Abstract

We investigate the behavior of the rare fluctuations of the free energy in the p-spin spherical model, evaluating the corresponding rate function via the G\"artner-Ellis theorem. This approach requires the knowledge of the analytic continuation of the disorder-averaged replicated partition function to arbitrary real number of replicas. In zero external magnetic field, we show via a one-step replica symmetry breaking (1RSB) calculation that the rate function is infinite for fluctuations of the free energy above its typical value, corresponding to an anomalous, super-extensive suppression of rare fluctuations. We extend this calculation to non-zero magnetic field, showing that in this case this very large deviation disappears and we try to motivate this finding in light of a geometrical interpretation of the scaled cumulant generating function.

Highlights

  • We investigate the behavior of the rare fluctuations of the free energy in the p-spin spherical model, evaluating the corresponding rate function via the Gärtner-Ellis theorem

  • Rivoire [4], Parisi and Rizzo [5,6,7,8], and others [9,10,11] followed this line of thought, providing a bridge between spin glasses and the theory of large deviations, which deals with rare events whose probability decays exponentially in the system size

  • In zero external magnetic field, we show that the 1RSB calculation at finite k produces a scaled cumulant generating function (SCGF) with a linear behavior below a certain value kc; a nice geometrical interpretation of this, dating back to Kondor’s work on the SK model [18], is discussed

Read more

Summary

DISORDERED SYSTEMS AND LARGE DEVIATIONS

The theory of disordered systems has been mainly developed to describe the typical behavior of physical observables. From the disordered systems perspective, most of the standard results of spin glass theory obtained within the replica method concern only the very special limit k → 0, since ftyp = f = ψ (0), whereas to obtain the full form of I (x) that describes arbitrary rare fluctuations of the free energy, one needs to work out the SCGF for finite replica index k. This problem is clearly equivalent to determine the full analytical continuation of the averaged replicated partition. In the Appendix, we discuss the details of the geometrical interpretation of the 1RSB ansatz

LARGE DEVIATIONS OF THE p-SPIN SPHERICAL MODEL FREE ENERGY
From replicas to the scaled cumulant generating function
Rate function and very large deviations
LARGE DEVIATIONS OF THE p-SPIN MODEL IN A MAGNETIC FIELD
DISCUSSION
Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.