<oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
<dc:title>The growth of the Martin kernel in a horn-shaped domain</dc:title>
<dc:creator>Dante DeBlassie</dc:creator>
<dc:subject>31C35</dc:subject><dc:subject>31C05</dc:subject><dc:subject>35C20</dc:subject><dc:subject>60J50</dc:subject><dc:subject>horn-shaped domain</dc:subject><dc:subject>Martin kernel at infinity</dc:subject><dc:subject>growth rate at infinity</dc:subject><dc:subject>small perturbations</dc:subject><dc:subject>$h$-transform</dc:subject>
<dc:description>If a horn-shaped domain in $\mathbb{R}^{d+1}$ does not open too rapidly at $\infty$, then the Martin boundary (with respect to the Laplacian) at $\infty$ is homeomorphic to the sphere $S^{d-1}$. Given a point $\varphi$ in the sphere, we determine the growth rate of the Martin kernel with pole at $\varphi$ explicitly in terms of the speed at which the horn opens at $\infty$.</dc:description>
<dc:publisher>Indiana University Mathematics Journal</dc:publisher>
<dc:date>2008</dc:date>
<dc:type>text</dc:type>
<dc:format>pdf</dc:format>
<dc:identifier>10.1512/iumj.2008.57.3392</dc:identifier>
<dc:source>10.1512/iumj.2008.57.3392</dc:source>
<dc:language>en</dc:language>
<dc:relation>Indiana Univ. Math. J. 57 (2008) 3115 - 3130</dc:relation>
<dc:coverage>state-of-the-art mathematics</dc:coverage>
<dc:rights>http://iumj.org/access/</dc:rights>
</oai_dc:dc>