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Very low truncation dimension for high dimensional integration under modest error demand
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We consider the problem of numerical integration for weighted anchored and ANOVA Sobolev spaces of g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si1.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=f8618a50cace5423b26b8044d1ac1cfd" title="Click to view the MathML source">s-variate functions. Here g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si1.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=f8618a50cace5423b26b8044d1ac1cfd" title="Click to view the MathML source">s is large including g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si3.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=fe1007b6cb91368e68ac8c5817f0a16c" title="Click to view the MathML source">s=∞. Under the assumption of sufficiently fast decaying weights, we prove in a constructive way that such integrals can be approximated by quadratures for functions g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si4.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=74f997ec196e4bffb4cc200252a27eb5" title="Click to view the MathML source">fk with only g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si5.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=0d18c77bf1d6916d5f6650c63cfa5de9" title="Click to view the MathML source">k variables, where g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si6.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=e9bcf60e2e8824b8539abdbe56bf616d" title="Click to view the MathML source">k=k(ε) depends solely on the error demand g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si7.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=d5ae9824da807af628cd73689491f95f" title="Click to view the MathML source">ε and is surprisingly small when g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si1.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=f8618a50cace5423b26b8044d1ac1cfd" title="Click to view the MathML source">s is sufficiently large relative to g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si7.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=d5ae9824da807af628cd73689491f95f" title="Click to view the MathML source">ε. This holds, in particular, for g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si3.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=fe1007b6cb91368e68ac8c5817f0a16c" title="Click to view the MathML source">s=∞ and arbitrary g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si7.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=d5ae9824da807af628cd73689491f95f" title="Click to view the MathML source">ε since then g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si12.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=0af0a5c9f670f88d332601cc6730be3f" title="Click to view the MathML source">k(ε)<∞ for all g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si7.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=d5ae9824da807af628cd73689491f95f" title="Click to view the MathML source">ε. Moreover g" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0885064X16000145&_mathId=si14.gif&_user=111111111&_pii=S0885064X16000145&_rdoc=1&_issn=0885064X&md5=829cabb3b9f2a48fe0280acc8c76aa8b" title="Click to view the MathML source">k(ε) does not depend on the function being integrated, i.e., is the same for all functions from the unit ball of the space.

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