctuations exceed a critical strength. Beyond this critical strength, gravitational fluctuations can generate complex fixed-point values in higher-order scalar interactions. Asymptotic safety can thus only be realized at sufficiently weak gravitational interactions. We find that within truncations of the matter-gravity dynamics, the fixed point lies beyond the critical strength, unless spinning matter, i.e., fermions and vectors, is also included in the model.
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2009 ◽
Vol 24
(28)
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pp. 2233-2241
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2021 ◽
2017 ◽
Vol 668
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pp. 27-42
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2017 ◽
Vol 32
(08)
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pp. 1750048
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2015 ◽
Vol 60
(12)
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pp. 1658-1667
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2015 ◽
Vol 191
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pp. 18-32
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