2015
DOI: 10.1007/s00220-015-2525-3
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The Dynamical Sine-Gordon Model

Abstract: We introduce the dynamical sine-Gordon equation in two space dimensions with parameter β, which is the natural dynamic associated to the usual quantum sineGordon model. It is shown that when β 2 ∈ (0, 16π 3 ) the Wick renormalised equation is well-posed. In the regime β 2 ∈ (0, 4π), the Da Prato-Debussche method [DPD02, DPD03] applies, while for3 ), the solution theory is provided via the theory of regularity structures [Hai13]. We also show that this model arises naturally from a class of 2+1-dimensional equi… Show more

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Cited by 76 publications
(156 citation statements)
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“…In the stationary and parabolic settings, analogous results were established by Lacoin, Rhodes, and Vargas [28, Theorem 3.1] and Hairer and Shen [24, Theorem 2.1]. 5 The main difference between Proposition 1.1 and the previous results in [28,24] is the dependence of the regularity on the time parameter T > 0. In particular, as T increases, the regularity of Θ N gets worse.…”
Section: 2supporting
confidence: 54%
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“…In the stationary and parabolic settings, analogous results were established by Lacoin, Rhodes, and Vargas [28, Theorem 3.1] and Hairer and Shen [24, Theorem 2.1]. 5 The main difference between Proposition 1.1 and the previous results in [28,24] is the dependence of the regularity on the time parameter T > 0. In particular, as T increases, the regularity of Θ N gets worse.…”
Section: 2supporting
confidence: 54%
“…In particular, by introducing a suitable time-dependent renormalization for the relevant imaginary multiplicative Gaussian chaos, we prove local wellposedness of SSG for any value of a parameter β 2 > 0 in the nonlinearity. This exhibits sharp contrast with the parabolic case studied by Hairer and Shen (2016) and Chandra, Hairer, and Shen (2018), where the parameter is restricted to the subcritical range: 0 < β 2 < 8π. We also present a triviality result for the unrenormalized SSG.2010 Mathematics Subject Classification.…”
contrasting
confidence: 62%
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“…From the linear theory we know that u is not expected to have better (parabolic) regularity than 1/2, so its spatial derivative is a distribution, which, in general, one cannot take the square of. The theory developed in [10] provided a robust concept of solution to equations like KPZ [9], Φ 4 3 , the parabolic Anderson model in both two [10] and three [12] dimensions, the dynamical Sine-Gordon model [14] on the torus, or such equations on the whole Euclidean space [11]. As neither the torus nor the whole space has boundaries, the spatial behaviour in these examples are 'uniform', and the only blow-up of the generalised abstract Taylor expansions-also referred to as 'modelled distributions'-that describe the solutions occur at the {t = 0} hyperplane of the initial time.…”
Section: Introductionmentioning
confidence: 99%