-
Even at this maximal rate if a solar type star were to accrete in Hubble
time a solar mass of dark matter, we need that the DM density in its neighborhood will
be 109
times larger than the local ha…
-
For our application (neutron scattering) we frequently deal with axis-arrays that have more than one dimension. To my understanding this mainly occurs when one of the dimensions is not a continuous va…
-
![qmy](https://f.cloud.github.com/assets/3853527/262058/f98468ae-8d12-11e2-93dd-94d7445324d5.png)
“/dd/Materials/...”,不应该找得到吧?貌似输出的信息也没有。。。
-
-
This is a follow up of #103 presented by @chlavell, and might be of interest to @ameliajo.
I tried to recreate the evaluation for solid methane in ENDF/B-VIII.0 using a current version of NJOY an…
-
wxmacmolplt fails to open the main window, then crashes. I am using wxmacmolplt-7.7.2-1.fc35.x86_64 with xfce as the desktop environment.
The crash states that
----------------------------------…
-
-
This is related to the issue of "differential cross sections", but loosely speaking (ignoring non-isotropic materials for now) one of the two variables (E,mu) is sampled and the other is used as a dif…
-
I would like to propose that the scope of the data that SasView supports be expanded to include Dynamic Light Scattering data; specifically, intensity autocorrelation functions, g2(tau). In essence th…
-
[neutron diffraction](http://purl.org/pan-science/PaNET/PaNET01217) and [neutron single crystal diffraction](
http://purl.org/pan-science/PaNET/PaNET01236) are both direct subclasses of [neutron prob…