2014
DOI: 10.48550/arxiv.1403.1277
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Decoding perturbation theory using resurgence: Stokes phenomena, new saddle points and Lefschetz thimbles

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Cited by 57 publications
(103 citation statements)
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“…Conclusions -Recent advances in applying the theory of resurgence to quantum theories [25][26][27][28][29][30] have motivated us to rethink the foundational aspects of relativistic hydrodynamics.…”
mentioning
confidence: 99%
“…Conclusions -Recent advances in applying the theory of resurgence to quantum theories [25][26][27][28][29][30] have motivated us to rethink the foundational aspects of relativistic hydrodynamics.…”
mentioning
confidence: 99%
“…There is also another type of interpolating functions[8], which is not special case of the FPR. This has been applied to O(N ) non-linear sigma model.2 Note that our interpolating function approach is different from resurgence approach, which has been recently studied in a series of works[9,10,11,12,13,14,15,16,17,18,19,20,21,22,23]. While we use single types of weak and strong coupling expansions as input data, the resurgence approach uses weak coupling expansions around multiple saddle points and does not use strong coupling expansion.…”
mentioning
confidence: 99%
“…Note that (13) has two independent solutions. The solution in (14) was picked on the grounds that there should be only ingoing wave at the horizon, z = 0. (we will elaborate on the boundary conditions in more detail when we discuss the Stokes phenomenon) This solution is to be matched with the far region solution and for this we need the asymptotic expansion of ( 14) for large r (z → 1).…”
Section: A Near Regionmentioning
confidence: 99%
“…For this, the identification dominant and subdominant solutions is essential. In quantum mechanical scattering problems, the Stokes phenomenon gives rise to the reflection phenomena [13] and also plays a key role, in somewhat different context, in the application of resurgence theory to the perturbative expansions of quantum field theories [14,15]. As we will discuss shortly, the Hawking quanta responsible for the emission is encoded by the subdominant solution in the horizon region and the appearance of such solution is in fact brought by the requirement of causality.…”
Section: Re Tmentioning
confidence: 99%