• • • We do not use the following data for averages, fits, limits, etc. • • • |
$>3.5 \times 10^{-4}$ |
95 |
1 |
|
ATLS |
$>3 \times 10^{-4}$ |
95 |
1 |
|
ATLS |
$>2 \times 10^{-4}$ |
95 |
1 |
|
ATLS |
$>1.09 \times 10^{-5}$ |
95 |
2 |
|
DLPH |
$>1.35 \times 10^{-5}$ |
95 |
3 |
|
L3 |
$>1.3 \times 10^{-5}$ |
|
4 |
|
ALEP |
$>11.7 \times 10^{-6}$ |
95 |
5 |
|
CDF |
$>8.7 \times 10^{-6}$ |
95 |
6 |
|
OPAL |
1
AAD 2015BH searched in 20.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for associated production of a light gravitino and a squark or gluino. The squark (gluino) is assumed to decay exclusively to a quark (gluon) and a gravitino. No evidence was found for an excess above the expected level of Standard Model background and 95$\%$ C.L. lower limits were set on the gravitino mass as a function of the squark/gluino mass, both in the case of degenerate and non-degenerate squark/gluino masses, see Figs. 14 and 15.
|
2
ABDALLAH 2005B use data from $\sqrt {s }$ = $180 - 208$~GeV. They look for events with a single photon + $\not E$ final states from which a cross section limit of $\sigma $ $<$ 0.18~$\mathit pb$ at 208~GeV is obtained, allowing a limit on the mass to be set. Supersedes the results of ABREU 2000Z.
|
3
ACHARD 2004E use data from $\sqrt {s }$ = $189 - 209$~GeV. They look for events with a single photon + $\not E$ final states from which a limit on the Gravitino mass is set corresponding to $\sqrt {F }$ $>$ 238~GeV. Supersedes the results of ACCIARRI 1999R.
|
4
HEISTER 2003C use the data from $\sqrt {s }$ = $189 - 209$ GeV to search for ${{\mathit \gamma}}\not E_T$ final states.
|
5
ACOSTA 2002H looked in 87 $\mathit pb{}^{-1}$ of ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$=1.8 TeV for events with a high-$\mathit E_{T}$ photon and $\not E_T$. They compared the data with a GMSB model where the final state could arise from ${{\mathit q}}$ ${{\overline{\mathit q}}}$ $\rightarrow$ ${{\widetilde{\mathit G}}}{{\widetilde{\mathit G}}}{{\mathit \gamma}}$ . Since the cross section for this process scales as 1/$\vert \mathit F$ $\vert {}^{4}$, a limit at 95$\%$ CL is derived on $\vert \mathit F$ $\vert {}^{1/2}$ $>$ 221 GeV. A model independent limit for the above topology is also given in the paper.
|
6
ABBIENDI,G 2000D searches for ${{\mathit \gamma}}\not E$ final states from $\sqrt {\mathit s }$=189 GeV.
|