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UV completion without symmetry restoration · Around

2013

UV completion without symmetry restoration

Endlich, Solomon, Nicolis, Alberto, Penco, Riccardo

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We show that it is not possible to UV-complete certain low-energy effective theories with spontaneously broken space-time symmetries by embedding them into linear sigma models, that is, by adding "radial" modes and restoring the broken symmetries.

When such a UV completion is not possible, one can still raise the cutoff up to arbitrarily higher energies by adding fields that transform non-linearly under the broken symmetries, that is, new Goldstone bosons.
However, this (partial) UV completion does not necessarily restore any of the broken symmetries.
We illustrate this point by considering a concrete example in which a combination of space-time and internal symmetries is broken down to a diagonal subgroup.

Built on

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Then

I. McArthur, JHEP 1011
Original
2010
Later among the works it cites.
S. Endlich, A. Nicolis, R. Rattazzi, and J. Wang, JHEP 1104
Original
2011
Later among the works it cites.
A. Kapustin, (2012), arXiv:1207.0457 [hep-ph]
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2012
Later among the works it cites.
A. Nicolis and F. Piazza, Phys.Rev.Lett. 110
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2013
Closest in time.

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