Estimation of Critical Collapse Solutions to Black Holes with Nonlinear Statistical Models

The self-similar gravitational collapse solutions to the Einstein-axion–dilaton system have already been discovered. Those solutions become invariants after combining the spacetime dilation with the transformations of internal <i>SL</i>(2, <i>R</i>). We apply nonlinear statis...

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Main Authors: Ehsan Hatefi, Armin Hatefi
Format: Article
Language:English
Published: MDPI AG 2022-11-01
Series:Mathematics
Subjects:
Online Access:https://www.mdpi.com/2227-7390/10/23/4537
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author Ehsan Hatefi
Armin Hatefi
author_facet Ehsan Hatefi
Armin Hatefi
author_sort Ehsan Hatefi
collection DOAJ
description The self-similar gravitational collapse solutions to the Einstein-axion–dilaton system have already been discovered. Those solutions become invariants after combining the spacetime dilation with the transformations of internal <i>SL</i>(2, <i>R</i>). We apply nonlinear statistical models to estimate the functions that appear in the physics of Black Holes of the axion–dilaton system in four dimensions. These statistical models include parametric polynomial regression, nonparametric kernel regression and semi-parametric local polynomial regression models. Through various numerical studies, we reached accurate numerical and closed-form continuously differentiable estimates for the functions appearing in the metric and equations of motion.
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spelling doaj.art-1907d2b4bb884c1e8c0de5806029f8782023-11-24T11:35:13ZengMDPI AGMathematics2227-73902022-11-011023453710.3390/math10234537Estimation of Critical Collapse Solutions to Black Holes with Nonlinear Statistical ModelsEhsan Hatefi0Armin Hatefi1GRAM Research Group, Department of Signal Theory and Communications, University of Alcala, 28805 Alcala de Henares, SpainDepartment of Mathematics and Statistics, Memorial University of Newfoundland, St. John’s, NL A1C 5S7, CanadaThe self-similar gravitational collapse solutions to the Einstein-axion–dilaton system have already been discovered. Those solutions become invariants after combining the spacetime dilation with the transformations of internal <i>SL</i>(2, <i>R</i>). We apply nonlinear statistical models to estimate the functions that appear in the physics of Black Holes of the axion–dilaton system in four dimensions. These statistical models include parametric polynomial regression, nonparametric kernel regression and semi-parametric local polynomial regression models. Through various numerical studies, we reached accurate numerical and closed-form continuously differentiable estimates for the functions appearing in the metric and equations of motion.https://www.mdpi.com/2227-7390/10/23/4537mathematical physicsblack holesstatistical analysis
spellingShingle Ehsan Hatefi
Armin Hatefi
Estimation of Critical Collapse Solutions to Black Holes with Nonlinear Statistical Models
Mathematics
mathematical physics
black holes
statistical analysis
title Estimation of Critical Collapse Solutions to Black Holes with Nonlinear Statistical Models
title_full Estimation of Critical Collapse Solutions to Black Holes with Nonlinear Statistical Models
title_fullStr Estimation of Critical Collapse Solutions to Black Holes with Nonlinear Statistical Models
title_full_unstemmed Estimation of Critical Collapse Solutions to Black Holes with Nonlinear Statistical Models
title_short Estimation of Critical Collapse Solutions to Black Holes with Nonlinear Statistical Models
title_sort estimation of critical collapse solutions to black holes with nonlinear statistical models
topic mathematical physics
black holes
statistical analysis
url https://www.mdpi.com/2227-7390/10/23/4537
work_keys_str_mv AT ehsanhatefi estimationofcriticalcollapsesolutionstoblackholeswithnonlinearstatisticalmodels
AT arminhatefi estimationofcriticalcollapsesolutionstoblackholeswithnonlinearstatisticalmodels