Direct Detection of Dark Matter Rates for Various Wimps

Abstract

The event rates for the direct detection of a dark matter candidate, which is a Kaluza-Klein gauge boson, are evaluated for a number of nuclear targets. Realistic form factors as well as spin ME and response functions are employed.

23 LaTex pages, 22 eps figures

References in corpus (1)

• Common Origin of Neutrino Mass, Dark Matter, and Baryogenesis

Cited by in corpus (21)

• Unifying of Inflation with Early and Late Dark Energy Epochs in Axion $F(R)$ Gravity
• Unification of Inflation with Dark Energy in $f(R)$ Gravity and Axion Dark Matter
• Geometric Inflation and Dark Energy with Axion $F(R)$ Gravity
• $f(R)$ Gravity Inflation with String-Corrected Axion Dark Matter
• Unification of a Bounce with a Viable Dark Energy Era in Gauss-Bonnet Gravity
• Dark Majorana Particles from the Minimal Walking Technicolor
• Kaluza-Klein Dark Matter: Direct Detection vis-a-vis LHC
• Can Solar Neutrinos be a Serious Background in Direct Dark Matter Searches?
• Discriminating dark matter candidates using direct detection
• Kinetic Axion $F(R)$ Gravity Inflation
• Late-Time Cosmology of Scalar-Coupled $f(R,\mathcal{G})$ Gravity
• The Classical and Loop Quantum Cosmology Phase Space of Interacting Dark Energy and Superfluid Dark Matter
• Dark Energy and Equation of State Oscillations with Collisional Matter Fluid in Exponential Modified Gravity
• Finite Temperature Casimir Effect for Massless Majorana Fermions in a Magnetic Field
• Late Time Cosmological Evolution in f(R) theories with Ordinary and Collisional Matter
• The Casimir effect for parallel plates involving massless Majorana fermions at finite temperature
• $R^2$ Gravity Effects on the Kinetic Axion Phase Space
• Kinetic Axion Dark Matter in String Corrected $f(R)$ Gravity
• The interaction of extended Bose-Einstein condensate dark matter with viscous $f(T,B)$ gravity
• Constraining Light Scalar Field with Torsion-Balance Gravity Experiments
• Cosmology in the mimetic higher-curvature $f(R,R_{\mu \nu }{R}^{\mu \nu })$ gravity