The Dark Matter Inverse Problem:
Extracting Particle Physics from Scattering Events
The central page for the Dark Matter Inverse Problem is here.
Equal Exposure Plots
Plots with all 10 GeV, 50 GeV, and 250 GeV 95% confidence level contours displayed. These events were genereated with equal exposures on all targets.
- Input data from a standard (spin- and momentum-independent) interaction:
input=std, fit=std
input=std, fit=ana
input=std, fit=dip
input=std, fit=q2
input=std, fit=q4
input=std, fit=qm2
input=std, fit=qm4
- Input data from an anapole moment (mixed standard and q^2 dependence, with additional spin coupling) interaction:
input=ana, fit=std
input=ana, fit=ana
input=ana, fit=dip
input=ana, fit=q2
input=ana, fit=q4
input=ana, fit=qm2
input=ana, fit=qm4
- Input data from a dipole moment (mixed q^2 and q^4 dependence, with additional spin coupling) interaction:
input=dip, fit=std
input=dip, fit=ana
input=dip, fit=dip
input=dip, fit=q2
input=dip, fit=q4
input=dip, fit=qm2
input=dip, fit=qm4
- Input data from a q^2 interaction:
input=q2, fit=std
input=q2, fit=ana
input=q2, fit=dip
input=q2, fit=q2
input=q2, fit=q4
input=q2, fit=qm2
input=q2, fit=qm4
- Input data from a q^-4 interaction:
input=qm4, fit=std
input=qm4, fit=ana
input=qm4, fit=dip
input=qm4, fit=q2
input=qm4, fit=q4
input=qm4, fit=qm2
input=qm4, fit=qm4