An Introduction to Supernovae - LUTH
An Introduction to Supernovae - LUTH
An Introduction to Supernovae - LUTH
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Einstein quadrupole formula<br />
(valid for slow motion v«c and weak fields « c 2 )<br />
h jk= 2G<br />
c 4<br />
R s =1 km , v/c=0.1 , R=10kpc ---> h ~ 10 -20<br />
GW luminosity<br />
L GW= d E GW<br />
dt<br />
1<br />
R ¨Q jk ~ R s<br />
R v<br />
c 2<br />
= 1<br />
5<br />
G<br />
c 5 〈 Q jk 2<br />
〉 ~ R S<br />
R 2<br />
v<br />
c 6<br />
¨Q~MR 2 /T 2 ~Mv 2
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