SUSY Dark Matter and Colliders - whepp-9
SUSY Dark Matter and Colliders - whepp-9
SUSY Dark Matter and Colliders - whepp-9
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Likelihood<br />
L ≡ p(d|m) is pdf of reproducing data d assuming<br />
mSUGRA model m (which depends on parameters).<br />
p(m|d) = p(d|m) p(m)<br />
p(d)<br />
p(m 1 |d)<br />
p(m 2 |d)<br />
= p(d|m 1)p(m 1 )<br />
p(d|m 2 )p(m 2 )<br />
Thus, you can interpret the likelihood distribution as<br />
relative probabilities if your ratio of priors is 1. Otherwise,<br />
convolute it with YOUR priors!<br />
<strong>SUSY</strong> <strong>Dark</strong> <strong>Matter</strong> <strong>and</strong> <strong>Colliders</strong><br />
B.C. Allanach – p.34/53
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