| 8 |
|
corresponding to an integrated luminosity of \lumi. |
| 9 |
|
|
| 10 |
|
The production of Z bosons is expected in many BSM scenarios, for example supersymmetric (SUSY) |
| 11 |
< |
models. For example, Z bosons may be produced in the decays $\chi^0_2\to Z \chi^0_1$ |
| 12 |
< |
$\chi^0_1\to Z \tilde{G}$, where $\chi^0_2$ is the second lightest neutralino, $\chi^0_1$ is |
| 13 |
< |
the lightest neutralino, and $\tilde{G}$ is the gravitino. Such decays may occur in the cascade |
| 11 |
> |
models. In SUSY models with neutralino lightest SUSY particle (LSP), Z bosons may be produced in the decays $\chi^0_2\to Z \chi^0_1$, |
| 12 |
> |
where $\chi^0_2$ is the second lightest neutralino and $\chi^0_1$ is |
| 13 |
> |
the lightest neutralino. |
| 14 |
> |
In models with gravitino LSP such as gauge-mediated SUSY breaking (GMSB) models, Z bosons may be produced via |
| 15 |
> |
$\chi^0_1\to Z \tilde{G}$, where $\tilde{G}$ is the gravitino. Such decays may occur either in the cascade |
| 16 |
|
decays of the strongly-produced squarks and gluinos, or via direct production of the electroweak |
| 17 |
|
charginos and neutralino. Examples of such processes (see Fig.~\ref{fig:diagrams}) are: |
| 18 |
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|
