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An Introduction to Supernovae - LUTH

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● Looking in<strong>to</strong> the heart of a core collapse supernova<br />

● - through observations of neutrinos<br />

● (up <strong>to</strong> now only SN1987A)<br />

●<br />

● - through observations of gravitational waves<br />

● (not yet occured! Would provide kind of Rosetta s<strong>to</strong>ne!)<br />

●<br />

● - th ro u g h s im u la tio n s<br />

● (a lre a d y a 4 0 y e a r e ffo rt ; e x tre m e ly c o m p le x &<br />

● e x p e n s ive 6 D ra d ia tio n -h y d ro d y n a m ic s p ro b le m<br />

● re q u irin g ~1 0 21 o p e ra tio n s / s im u la tio n<br />

● o r ~1 C P U -y r @ 3 0 T e ra flo p / s im u la tio n )<br />

●<br />

●<br />

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