Some sharp bounds for Steklov eigenvalues
This work is an extension of a result given by Kuttler and Sigillito (SIAM Rev $10$:$368-370$, $1968$) on a star-shaped bounded domain in $\mathbb{R}^2$. Let $\Omega$ be a star-shaped bounded domain in a hypersurface of revolution, having smooth boundary. In this article, we obtain a sharp lower bou...
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creator | Verma, Sheela Santhanam, G |
description | This work is an extension of a result given by Kuttler and Sigillito (SIAM
Rev $10$:$368-370$, $1968$) on a star-shaped bounded domain in $\mathbb{R}^2$.
Let $\Omega$ be a star-shaped bounded domain in a hypersurface of revolution,
having smooth boundary. In this article, we obtain a sharp lower bound for all
Steklov eigenvalues on $\Omega$ in terms of the Steklov eigenvalues of the
largest geodesic ball contained in $\Omega$ with the same center as $\Omega$.
We also obtain similar bounds for all Steklov eigenvalues on star-shaped
bounded domain in paraboloid, $P = \left\lbrace (x, y, z) \in \mathbb{R}^{3} :
z = x^2 + y^2\right\rbrace$. |
doi_str_mv | 10.48550/arxiv.1901.00133 |
format | Article |
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Rev $10$:$368-370$, $1968$) on a star-shaped bounded domain in $\mathbb{R}^2$.
Let $\Omega$ be a star-shaped bounded domain in a hypersurface of revolution,
having smooth boundary. In this article, we obtain a sharp lower bound for all
Steklov eigenvalues on $\Omega$ in terms of the Steklov eigenvalues of the
largest geodesic ball contained in $\Omega$ with the same center as $\Omega$.
We also obtain similar bounds for all Steklov eigenvalues on star-shaped
bounded domain in paraboloid, $P = \left\lbrace (x, y, z) \in \mathbb{R}^{3} :
z = x^2 + y^2\right\rbrace$.</description><identifier>DOI: 10.48550/arxiv.1901.00133</identifier><language>eng</language><subject>Mathematics - Differential Geometry</subject><creationdate>2019-01</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/1901.00133$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.1901.00133$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Verma, Sheela</creatorcontrib><creatorcontrib>Santhanam, G</creatorcontrib><title>Some sharp bounds for Steklov eigenvalues</title><description>This work is an extension of a result given by Kuttler and Sigillito (SIAM
Rev $10$:$368-370$, $1968$) on a star-shaped bounded domain in $\mathbb{R}^2$.
Let $\Omega$ be a star-shaped bounded domain in a hypersurface of revolution,
having smooth boundary. In this article, we obtain a sharp lower bound for all
Steklov eigenvalues on $\Omega$ in terms of the Steklov eigenvalues of the
largest geodesic ball contained in $\Omega$ with the same center as $\Omega$.
We also obtain similar bounds for all Steklov eigenvalues on star-shaped
bounded domain in paraboloid, $P = \left\lbrace (x, y, z) \in \mathbb{R}^{3} :
z = x^2 + y^2\right\rbrace$.</description><subject>Mathematics - Differential Geometry</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotzruOwjAQhWE3FCvgAbbCLUXCOGM7mRIhWJCQKKCPDBlDRCDIgQjefrlVR_qLo0-IXwWxzoyBkQv3so0VgYoBFOKPGK7rE8vm4MJFbuvbuWikr4NcX_lY1a3kcs_n1lU3bnqi413VcP-7XbGZTTeTebRc_S0m42XkbIqRItTesSlswTb1RBo4JWbiZ2fwmcmg8KQ0OoN2hzsyJkmIsq1GBrDYFYPP7duaX0J5cuGRv8z524z_IfA61Q</recordid><startdate>20190101</startdate><enddate>20190101</enddate><creator>Verma, Sheela</creator><creator>Santhanam, G</creator><scope>AKZ</scope><scope>GOX</scope></search><sort><creationdate>20190101</creationdate><title>Some sharp bounds for Steklov eigenvalues</title><author>Verma, Sheela ; Santhanam, G</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a673-1934fae5d6de67f9940e79ee9e34fe0f8580df9143a536c3c95522998b43e0063</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Mathematics - Differential Geometry</topic><toplevel>online_resources</toplevel><creatorcontrib>Verma, Sheela</creatorcontrib><creatorcontrib>Santhanam, G</creatorcontrib><collection>arXiv Mathematics</collection><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Verma, Sheela</au><au>Santhanam, G</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Some sharp bounds for Steklov eigenvalues</atitle><date>2019-01-01</date><risdate>2019</risdate><abstract>This work is an extension of a result given by Kuttler and Sigillito (SIAM
Rev $10$:$368-370$, $1968$) on a star-shaped bounded domain in $\mathbb{R}^2$.
Let $\Omega$ be a star-shaped bounded domain in a hypersurface of revolution,
having smooth boundary. In this article, we obtain a sharp lower bound for all
Steklov eigenvalues on $\Omega$ in terms of the Steklov eigenvalues of the
largest geodesic ball contained in $\Omega$ with the same center as $\Omega$.
We also obtain similar bounds for all Steklov eigenvalues on star-shaped
bounded domain in paraboloid, $P = \left\lbrace (x, y, z) \in \mathbb{R}^{3} :
z = x^2 + y^2\right\rbrace$.</abstract><doi>10.48550/arxiv.1901.00133</doi><oa>free_for_read</oa></addata></record> |
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subjects | Mathematics - Differential Geometry |
title | Some sharp bounds for Steklov eigenvalues |
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