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DOI: 10.17760/d20289557
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High performance algorithms for quantum gravity and cosmology

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Cited by 4 publications
(5 citation statements)
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References 134 publications
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“…Nevertheless, to get to the asymptotic regime in d = 4 will require far more extensive computational power. Recently, using new sophisticated computational techniques (Cunningham 2018b), the algorithms of Surya (2012) have been updated, so that n ∼ 300 simulations can be done in a reasonable time.…”
Section: A Continuum-inspired Dynamicsmentioning
confidence: 99%
See 1 more Smart Citation
“…Nevertheless, to get to the asymptotic regime in d = 4 will require far more extensive computational power. Recently, using new sophisticated computational techniques (Cunningham 2018b), the algorithms of Surya (2012) have been updated, so that n ∼ 300 simulations can be done in a reasonable time.…”
Section: A Continuum-inspired Dynamicsmentioning
confidence: 99%
“…( 31) in general is however non-trivial since there are caustics in a generic spacetime which complicate the calculation. On the other hand, numerical simulations suggest that again, up to boundary terms, the Benincasa-Dowker action S is the Einstein-Hilbert action (Benincasa 2013;Cunningham 2018b). We will discuss these boundary terms below.…”
Section: The Ricci Scalar and The Benincasa-dowker Actionmentioning
confidence: 99%
“…Recently, there has been a great amount of interest in applying techniques of machine learning to string theory, as pioneered in [29][30][31][32][33]. In particular, methods of machine learning have been applied to various "Big Data" problems in string compactifications, such as string vacua, the AdS/CFT correspondence, bundle cohomology and stability, cosmology and beyond, [34][35][36][37][38][39][40][41][42][43][44][45][46][47][48][49][50][51] as well as the structure of mathematics. [52][53][54][55] The idea of this present work is to apply these same methods to see whether they are able to increase the accuracy and/or reduce the time and cost of numerical calculations, specifically of the Calabi-Yau metric on generic threefolds.…”
Section: Introductionmentioning
confidence: 99%
“…in which N k (C) denotes the number of discrete spacetime order intervals containing k elements in the causal set C, and n denotes the cardinality of the causal set n = |C|. As argued by Sorkin [44], Benincasa and Dowker [46], and shown numerically by Cunningham [49] for certain restricted cases, under the assumption that the contribution to the integral from the W 2 region down the light cone vanishes, the discrete action S (4) limits (assuming zero surface terms) to the continuum Einstein-Hilbert action for the Lorentzian manifold (M, g) in the limit of infinite sprinkling density:…”
mentioning
confidence: 99%