Specific heat in the superconducting and normal state (2-300 K, 0-16 T), and magnetic susceptibility of the 38 K superconductor MgB2: evidence for a multicomponent gap
Yx. Wang et al., Specific heat in the superconducting and normal state (2-300 K, 0-16 T), and magnetic susceptibility of the 38 K superconductor MgB2: evidence for a multicomponent gap, PHYSICA C, 355(3-4), 2001, pp. 179-193
The specific heat C of a sintered polycrystalline sample of MgB2 with a bul
k superconducting transition temperature T-c = 36.7 K is measured as a func
tion of the temperature (2-300 K) and magnetic field (0-16 T), together wit
h magnetic properties (normal-state susceptibility, superconducting-state m
agnetization, etc.). The Sommerfeld constant gamma = 0.89 +/- 0.05 mJ/K-2/g
at (2.7 mJ/K-2/mol) is determined in the normal state above H-c2 The normal
- and superconducting-state entropies are equal at T,. Several moments of t
he PDOS are obtained from the lattice specific heat. We report bulk values
for: the thermodynamic critical field, B-c(0) = 0.26 T; the slope of the up
per critical field, (dB(c2)/ dT)(Tc) = 0.56 T/K; the Ginzburg-Landau parame
ter, kappa = 38; the coherence length, xi approximate to 5 nm; the lower cr
itical field, B-c1 approximate to 0.018 T; the London penetration depth, la
mbda (0) approximate to 180 nm. These results characterize MgB2 as a type-I
I superconductor. The nearly quadratic dependence of C(T) versus T at T muc
h less than T-c, its non-linear field dependence, and the discrepancy betwe
en the electron-phonon coupling constant lambda (ep) as determined by the r
enormalization of the electron density of states (lambda (ep) approximate t
o 0.6) and by McMillan's equation for isotropic superconductors (lambda (ep
) approximate to 1.1), are inconsistent with a single isotropic gap. In add
ition to high phonon frequencies, anisotropy or two-band gap structure may
explain why the critical temperature of this superconductor is high in spit
e of its low condensation energy, which does not exceed 1/16 of that of YBa
2Cu3O7 and 1/4 of that of Nb3Sn. (C) 2001 Elsevier Science B.V. All rights
reserved.