<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>On the energy behavior of locally self-similar blowup for the Euler equation</dc:title>
<dc:creator>Anne Bronzi</dc:creator><dc:creator>Roman Shvydkoy</dc:creator>
<dc:subject>Primary:76B03</dc:subject><dc:subject>Secondary:35Q31</dc:subject><dc:subject>Euler equation</dc:subject><dc:subject>self-similar solutions</dc:subject>
<dc:description>In this note, we study locally self-similar blowup for the Euler equation. The main result states that under a mild $L^p$-growth assumption on the profile $v$, namely $\displaystyle\int_{|y|\sim L}|v|^p\,\mathrm{d}y\lesssim L^{\gamma}$ for some $\gamma&lt;p-2$, the self-similar solution carries a positive amount of energy up to the time of blowup $T$, namely, $\displaystyle\int_{|y|\sim L}|v|^2\,\mathrm{d}y\sim L^{N-2\alpha}$. The result implies and extends several previously known exclusion criteria. It also supports a general conjecture relating fractal local dimensions of the energy measure with the rate of velocity growth at the time of possible blowup.</dc:description>
<dc:publisher>Indiana University Mathematics Journal</dc:publisher>
<dc:date>2015</dc:date>
<dc:type>text</dc:type>
<dc:format>pdf</dc:format>
<dc:identifier>10.1512/iumj.2015.64.5657</dc:identifier>
<dc:source>10.1512/iumj.2015.64.5657</dc:source>
<dc:language>en</dc:language>
<dc:relation>Indiana Univ. Math. J. 64 (2015) 1291 - 1302</dc:relation>
<dc:coverage>state-of-the-art mathematics</dc:coverage>
<dc:rights>http://iumj.org/access/</dc:rights>
</oai_dc:dc>