Fateev-Zamolodchikov and Kashiwara-Miwa models: boundary star-triangle relations and surface critical properties

Details Fateev-Zamolodchikov and Kashiwara-Miwa models: boundary star-triangle relations and surface critical properties Fateev-Zamolodchikov and Kashiwara-Miwa models: boundary star-triangle relations and surface critical properties

1997-03-27

arxiv.org/abs/cond-mat/9703231v1

Nucl Phys B 487(1997)779

Physics

Condensed Matter

Statistical Mechanics

17 pages, no ps figures, latex file

Scientific paper

10.1016/S0550-3213(96)00674-8

The boundary Boltzmann weights are found by solving the boundary
star-triangle relations for the Fateev-Zamolodchikov and Kashiwara-Miwa models.
We calculate the surface free energies of the models. The critical surface
exponent \alpha_s of the Kashiwara-Miwa model is given and satisfies the
scaling relation \alpha_b=2\alpha_s-2, where \alpha_b is the bulk exponent.

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