Euclidean Q-balls of fluctuating SDW/CDW in the 'nested' Hubbard model of high-T$_c$ superconductors as the origin of pseudogap and superconducting behavior
Sergei I. Mukhin
Abstract
Euclidean Q-ball type solutions carrying Cooper/local-pair condensates inside finite volume with classically oscillating in Matsubara time spin-/charge densities (SDW/CDW) are found in the 'nested' repulsive Hubbard model of high-T$_c$ superconductors. An exchange between fermions with coherently oscillating SDW/CDW inside the Q-balls provides `pairing glue', that couples fermions into Cooper/local-pairs. Euclidean Q-ball solutions arise below some temperature $T^{*}$ due to global invariance of the effective theory under the phase rotation of the SDW/CDW fluctuations amplitudes, that conserves a 'Noether charge' Q along the Matsubara time axis. At $T^{*}$ the classical SDW/CDW fluctuations arise via 1$^{st}$ order phase transition, while superconducting condensate density inside Q-balls is zero at $T^{*}$ and possesses a steep maximum at $T<T^{*}$, causing a similar maximum in specific heat of the Q-balls 'gas'. Below $T^{*}$ the volume of the Q-balls is inversely proportional to the square of SDW/CDW fluctuation amplitude. The fermionic spectral gap inside Euclidean Q-balls arises in the vicinity of the 'nested' regions of the bare Fermi surface and scales with the square root of the superconducting density. All the described solutions are found analytically from the Eliashberg like equations for the two cases of 'nesting' wave vectors: a CDW wave vector $Q_{CDW}$, connecting regions near the Fermi surface with equal signs of the superconducting order parameter, or for a SDW wave vector $Q_{SDW}$, connecting regions with the opposite signs of the $d$-wave superconducting order parameter. Possible relation of the presented theory with thermodynamic time-crystals and different properties of superconductors is discussed.