• • • We do not use the following data for averages, fits, limits, etc. • • • |
$<1.2 \times 10^{-11}$ |
95 |
1 |
|
SPEC |
$<6.9 \times 10^{-10}$ |
95 |
1 |
|
SPEC |
$<1 \times 10^{-11}$ |
95 |
2 |
|
SPEC |
$<1 \times 10^{-8}$ |
95 |
2 |
|
SPEC |
$<6 \times 10^{-9}$ |
95 |
2 |
|
SPEC |
$<1 \times 10^{-8}$ |
95 |
2 |
|
SPEC |
$<4 \times 10^{-20}$ |
90 |
3 |
|
SPEC |
$<8 \times 10^{-20}$ |
90 |
3 |
|
SPEC |
$<2 \times 10^{-16}$ |
90 |
3 |
|
SPEC |
$<6 \times 10^{-13}$ |
90 |
3 |
|
SPEC |
$<1 \times 10^{-11}$ |
90 |
3 |
|
SPEC |
$<6 \times 10^{-14}$ |
90 |
3 |
|
SPEC |
$<4 \times 10^{-17}$ |
90 |
3 |
|
SPEC |
$<4 \times 10^{-15}$ |
90 |
3 |
|
SPEC |
$<1.5 \times 10^{-13}/\text{nucleon }$ |
68 |
4 |
|
SPEC |
$<1.2 \times 10^{-12}/\text{nucleon }$ |
68 |
4 |
|
SPEC |
1
JAVORSEK 2001 search for (neutral) SIMPs (strongly interacting massive particles) bound to Au nuclei. Here $\mathit M$ is the effective SIMP mass.
|
2
JAVORSEK 2001B search for (neutral) SIMPs (strongly interacting massive particles) bound to Au and Fe nuclei from various origins with exposures on the earth's surface, in a satellite, heavy ion collisions, etc. Here $\mathit M$ is the mass of the anomalous nucleus. See also JAVORSEK 2002 .
|
3
See HEMMICK 1990 Fig.$~$7 for other masses $100 - 10000~{\mathit m}_{{{\mathit p}}}$.
|
4
Bound valid up to ${\mathit m}_{{{\mathit X}^{-}}}$ $\sim{}$ 100 TeV.
|