Using a dataset corresponding to an integrated luminosity of 3.0 fb$^{ -1}$ collected in $pp$ collisions at centre-of-mass energies of 7 and 8 TeV, the $B_s^0 \to \phi \phi$ branching fraction is measured to be \[ \mathcal{ B}(B_s^0 \to \phi \phi) = ( 1.84 \pm 0.05 (\text{ stat}) \pm 0.07 (\text{ syst}) \pm 0.11 (f_s/f_d) \pm 0.12 (\text{ norm}) ) \times 10^{ -5}, \] where $f_s/f_d$ represents the ratio of the $B_s^0$ to $B^0$ production cross-sections, and the $B^0 \to \phi K^*(892)^0$ decay mode is used for normalization. This is the most precise measurement of this branching fraction to date, representing a factor five reduction in the statistical uncertainty compared with the previous best measurement. A search for the decay $B^0 \to \phi \phi$ is also made. No signal is observed, and an upper limit on the branching fraction is set as \[ \mathcal{ B}(B^0 \to \phi \phi) < 2.8 \times 10^{ -8} \] at 90% confidence level. This is a factor of seven improvement compared to the previous best limit.
Categories: hep-ex