F. Mila et K. Penc, SPECTRAL-FUNCTION AND SELF-ENERGY OF THE ONE-DIMENSIONAL HUBBARD-MODEL IN THE U-]INFINITY LIMIT, Zeitschrift fur Physik. B, Condensed matter, 103(2), 1997, pp. 201-203
The interpretation of the k dependent spectral functions of the one-di
mensional, infinite U Hubbard model obtained by using the factorized w
ave-function of Ogata and Shiba is revisited. The well defined feature
which appears in addition to low energy features typical of Luttinger
liquids, and which, close to the Fermi energy, dan be interpreted as
the shadow band resulting from 2k(F) spin fluctuations, is further inv
estigated. A calculation of the self-energy shows that, not too close
to the Fermi energy, this feature corresponds to a band, i.e. to a sol
ution of the Dyson equation omega - epsilon(k) - Re Sigma(k, omega) =
0.