The Dark Matter Inverse Problem:
Extracting Particle Physics from Scattering Events
The central page for the Dark Matter Inverse Problem is here.
Equal Exposure Low Mass Plots
Plots with 10 and 50 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