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<oembed><version>1.0</version><provider_name>KMI - Nagoya University</provider_name><provider_url>https://www.kmi.nagoya-u.ac.jp/eng</provider_url><title>Deep learning for continuous gravitational waves - KMI - Nagoya University</title><type>rich</type><width>600</width><height>338</height><html>&lt;blockquote class="wp-embedded-content" data-secret="CEbRoIukyE"&gt;&lt;a href="https://www.kmi.nagoya-u.ac.jp/eng/seminar/2915/"&gt;Deep learning for continuous gravitational waves&lt;/a&gt;&lt;/blockquote&gt;&lt;iframe sandbox="allow-scripts" security="restricted" src="https://www.kmi.nagoya-u.ac.jp/eng/seminar/2915/embed/#?secret=CEbRoIukyE" width="600" height="338" title="&#x201C;Deep learning for continuous gravitational waves&#x201D; &#x2014; KMI - Nagoya University" data-secret="CEbRoIukyE" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"&gt;&lt;/iframe&gt;&lt;script type="text/javascript"&gt;
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</html><description>Since the first discovery of the binary black hole merger, the gravitational wave detectors, Advanced LIGO, Advanced Virgo, and KAGRA have provided astonishing information about our universe. Persistent, quasi-monochromatic gravitational waves, so-called continuous gravitational waves are also targets of these detectors. We expect continuous waves to bring information about various aspects of physics such as the inner structure of the neutron stars, the existence of a boson cloud around a rotating black hole, and the abundance of the sub-solar mass &hellip;</description></oembed>
