Critical energy density of O$(n)$ models in $d=3$
Rachele Nerattini, Andrea Trombettoni, and Lapo Casetti

TL;DR
This study investigates the critical energy densities of O(n) models in three dimensions, comparing them to the Ising model, and finds that their differences are very small for n<8, supporting a conjectured relation between these models.
Contribution
The paper provides new Monte Carlo estimates of critical energy densities for O(n) models in 3D and introduces an interpolation formula quantifying their similarity to the Ising model.
Findings
Critical energy densities for O(2), O(3), and O(4) models are precisely determined.
Differences between O(n) and Ising models' critical energies are less than 1% for n<8.
An interpolation formula shows the small variation of critical energies across different n.
Abstract
A relation between O models and Ising models has been recently conjectured [L. Casetti, C. Nardini, and R. Nerattini, Phys. Rev. Lett. 106, 057208 (2011)]. Such a relation, inspired by an energy landscape analysis, implies that the microcanonical density of states of an O spin model on a lattice can be effectively approximated in terms of the density of states of an Ising model defined on the same lattice and with the same interactions. Were this relation exact, it would imply that the critical energy densities of all the O models (i.e., the average values per spin of the O Hamiltonians at their respective critical temperatures) should be equal to that of the corresponding Ising model; it is therefore worth investigating how different the critical energies are and how this difference depends on . We compare the critical energy densities of O models in three…
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