Research Article

Generalising Holographic Superconductors

Figure 6

Critical temperature in Kelvin for s-, p-, d-, f-, and g-wave superconductors as a function of for and all masses chosen at the respective BF bound, Equation (38). The energy density of the gauge field near the horizon has been set to so as to relate the prediction of the model with physical systems. The dashed blue vertical line emphasises the AdS Schwarzschild BH case .