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2018
DOI: 10.1103/physrevd.97.126017
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GUT precursors and entwined SUSY: The phenomenology of stable nonsupersymmetric strings

Abstract: Recent work has established a method of constructing nonsupersymmetric string models that are stable, with near-vanishing one-loop dilaton tadpoles and cosmological constants. This opens up the tantalizing possibility of realizing stable string models whose low-energy limits directly resemble the Standard Model rather than one of its supersymmetric extensions. In this paper we consider the general structure of such strings and find that they share two important phenomenological properties. The first is a so-ca… Show more

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Cited by 40 publications
(21 citation statements)
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References 89 publications
(200 reference statements)
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“…This result garners non-trivial evidence for the de Sitter conjecture and for the TCC in top-down nonsupersymmetric settings. It would be interesting to further investigate additional Swampland conjectures within a non-supersymmetric context and the resulting constraints on non-supersymmetric string phenomenology [128][129][130]. Here we have pointed out possible realizations of the 'distance conjecture', identifying Kaluza-Klein states as the relevant tower of states that become massless at infinite distance in field space.…”
Section: Jhep10(2020)108mentioning
confidence: 94%
“…This result garners non-trivial evidence for the de Sitter conjecture and for the TCC in top-down nonsupersymmetric settings. It would be interesting to further investigate additional Swampland conjectures within a non-supersymmetric context and the resulting constraints on non-supersymmetric string phenomenology [128][129][130]. Here we have pointed out possible realizations of the 'distance conjecture', identifying Kaluza-Klein states as the relevant tower of states that become massless at infinite distance in field space.…”
Section: Jhep10(2020)108mentioning
confidence: 94%
“…[14] models with spontaneously broken supersymmetry and dynamical stabilization of moduli at self-dual radii in AdS vacua were already considered. 2 In our conventions, all dimensionfull quantities are expressed in string units, with α set to 1. degenerate spectra (n F = n B ), should be considered [26][27][28][29][30][31][32]. 3 Alternatively, one can deal with Friedmann-Lemaître-Robertson-Walker flat cosmological evolutions, where the supersymmetry breaking scale [33][34][35] and possibly the finite temperature of the Universe [36][37][38][39][40][41][42] are time-dependent.…”
Section: Introductionmentioning
confidence: 99%
“…This is done by developing a global geometric picture of the potential, first described in [2,3] in the case of N = 4 → N = 0 models. The general route of breaking supersymmetry at the classical level in flat space, and analyzing the induced effective potential, was advocated in Refs [4,5,6,7,8,9,10,11,12,13,14]. Moreover, the question of stability was addressed in the heterotic string framework in [6,7,15,16,17,18,19].…”
Section: Introductionmentioning
confidence: 99%