We investigate the critical properties and phase structure of excited states in a holographic superconductor model within the framework of Varying Central Charge Thermodynamics, where the cosmological constant serves as a fundamental parameter controlling the number of degrees of freedom in the boundary conformal field theory. Employing Born-Infeld nonlinear electrodynamics, we explore how the nonlinear parameter affects the condensation of the ground state (GS) and the two lowest excited states (ES1, ES2) in the background of a spherically symmetric Schwarzschild-AdS black hole. A state is classified as possessing a if its optical conductivity exhibits for , indicating a hard energy gap in the excitation spectrum and the Meissner effect. In contrast, a possesses a non-zero order parameter but lacks a hard gap, with as . Our central finding reveals that the emergence of gapless phases in the excited states represents a genuine physical phenomenon arising from the competition between Born-Infeld nonlinear screening effects and the spatial curvature of the black hole geometry, not from numerical artifacts. Specifically, when the pressure exceeds the critical pressure , both GS and ES1 are gapped superconductors with hard energy gaps while ES2 is a gapless superconductor. However, when , only GS remains gapped while both ES1 and ES2 condense into gapless phases. This curvature-controlled switching of superconducting properties provides a novel mechanism for engineering gapless superconductivity in strongly coupled systems through variation of the boundary CFT degrees of freedom, with potential implications for understanding unconventional high-temperature superconductors.

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