Well, maybe it's a language problem. I will give it one more try.
When I say please post your problem I mean, please describe the system you are trying to solve. What material is between your source and detector? Are you doing a source calculation or a kcode calculation? That sort of thing. Just saying your stats are bad does not let me help you. I need to know about the system you want to analyze.
You have now posted some vague hints. It seems like you have an x-ray source and some detectors.
For MCNP 6.2, the user manual section 3.3.6 is where you want to start reading.
When you have a source there are a couple reasons the stats may be bad.
One is simple geometry. As you get farther from the source many of the particles go somewhere besides the detector. You can deal with this through a variety of biasing methods. You make your source point in the direction of the detector. Then you adjust the normalizing of the detector to account for the biasing. For example, a spherical source could be adjusted to only send particles in a tiny cone. Then you adjust for the relative area of the cone versus the full sphere.
Another method for geometry is the DXTRAN sphere. Before you use this one you should read the manual VERY carefully. You can get misleading results very easily if you do things wrong.
There are also a variety of detector tallies that are semi-deterministic. Again, you need to read the manual on these VERY carefully.
Another reason you may be getting bad stats is shielding. If there is a lot of material between your source and detector then nearly all the particles get absorbed before they get to your detector. There are a bunch of things you can do in that case. The simplest is adjusting the importance of various parts of the system. The goal is to have the number of particles at your detector be larger. There are several methods with additional levels of sophistication, but also additional effort required.
In very broad outline, importance adjusting goes like so. Consider a source, shielding material, and a detector on the other side.
source | shielding | shielding| shielding| shielding| detector
By the time particles get through there are very few left. Most get absorbed. The basic idea is you set the importance higher and higher as you get closer to the detector.
source | shielding | shielding| shielding| shielding| detector
imp:1 imp:1 imp:2 imp:4 imp:8 imp:16
The idea is, when importance changes from 1 to 2, the code will change one particle of weight 1 to two particles of weight 1/2. The ideal is to keep the number of particles roughly constant across each layer. That way you can get good stats at the detector.
For simple systems you can apply this by hand. For more complicated systems there are some automated utilities in MCNP. They are fairly complicated and require a lot of careful reading of the user manual.