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Superfluid Density, Penetration Depth, Condensate Density

Warren E. Pickett

TL;DR

The paper addresses how to meaningfully define and relate three interconnected quantities in superconductors—the unitless superfluid density $\rho_s$, the penetration-depth-based response, and the scalar condensate density ${\cal N}_s$—by tracing their historical development from London to GL to BCS formalisms. It emphasizes that, in conventional superconductors, the penetration depth is governed by band-structure properties via the Drude plasma frequency and $N(0)$, with $\frac{c^2}{\lambda^2_{band}(0)}=\Omega_p^2=4\pi e^2 N(0) v_F^2$, while the true superfluid density $\rho_s$ tracks the temperature dependence of $\lambda$ and thus the gap. The work introduces and quantifies the condensate density ${\cal N}_s$ as the density of superconducting electrons, deriving its zero-temperature relation ${\cal N}^{BCS}_s(0) \approx N(0)\Delta_0$ and linking its thermodynamics to the energy gain of pairing via $\delta {\cal G}(T)$. It further discusses how optical sum rules and far-IR spectroscopy separate normal and condensate contributions, illustrating how $\Omega_p^*$ and the fractions $w_n(T)$, $w_s(T)$ describe spectral weight transfer in the superconducting state. The findings provide a framework for comparing conventional and exotic superconductors, clarifying when band-structure parameters set the scale for $\lambda$ and $n_s$, and offering a path to interpret the observed $T_c$–$\rho_s$ correlations in cuprates and related materials.

Abstract

Fascination with the concept of superconducting (SC) {\it superfluid density} $ρ_s$ has persisted since the beginning of superconductivity theory, with numerical values of an actual density rarely provided. Over time $ρ_s$, addressed mostly in cuprate and following high temperature superconductors, has become synonymous with the normalized (unitless) inverse square of the magnetic penetration depth $λ_L$ (the London expression, with superfluid density denoted $n_s$), with interest primarily on its temperature $T$ dependence that is expected to reflect the T-dependence of the SC gap amplitude and gap symmetry. In conventional superconductors, generalized expressions from the London penetration depth via Ginzburg-Landau theory, then to BCS theory provide updated pictures of the supercurrent density-vector potential relationship. The BCS value $λ_{band}$ is distinct from any particle density, instead involving particle availability at the Fermi surface and Fermi velocity as the determining factors, thus providing a basis for a more fundamental theory and understanding of what is being probed in penetration depth studies. The number density of superconducting electrons ${\cal N}_s(T$=0) -- the scalar SC {\it condensate density} -- is provided, first from a phenomenological estimate but then supported by BCS theory. A straightforward relation connecting ${\cal N}_s(0)$ to the density of dynamically transporting carriers in the normal state at $T_c$ is obtained. Numerical values of relevant material parameters including $λ_{band}$ and ${\cal N}_s$ are provided for a few conventional SCs.

Superfluid Density, Penetration Depth, Condensate Density

TL;DR

The paper addresses how to meaningfully define and relate three interconnected quantities in superconductors—the unitless superfluid density , the penetration-depth-based response, and the scalar condensate density —by tracing their historical development from London to GL to BCS formalisms. It emphasizes that, in conventional superconductors, the penetration depth is governed by band-structure properties via the Drude plasma frequency and , with , while the true superfluid density tracks the temperature dependence of and thus the gap. The work introduces and quantifies the condensate density as the density of superconducting electrons, deriving its zero-temperature relation and linking its thermodynamics to the energy gain of pairing via . It further discusses how optical sum rules and far-IR spectroscopy separate normal and condensate contributions, illustrating how and the fractions , describe spectral weight transfer in the superconducting state. The findings provide a framework for comparing conventional and exotic superconductors, clarifying when band-structure parameters set the scale for and , and offering a path to interpret the observed correlations in cuprates and related materials.

Abstract

Fascination with the concept of superconducting (SC) {\it superfluid density} has persisted since the beginning of superconductivity theory, with numerical values of an actual density rarely provided. Over time , addressed mostly in cuprate and following high temperature superconductors, has become synonymous with the normalized (unitless) inverse square of the magnetic penetration depth (the London expression, with superfluid density denoted ), with interest primarily on its temperature dependence that is expected to reflect the T-dependence of the SC gap amplitude and gap symmetry. In conventional superconductors, generalized expressions from the London penetration depth via Ginzburg-Landau theory, then to BCS theory provide updated pictures of the supercurrent density-vector potential relationship. The BCS value is distinct from any particle density, instead involving particle availability at the Fermi surface and Fermi velocity as the determining factors, thus providing a basis for a more fundamental theory and understanding of what is being probed in penetration depth studies. The number density of superconducting electrons =0) -- the scalar SC {\it condensate density} -- is provided, first from a phenomenological estimate but then supported by BCS theory. A straightforward relation connecting to the density of dynamically transporting carriers in the normal state at is obtained. Numerical values of relevant material parameters including and are provided for a few conventional SCs.
Paper Structure (19 sections, 29 equations, 1 table)