# Dark Suzy¶

http://www.darksusy.org

Then do

./configure
make

In examples/aux/ you will then find the tool flxconv. This is the tool she needs to run.

1) From the website: http://www.darksusy.org
2) Unzip the folder
3) make sure to have XCode and Fortran available on your laptop.
If you don't have a Fortran compiler (why should we?! ðŸ˜ƒ) you can download it from here for mac: download gfortran 6.3 Website(https://gcc.gnu.org/wiki/GFortranBinaries)
4)once you have that go in the darksusy folder and do:
./configure
make
To test whether the installation was successful, type
cd examples/test
./dstest
and should give you exit status zero.
5) Go in the examples/aux folder and do
make
./flxconv
again if flxconv is not exectutable, otherwise simply
./flxconv
6) the code will ask you:
Enter WIMP mass [GeV]
Annihilation in the Earth('ea') or the Sun('su'):
Annihilation channel?
Density of target detector material (g/cm^3):
Now enter STARTING fluxes: What type of flux do you have?Now enter ENDING fluxes: What type of flux do you have?Enter kind of flux:
1 = integrated above E_min and below tehta_max
2 = differential in energy and angle
Enter energy threshold:
Enter opening angle (half-aperture) in degrees:

• RESULTS ***
mneu = 10.00 GeV wh = su ch = 11 dens = 0.9200 g/cm^3
STARTING flux ENDING flux
------------- -----------
e1 = 0.00 GeV e2 = 4.00 GeV
th1 = 0.00 deg. th2 = 0.50 deg.
kind1 = 0 kind2 = 1
type1 = 31 type2 = 28
Unit: pb Unit: km^-2 yr^-1
Conversion from STARTING flux to annihilation rate (ann. s^-1):
====> Conversion factor cf2a = 4.8082842650328106E+027
Conversion from annihilation rate (ann. s^-1) to ENDING flux:
====> Conversion factor ca2f = 2.0756870847127290E-026

Conversion from STARTING flux to ENDING flux:
====> Conversion factor cf2f = 99.804935485560407