Nonlinear Sigma Models with Compact Hyperbolic Target Spaces
Abstract
We explore the phase structure of nonlinear sigma models with target spaces corresponding to compact quotients of hyperbolic space, focusing on the case of a hyperbolic genus-2 Riemann surface. The continuum theory of these models can be approximated by a lattice spin system which we simulate using Monte Carlo methods. The target space possesses interesting geometric and topological properties which are reflected in novel features of the sigma model. In particular, we observe a topological phase transition at a critical temperature, above which vortices proliferate, reminiscent of the Kosterlitz-Thouless phase transition in the O(2) model [1, 2]. Unlike in the O(2) case, there are many different types of vortices, suggesting a possible analogy to the Hagedorn treatment of statistical mechanics of a proliferating number of hadron species. Below the critical temperature the spins cluster around six special points in the target space known as Weierstrass points. The diversity of compact hyperbolic manifolds suggests that our model is only the simplest example of a broad class of statistical mechanical models whose main features can be understood essentially in geometric terms.
Additional Information
© 2016 The Authors. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. Article funded by SCOAP3. Received: December 10, 2015; Revised: May 14, 2016; Accepted: June 3, 2016; Published: June 23, 2016. J.S., Z.H.S. and S.S.S. would like thank Randall Kamien, Hernan Piragua and Alexander Polyakov for discussions. B.S. would like to thank Hirosi Ooguri for useful discussions, and the Institute for Advanced Study, Princeton University, and the Simons Center for Geometry and Physics for hospitality. B.S. also gratefully acknowledges support from the Simons SummerWorkshop 2015, at which part of the research for this paper was performed. J.S. is supported in part by NASA ATP grant NNX14AH53G. Z.H.S. is supported in part by DOE Grant DOE-EY-76-02-3071. S.S.S. is supported by DOE DE-FG02-05ER46199. B.S. is supported in part by the Walter Burke Institute for Theoretical Physics at Caltech and by U.S. DOE grant DE-SC0011632.Attached Files
Published - art_10.1007_JHEP06_2016_145.pdf
Submitted - 1510.02129v1.pdf
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Additional details
- Eprint ID
- 61426
- Resolver ID
- CaltechAUTHORS:20151022-123136159
- NASA
- NNX14AH53G
- Department of Energy (DOE)
- DOE-EY-76-02-3071
- Department of Energy (DOE)
- DE-FG02-05ER46199
- Walter Burke Institute for Theoretical Physics, Caltech
- Department of Energy (DOE)
- DE-SC0011632
- SCOAP3
- Created
-
2015-10-22Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Walter Burke Institute for Theoretical Physics
- Other Numbering System Name
- CALT-TH
- Other Numbering System Identifier
- 2015-019