Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/111884
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dc.contributorDepartment of Applied Mathematics-
dc.creatorLiu, S-
dc.creatorHu, Y-
dc.creatorWang, X-
dc.date.accessioned2025-03-18T01:13:24Z-
dc.date.available2025-03-18T01:13:24Z-
dc.identifier.urihttp://hdl.handle.net/10397/111884-
dc.language.isoenen_US
dc.publisherInstitute of Mathematical Statisticsen_US
dc.rightsAll works in this journal are licensed under a Creative Commons Attribution 4.0 International License (https://creativecommons.org/licenses/by/4.0/).en_US
dc.rightsThe following publication Shuhui Liu. Yaozhong Hu. Xiong Wang. "In search of necessary and sufficient conditions to solve the parabolic Anderson model with fractional Gaussian noises." Electron. J. Probab. 29 1 - 48, 2024 is available at https://doi.org/10.1214/24-EJP1200.en_US
dc.subjectChaos expansionen_US
dc.subjectFractional Gaussian noiseen_US
dc.subjectHardy-Littlewood-Sobolev inequalityen_US
dc.subjectHölder-Young-Brascamp-Lieb inequalityen_US
dc.subjectNecessary and sufficient conditionen_US
dc.subjectParabolic Anderson modelen_US
dc.subjectSolvabilityen_US
dc.titleIn search of necessary and sufficient conditions to solve the parabolic Anderson model with fractional Gaussian noisesen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.spage1-
dc.identifier.epage48-
dc.identifier.volume29-
dc.identifier.doi10.1214/24-EJP1200-
dcterms.abstractThis paper attempts to obtain necessary and sufficient conditions to solve the parabolic ∂ Anderson model with fractional Gaussian noises: [Formula Presented] where W (t, x) is the fractional Brownian field with temporal Hurst parameter H0 ∈ [1/2, 1) and spatial Hurst parameters H = (H1, · · ·, Hd) ∈ (0, 1)d, and Ẇ (t, x) = [Formula Presented]. When d = 1 and when (H0, H) ∈ [Formula Presented] we show that the condition 2H0 + H > 5/2 is necessary and sufficient to ensure the existence of a unique solution for the parabolic Anderson Model. When d ≥ 2, we find the necessary and sufficient condition on the Hurst parameters so that each chaos of the solution candidate is square integrable.-
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationElectronic journal of probability, 2024, v. 29, 140, p. 1-48-
dcterms.isPartOfElectronic journal of probability-
dcterms.issued2024-
dc.identifier.scopus2-s2.0-85205272054-
dc.identifier.eissn1083-6489-
dc.identifier.artn140-
dc.description.validate202503 bcrc-
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberOA_Scopus/WOSen_US
dc.description.fundingSourceSelf-fundeden_US
dc.description.pubStatusPublisheden_US
dc.description.oaCategoryCCen_US
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